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112271 | 3701662 | On the Synthesis of Leucic Acid | 396 | 398 | 1,862 | 12 | Proceedings of the Royal Society of London | Edward Frankland | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0082 | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 46 | 949 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112271 | 10.1098/rspl.1862.0082 | http://www.jstor.org/stable/112271 | null | null | Chemistry 2 | 97.967003 | Fluid Dynamics | 1.700396 | Chemistry | [
-38.37351989746094,
-63.83686065673828
] | III .
" On the Synthesis of Leucic Acid .
" By Dr. EDWARD FRANKLAND , F.R.S. Received December 26 , 1862 .
When oxalic ether is mixed with more than its own weight of zincethyl , the temperature of the mixture slowly rises , and soon considerable quantities of gas begin to be evolved , unless the heat be moderated by plunging the vessel , in which the reaction takes place , into cold water .
The gas consists of equal volumes of ethylene and hydride of ethyl ; and as it is the product of a secondary decomposition , its evolution should be avoided as much as possible in the manner just indicated .
The final application of a gentle heat completes the reaction .
The mixture generally continues fluid , but it becomes of a light strawcolour , and of an oily consistency .
On being heated to 130 ?
C. in a retort , no distillate passes over .
If , after cooling , its own volume of water be very gradually added to it , torrents of hydride of ethyl , derived from excess of zincethyl , are evolved .
By subsequent distillation in a water-bath , weak alcohol containing an ethereal oil in solution passes over ; and a further quantity of the oil may be obtained by adding water to the residue in the retort , and continuing the distillation upon a sand-bath .
The ethereal oil was precipitated from the alcoholic distillate by the addition of water , and was added to that which floated upon the surface of the aqueous distillate .
It was then dried over chloride of calcium , and rectified .
A very large proportion of the liquid distilled between 174 ?
and 176 ?
C. , and was collected apart .
Numerous analyses of this liquid agree closely with the formula* C H6 03 .
The liquid is in fact the ethylic ether of an acid possessing the same composition as the leucic acid obtained by Strecker* in acting on leucin by nitrous acid .
Upon the oxalic acid type its formula may be thus expressed : ( C2 H5 I C2 HR C0,0 1 HO C2 H5 0 .
Leucic ether cannot be directly derived from the action of zincethyl upon oxalic ether , but it is produced when water is added to the result of that reaction .
There can scarcely be a doubt that the body first formed is zincoleucic ether , rC , H , 02 115 C2 H , C2( 0 !
ZnO .
C , H O. I have not succeeded in isolating this body ; but , on the assumption of its production , the action of zincethyl upon oxalic ether may be thus formulated : Co 1 C2H , Z CHO+Zn O ZnO C2HO 1C 5 2ZnO r2C2 Zn 110 CH .
5 Zincethyl .
H6 Ethylate of Oxalic ether .
----zinc .
Zincoleucic ether .
In contact with water zincoleucic ether is decomposed with the formation of leuci c ether and hydratend oide of zinc : c2 0 +H } O=C+Z } O. , ZnO ... ... ..| .
H , Zincoleucic ether .
Leucic ether .
Leucic ether is a colourless , transparent , and somewhat oily liquid , possessing a peculiar and penetrating ethereal odour and a sharp taste .
It is insoluble in water , but readily soluble in alcohol or ether .
Its specific gravity is '9613 at 18 ?
'7 C. ; it boils at 175 ?
C. , and distils unchanged .
A determination of the density of its vapour gave the number 5 241 : the above formula , corresponding to 2 vols .
of vapour* , requires the number 5'528 .
When leucic ether is treated with solution of hydrate of baryta , it gradually dissolves even in the cold ; on heating the solution in a water-bath , a liquid having the properties of alcohol distils off ; and on separating the excess of baryta by carbonic acid and filtration , the solution yields , on evaporation , a crystallizable baryta-salt which , after drying at 100 ?
C. , gives on analysis numbers closely corresponding with the formula of leucate of baryta : C2H C2 0 HO KBaO .
Leucate of potash is similarly produced when leucic ether is treated with an aqueous solution of caustic potash .
It separates as a semisolid soap upon the surface of the potash solution , if the latter be concentrated .
All the salts of this acid appear to be soluble in water .
Leucic acid in solution is obtained when dilute sulphuric acid is added to leucate of baryta ; the acid has a sour taste , reddens litmus strongly , and is readily soluble both in water and alcohol .
It can be boiled with water without decomposition , and traces only of the acid distil off with the water .
So far as I have studied its properties , leucic acid thus obtained appears to be identical with that derived from leucin ; but it will be necessary to establish this identity by a more rigorous comparison of the two acids .
The production of leucic acid from oxalic acid , as just described , obviously affords an insight into the molecular constitution of the class of organic acids of which lactic acid is the representative ; I refrain , however , from offering any opinion upon a point which has already given rise to so many hypotheses , until I have completed the study of this reaction , and extended it to other homologous bodies .
|
112272 | 3701662 | On the Artificial Production of Fibrin from Albumen | 399 | 407 | 1,862 | 12 | Proceedings of the Royal Society of London | Alfred Hutchison Smee | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0083 | null | proceedings | 1,860 | 1,850 | 1,800 | 9 | 127 | 3,387 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112272 | 10.1098/rspl.1862.0083 | http://www.jstor.org/stable/112272 | null | null | Chemistry 2 | 36.729803 | Physiology | 30.37082 | Chemistry | [
-59.18621063232422,
-28.093530654907227
] | IV .
" On the Artificial Production of Fibrin from Albumen .
" By ALFRED HUTCHISON SMEE , Junior , Student of St. Bartholomew 's Hospital .
Communicated by W. S. SAVORY , Esq. Received January 15 , 1863 .
The condition in which fibrin exists in the blood and other fluids , and the deviation in quantity and quality in certain cases of disease from that of normal blood , has been to physiologists a subject of great interest .
From the close resemblance of fibrin to albumen , I was induced to undertake a series of experiments , which appear to me to have some value in determining the conditions under which fibrin is derived from albumen , and which have resulted in the discovery of the general principle by which the direct conversion of albumen into fibrin may be effected .
On referring to Lehmann 's ' Chemistry , ' in which the analyses of albumen and fibrin are quoted , it will be observed , on comparing them , that the difference appears to be the substitution of 1'5 part of oxygen per 100 for a similar amount of carbon , hydrogen , nitrogen , sulphur , phosphorus conjoined .
The following are the analyses quoted -Albumen .
Fibrin .
53-5 Carbon ... 52'7 7'0 Hydrogen ... .
69 15'5 Nitrogen ... .
15'4 1'6 Sulphur ... . .
12 0'4 Phosphorus ... .
0'3 22-0 Oxygen. .
23'5 100'0 100'0 The analyses made by Scherer give comparatively the same results .
From these analyses I was induced to make some experiments to endeavour to convert albumen into fibrin by the direct addition of oxygen gas , by which I anticipated that not only might the oxygen be imparted to the albumen , but also that the other elements might be oxidized and carried off .
In my first experiments I used blood from which the fibrin had been carefully whipped during the period of its coagulation , so that the serum might contain as many blood-cells as possible , upon the supposition that the cells would afford a large amount of surface to the action of the gas .
The serum , after being whipped , was permitted to stand for twenty-four hours , that any fibrin which it might contain , and which had not coagulated during the process of whipping , might do so .
The apparatus used in all cases will be easily understood by referring to the annexed diagram .
It consists , first , of a copper flask containing black oxide of manganese , from which the oxygen was slowly given off by the action of heat .
The gas was conveyed thence by tubes into a wash-bottle , B ( containing a dilute solution of potass ) , for the absorption of impurities .
From the bottle B the gas passed into the flask C , which contained the defibrinated blood .
This flask was placed in a vessel ( D ) containing water at a temperature varying between 95 ?
and 100 ?
Fahr. ; and I had no difficulty in preserving that heat continuously by a small gas-flame placed under a sand-bath .
After the gas had escaped from the blood , I generally passed it through a second portion of defibrinated blood contained in another vessel ( E ) .
For all these experiments pig 's blood was invariably chosen , on account of its richness in blood-cells .
My apparatus being ready , and oxygen being slowly given off , the whipped blood , from which every particle of fibrin had been previously removed , was introduced into the flask C. The blood employed was arterial , and not venous .
At first the bright scarlet colour of the blood increased somewhat , but after twelve hours the bright scarlet began to assume more the colour of venous blood : the cells at the same time began to shrivel .
From this time the blood began rapidly to grow darker and darker , when , after thirty-six hours , it was almost black* .
Virchow has shown that , by acting on the haematin contained in the blood-cells by acetic acid , and subsequently boiling it , a substance is formed to which he gives the name of hamine , which he considers to be a product in an intermediate stage between heematin and pigment .
The black substance formed by oxidation may probably be found to be analogous to , if not identical with , Virchow 's haemin .
I found in this blood , at the end of thirty-six hours , small masses , which had , under the microscope , the appearance of fibrin .
A small portion of the same blood as that used in the experiment was set aside till the completion of the experiment , when it was examined , but no fibrin was found .
Likewise in the glass E , although the gas was passed through it without heat , no fibrin was found , proving that temperature had also an effect on the production of fibrin .
This experiment was repeated many times : in all cases the blood assumed the black colour , but I did not invariably find fibrin .
The appearance of fibrin in some cases , and the non-appearance in many others , seemed at first sight to be inexplicable , though I shall be able to demonstrate , in a later portion of this paper , that the result may be explained upon the hypothesis that the alkaline salts were in relative excess in those cases where the fibrin did not appear .
In my next series of experiments , the white of an egg was added to about 4 oz. of the defibrinated blood .
The egg-albumen at first had a tendency to separate and float at the top of the blood-serum , although well agitated together .
In these cases the blood assumed the same dark colour as when it was subjected to experiment alone , though it did not appear until after the serum and egg-albumen had completely coalesced , which took place about ten hours after the subjection to temperatures between 95 ?
and 100 ?
Fahr. , and the action of oxygen gas .
At the end of thirty-six hours , the time when the experiment was stopped , masses of substances were found float* Crawford , about fifty years back , found that , after immersing animals in hot water , no difference could be discerned between arterial and venous blood .
ing , and also adhering to the bottom and sides of the vessel .
These clots were in sufficient quantity to be collected and washed in the filter to free them from blood-cells and other impurities .
The washed portion , under the microscope , had the distinct appearance of fibrin .
In cases where the albumen had not sufficient time to be mingled with the blood , little or no fibrin was formed .
The time occupied for its absorption varied from about ten to twenty hours .
In the experiments which I conducted with albumen alone , I experienced at first some difficulty in obtaining the albumen perfectly pure , on account of the presence of chalazm and other foreign matter .
To obviate this difficulty , I found that , by adding one drop of glacial acetic acid to every white of egg employed , and then by well beating up the albumen , I obtained , on subsequent filtration , a clear solution which gave to litmus-paper a slightly acid reaction .
On placing this transparent albumen in the ordinary apparatus , I found , after the passage of oxygen gas for four hours at the temperature before stated , that fibrin began to be formed .
I found that , by placing coils of platinum wire in the albumen whilst undergoing oxidation , the formation of fibrin was not only greatly facilitated , but its subsequent separation from the rest of the albumen was accomplished with greater ease , as the fibrin hung in threads upon the platinum wire .
When platinized platinum was used , the formation of fibrin , as might have been expected , was slightly improved .
Fibrin produced artificially in these experiments , and especially that formed on platinum wire , had a beautiful and regular arrangement , mostly being deposited in parallel lines .
The fibrin likewise was whiter , and had a more delicate consistence than the common fibrin in blood .
I next tried the effect of adding a small quantity of a strong solution of ammonia to the albumen , which had naturally a slightly alkaline reaction ; and then it was subjected to the influence of a current of oxygen in the same manner as in the preceding experiments .
I found that fibrin was formed to a much smaller extent than when acid albumen was employed .
The ammonia in all cases appears to be driven off to some extent by the oxygen , but was never entirely removed .
The fibrin in this case formed on the surface of the liquid , and did not appear to be dissolved as the experiment was progressing .
It is worthy of particular observation , that fibrin was formed in the liquid which still contained ammonia in appreciable quantity .
My father suggested to me that it would be desirable to try the effect of the decomposition of water by electricity on albumen , as by that process the effect of hydrogen and oxygen in a nascent state is presented to different parts of the same fluid .
For the purposes of this experiment I employed four cells ( of the test-tube form ) of Smee 's battery , in which the negative pole consisted of a platinized platinum wire .
This battery generated a continuous , but feeble , current of electricity ; and the smallest perceptible bubbles were evolved from the platinized platinum wire when in operation for the experiment .
The albumen was placed in the decomposition trough , where a very large positive pole was employed , but a smaller negative one , and the temperature was maintained as in former experiments .
After the passage of the electric current for some time , the positive pole of the decomposition cell was coated with a hard gelatinous mass , which , being immersed in water at 90 ?
Fahr. for a few hours , unravelled itself into long fibres , which had , under the microscope , the appearance of fibrin .
On the negative pole , however , a frothy deposit alone was formed ; but great care must be taken to stop the experiment before the products of the two poles grow together , to which they have a great tendency .
The moment this takes place the albumen begins to coagulate , and in a very short time the whole becomes converted into an almost semisolid mass .
The fibrin is not so perfect when made by this method , and is much more difficult to form than when made from neutral or slightly acid albumen by the ordinary process of oxidation .
In my experiments with egg-albumen to which a solution of potass had been added before it was subjected to the action of oxygen , the temperature ranging between 95 ?
and 110 ?
Fahr. , no fibrin was found when the experiment was stopped .
In one case oxygen was passed through a solution of potass and albumen for three days and nights , and yet not the slightest trace of fibrin was found .
The albumen became of a dark red hue , but two days after the experiment ceased it resumed its normal colour .
A few transparent hard substances were found , insoluble in water and weak acids which had separated from the albumen .
A few other small white substances were noticed , which had all the appearance of carbonate of lime , and which were soluble in acid .
Albumen was then mixed with gastric juice , and kept at the normal temperature of the body for the space of twelve hours , to produce artificial digestion , when it was subjected to experiment .
I should here state that the gastric juice was procured from a dog , which had a fistulous opening made into its stomach by Professor Savory .
All symptoms of inflammation and irritation had fully ceased ; the dog , in fact , was in perfect health , and beginning to get fat , when the gastric juice was procured ; so that the latter must be considered as healthy gastric juice .
From the dog large quantities of gastric juice were obtainable ; and I have to tender my best thanks to Professor Savory for his great kindness in placing whatever I required at my disposal .
After the albumen had been digested for twelve hours and filtered , that the solution might be perfectly clear , it was subjected to the action of oxygen for a few hours , when fibrin was formed , though not in so large an amount as in albumen to which one drop of the glacial acetic acid had been added .
The filaments of the fibrin , however , were of a more delicate constitution .
From a consideration of the above results , I thought that fibrin might be formed from the albumen which , after digestion with gastric juice , had passed through a membrane made of the parchment paper of Messrs. De la Rue and Gains .
In some experiments* to which I had been led from a study of Professor Graham 's elegant researches on dialysis , and which I had formerly been conducting , on the passage of various fluids through membranes , it was observed that albumen , after digestion with gastric juice , dialysed to a certain extent .
Three ounces of albumen were digested for the space of twelve hours , at the temperature of the body .
It was then placed on the dialyser : it should be remarked that gastric juice does not coagulate the albumen during its conversion into albuminose .
The digested albumen was kept for ten hours on the dialyser at the temperature of 98 ?
to 110 ?
Fahr. The water ( one and a half pint ) into which the digested albumen had passed was concentrated at a temperature of not more than 80 ?
Fahr. ; and the concentrated solution being afterwards oxidized , I found that fibrin was formed , notwithstanding the changes it had undergone by digestion , which had rendered it capable of dialysis .
During the process of passing oxygen into albumen , I found that carbonic acid was evolved .
This was ascertained by passing the oxygen , after it had escaped from the albumen , through limewater .
I also found that phosphoric acid was evolved , by subjecting the effluent oxygen to the molybdate-of-ammonia test .
Carbonic acid and phosphoric acid were also found when blood-serum was used , by the same tests as those employed when egg-albumen was the material used for experiment .
In some cases common air was driven through albumen in the place of oxygen , at a temperature between 95 ?
and 110 ?
Fahr. , and then I found the formation of fibrin differed but little from the quantity produced when oxygen alone was used .
To ascertain whether the formation of fibrin was due really to oxygen alone , I tried hydrogen gas in the place of oxygen or common air , and at the same temperature .
When hydrogen was passed into blood-cells sulphur was evolved .
This was detected by passing the hydrogen , after it had traversed the serum , into a solution of leadsalt , and also by suspending over the serum strips of lead paper , when they soon became blackened by the sulphur .
When egg-albumen was employed instead of the blood-serum , sulphur was again detected .
Fibrin was not formed by the action of hydrogen on blood-serum or egg-albumen , although in some cases the hydrogen was passed continuously for forty-eight hours through the fluids .
The action of carbonic acid gas on egg-albumen under the same condition of temperature produces no fibrin , but sulphur was again detected by suspending strips of lead paper over the albumen , which in a few hours became tinged .
The same result was obtained when defibrinated blood was used ; but in this case , in addition to the sulphur , a minute trace of phosphoric acid was found .
Not the slightest trace of fibrin was detected .
I conceived , from the result of my experiments on the oxidation of albumen , that , if oxygen was passed into milk , fibrin might be formed , from the fact that the analyses of albumen of egg , and the casein which the milk contains , differ little from each other , and because the analysis of the milk of an animal , a few days before and after parturition , shows that albumen is found in the place of casein .
On subjecting , however , milk to experiment , no fibrin was found after the lapse of twenty-four hours .
This may be due to either of two causes : first , the casein in the milk may not be in a fit state for undergoing the change before it has been acted on by the various digestive secretions , or , secondly , because in the dilute and fluid state in which it occurs in milk it does not offer sufficient resistance to the passage of the bubbles of oxygen to retain the gas sufficiently long for each bubble to have time to produce an effect .
In all my experiments I have found ( other conditions being equal ) the slower the bubbles passed through the liquid material , and the more viscid the fluid was , the greater was the amount of fibrin produced .
This may possibly in some degree account for the non-formation of fibrin when oxygen was passed through milk .
I tried the effect of oxygen upon fresh grape-juice , but was unable to form any fibrin from it .
Further experiments are required upon various vegetable juices .
I next experimented upon the oxidation of gluten , which was obtained from wheat-flour by the ordinary method .
This was digested in gastric juice for twelve hours , and then filtered .
After the clear liquid had been subjected to oxidation for some hours , small threads of a substance were formed .
When a portion of this was placed under the microscope , no difference could be detected between it and ordinary fibrin .
From these experiments , it seems to me that the following conclusions may be drawn : First , that fibrin is produced by the direct action of oxygen on albumen .
Secondly , that the alkalies and alkaline salts prevent the appearance of fibrin when albumen is acted upon by oxygen .
Thirdly , that the formation of fibrin from albumen is accompanied by the evolution of sulphur , phosphorus , and carbonic acid .
Fourthly , That a temperature ranging between 980 and 110 ?
Fahr. promotes the artificial formation of fibrin .
Fifthly , that the greatest amount of fibrin appears when the albumen is neutral or slightly acid .
Sixthly , that the viscidity of the material employed promotes the formation of fibrin .
Seventhly , that albumen , artificially digested in gastric juice , produces fibrin by its subsequent oxidation , even after dialysis .
Eighthly , that gluten dissolved in gastric juice , and then oxidized at the ordinary temperature , yields fibrin .
The formation of fibrin in the human body , and its relation to albumen , has long been a vexed question .
I venture to put forward these experiments in connexion with this important and interesting inquiry .
|
112273 | 3701662 | Note on the Spectrum of Thallium | 407 | 410 | 1,862 | 12 | Proceedings of the Royal Society of London | William Allen Miller | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0084 | null | proceedings | 1,860 | 1,850 | 1,800 | 4 | 32 | 1,195 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112273 | 10.1098/rspl.1862.0084 | http://www.jstor.org/stable/112273 | null | null | Atomic Physics | 42.578962 | Chemistry 2 | 24.434292 | Atomic Physics | [
11.440389633178711,
-44.149654388427734
] | V. " Note on the Spectrum of Thallium .
' By Professor WILLIAM ALLEN MILLER , M.D. , LL. D. , Treasurer and V.P.R.S. Received January 15 , 1863 .
My friend Mr. Crookes , the discoverer of the new metal thallium* , having kindly put into my hands a small quantity of the metal , which he believes to be chemically pure , I have been enabled to make some experiments upon its spectrum , the results of which may not be without interest to the members of the Royal Society .
Thallium , as is well known , when examined in the usual way by the spectroscope , yields a spectrum of remarkable simplicity , furnishing a single intense green line , the occurrence of which , as is familiar to chemists , led Mr. Crookes to the discovery of the metal , and suggested to him the name by which it is known .
In order to try the effect of a progressively increasing temperature upon the spectrum furnished by the metal and its compounds , the following experiments were made .
Portions of metallic thallium , as well as of an alloy formed by fusing a bead of thallium upon the end of a platinum wire , and portions of the sulphate of the metal were introduced successively , first , into the flame of burning hydrogen , and then into the oxyhydrogen jet , and were in each case viewed by the spectroscope .
As the temperature increased in intensity , the brilliancy of the thallium green line increased also , but no new lines made their appearance .
Two pieces of stout thallium wire were then arranged as electrodes to the secondary wire of an induction coil .
A continuous torrent of sparks was maintained without melting the wires or producing very rapid oxidation , or volatilization of the metal ; the light , however , was much whiter than its ordinary monochromatic character would have led us to expect .
Mr. Crookes , who was with me during the experiments , projected the image of the points by means of a lens upon a distant white screen , when it was at once obvious that the extremities of the spark were of a fine green colour , whilst the flickering luminous arc , which filled up the interval , due chiefly top ignited air , was much whiter .
On viewing the sparks from the induction-coil by the spectroscope , several new lines , independently of well-marked air-lines , made their appearance .
These lines were distinguished from air-lines by the peculiar character which distinguishes most metallic lines , viz. the much greater intensity of their extremities than of their central portions .
Besides the usual intense line in the green , five others were particularly observable : first , a very faint one in the orange ; next , two of nearly equal intensity in the green , more refrangible than TlM , with a third much fainter , these three lines in the green being nearly equidistant ; whilst , 5th , in the blue was a bright well-defined line all these were strong at each extremity and evanescent in the central portions .
The induction-spark of thallium was then observed when produced in a current of hydrogen gas .
The air-lines disappeared , the peculiar lines of hydrogen were very manifest , particularly the line in the red and one of the lines in the blue ; whilst the new thallium lines were preserved , with the exception of the feeblest , though all were reduced in intensity .
Finally , a photographic impression of the thallium spectrum upon collodion was obtained by the method which I have described in a paper communicated to the Royal Society in June last .
An impression extending to about division 154 of the scale then adopted was obtained .
This spectrum contains several very characteristic groups of lines ; it recalls the features of the spectra of cadmium and zinc , and less strongly that of lead .
Measuring by the scale already adopted in my former paper , it is found that there are two strong groups of lines at about 103 and 106 .
At 116 , 121 , and 126 are three groups the first two less intense than the third , which is of about the same strength as the earliest two .
Several feebler pairs of dots follow , and the spectrum terminates rather abruptly with four nearly equidistant groups , commencing respectively at 136 , 141 , 145 , and 151 .
The first of these groups is very strongly marked , the others are fainter , but of nearly equal intensity .
The remarkable way in which a spectrum at low temperatures so simple becomes increased in complexity , both in the visible and in the extra-visible portions , is of high interest considered in relation to the physical cause of these phenomena ; and it is not without interest in a chemical sense , from its bearing upon the view supported by Dumas , that thallium belongs to the alkaline group .
Potassium and sodium exhibit no new lines in the induction-spark , merely a diffuse light filling up the air-lines , and lithium but a single strong group at about 124 .
This physical character , added to the more purely chemical ones of the insolubility of the sulphide , the chromate , the iodide , the sparing solubility of the chloride , the phosphate , the oxalate , the ferrocyanide , the occurrence of a powerfully basic oxide , and of a higher feebly acid oxide , may therefore assist in showing the resemblance of thallium to silver or to lead , which latter metal in density , colour , softness , and external appearance it so closely simulates .
It would be easy to point out other particulars in which the properties of thallium are in strong contrast with those of the alkali metals .
The chemical energy of these metals , lithium , sodium , potassium , rubidium , and caesium , increases in the order mentioned , which is that of their equivalents .
Thallium , with a higher equivalent than any of these , shows a greatly diminished chemical activity .
The metal is readily reduced by zinc from its solutions .
Its oxide , instead of being like that of all the alkalies , excessively deliquescent , is permanent in air , and forms a closely adhering coat like that which is produced upon the surface of zinc or lead , protecting the metal beneath from further change .
In many points the chemical reactions of thallium resemble those of silver , to which metal it is also further approximated by the circumstance that the atomic heat of the metal , like that of silver , is double that of the series to which lead belongs .
Although therefore in other physical properties thallium differs greatly from silver , it seems to be more closely allied to that metal than to any other
|
112274 | 3701662 | Researches on Some of the Artificial Colouring Matters.--No. I. On the Composition of the Blue Derivatives of the Tertiary Monamines Derived from Cinchonine | 410 | 418 | 1,862 | 12 | Proceedings of the Royal Society of London | A. W. Hofmann | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0085 | null | proceedings | 1,860 | 1,850 | 1,800 | 9 | 97 | 3,114 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112274 | 10.1098/rspl.1862.0085 | http://www.jstor.org/stable/112274 | null | null | Chemistry 2 | 85.203854 | Biography | 10.188207 | Chemistry | [
-47.33931350708008,
-57.754356384277344
] | I. " Researches on some of the Artificial Colouring Matters .
No. I. On the Composition of the Blue Derivatives of the Tertiary Monamines derived from Cinchonine .
" By A. W. HOFMANN , LL. D. , F.R.S. Received December 18 , 1862 .
The chemical visitors of the International Exhibition will not easily forget the magnificent collection of products displayed in the French court by M. Menier of Paris .
Among these compounds , equally remarkable for their variety and beauty , the large crystals of cyanine , rivalling in splendour and purity Mr. Nicholson 's acetate of rosaniline , have attracted general attention .
M. Menier , who has produced this new dye on a very large scale , has most liberally placed at my disposal some of the finest of these crystals for examination , hoping that their more minute investigation might perhaps lead to a method of giving solidity to this new colour , which in brilliancy and purity of tint is second to none of the several blues lately derived from coal-tar .
The composition of cyanine and its mode of formation having hitherto remained unknown , I have gladly availed myself of this opportunity of performing some experiments with this interesting compound .
I am sorry to say that , in a practical point of view , these experiments have failed entirely ; but my studies have led me to some observations on this substance which , as a contribution to the history of cyanine , deserve to be recorded , and which I beg leave to communicate to the Royal Society .
The discovery of the blue compounds from chinoline and its homologues dates as far back as 1856 .
In that year Mr. G. Williams engaged in a renewed examination of the base extracted by Rung from coal-tar and obtained by Gerhardt from the alkaloids of the cinchona bark , the identity in composition of which I had established in one of my earlier researches .
Among the numerous compounds of these bases most carefully examined by Mr. G. Williams on this occasion , were also their methylated and ethylated derivatives , one of which , the iodide of methyl-leucolylammonium , I had discovered when studying the action of iodide of methyl upon ammonia and its analogues .
It was in preparing this compound from the chinoline obtained by the distillation of cinchonine , and in separating the ammonium-base corresponding to the iodide by means of oxide of silver , that Mr. Williams first observed the splendid coloration which has led him to the discovery of the new dye now commercially known under the name of cyanine .
Precisely similar phenomena were subsequently ( in 1857 ) observed by M. von Babo , who produced them by treating chinoline with the sulphates of methyl and ethyl , and described the coloured substances thus obtained as methylirisine and ethylirisine .
Mr. Williams was inclined to attribute the formation of the blue compounds , in which he recognized distinctly basic properties , to a process of oxidation ; M. von Babo represents his methyland ethylirisine , although with very great reserve , by the formulae C11HNO , and CliNG Cll H14 2 02 and C13 H18 N2 02 .
No attempt has since been made to establish the composition of these singular compounds by a more minute examination .
In fact several years elapsed without any further notice being taken of them , until the development of the aniline industry revived the memory of these remarkable colour phenomena , which have since attracted the general attention of dyers and printers .
Mr. G. Williams showed that , among the several coloured compounds produced by the action of iodides of alcohol radicals upon chinoline bases , the one obtained by means of iodide of amyl is particularly rich in tinctorial power ; he has given a very interesting account of this new dye , and accurately described the mode of manufacture of this body , which , under the name of cyanine , soon became an article of commerce .
Unfortunately the tint produced by cyanine is less fast than beautifil , and the hopes entertained of the industrial future of the new compound has not been realized ; nevertheless the importance attached by dyers to Mr. Williams 's discovery is well marked by the fact of a gold medal , together with a prize of 10,000 francs , having been proposed for the discovery of a means of rendering stable the beautiful colours dyed by cyanine .
The crystals submitted to me for examination by M. Menier were distinct prisms , sufficiently well formed for crystallographical determinations .
They are at present in the hands of Quintino Sella .
Their substance possesses a beautiful green metallic lustre with a golden tint , by which , as well as by crystalline form , they are readily distinguished from acetate of rosaniline , which they in other respects much resemble .
The crystals are insoluble in anhydrous ether , difficultly soluble in water , but dissolve readily in alcohol .
The solution has a magnificent blue colour , with a coppery iridescence on its surface .
Addition of acids destroys this colour .
Ammonia and the fixed caustic alkalies leave the colour apparently untouched ; but it is now produced by a finely divided deep-blue precipitate suspended in the liquid , which may be filtered off , the filtrate separated from it being colourless .
The green crystals were found to be the iodide of a peculiar basic compound .
The iodine is rather firmly held in this compound ; but it may be precipitated from the alcoholic solution by oxide of silver , and .
exchanged for bromine or chlorine by treatment of this solution with bromide or chloride of silver , when the bromide or chloride corresponding to the iodide are produced .
The analysis of the crystals gave results indicating unequivocally the formula C3o H39 N , I , which received a close confirmation by the examination of a fine platinum-salt crystallizing in rhombic tablets , which is obtained by precipitating the chloride corresponding to the iodide , strongly acidulated with hydrochloric acid , by dichloride of platinum .
Nevertheless slight discrepancies between the theoretical values of the formula and the results obtained led me to assume the existence in the crystals of a compound containing less carbon and hydrogen , indeed of a homologous iodide , C,2 , H , ,3 N2 .
This hypothesis , not countenanced at first by the remarkable constancy which the composition of the iodide presented even after three or four crystallizations , was fully confirmed when the chloride was submitted to a systematic partial precipitation by dichloride of platinum .
After several repetitions of the process , the partially precipitated platinum-salt being decomposed by sulphuretted hydrogen and the chlorides again partially precipitated , two platinum-salts were obtained , one of which , the less soluble one , proved to be the pure platinum-salt corresponding to the iodide with 30 equivalents of carbon , whilst the other one was sufficiently pure to show that it belonged in reality to the homologous iodide with 2 equivalents of carbon less .
The amount of the iodide C28 1H3 N2 I , which contaminated ( if the term may be applied to so beautiful a substance ) the iodide C30 H39 N2 1 , is , however , so small that its presence did not materially influence the analytical results obtained in the further examination of the compound .
The explanation of the formation of the iodide presents no difficulty ; this substance obviously derives from lepidine , C1 , H N , whilst only the slight admixture is due to the presence , in the original bases submitted to the action of iodide of amyl , of a small quantity of chinoline , C9 17N .
In fact Mr. Williams , in describing the preparation of his dye , distinctly states that the chinoline by no means requires to be pure for the purpose .
M. Menier has moreover kindly furnished me with a considerable quantity of the crude material from which the green crystals are obtained .
This proved to be a mixture of several bases , in which the presence of lepidine and chinoline was traced without the slightest difficulty , by the analyses of platinum-salts .
In the genesis of the new iodide two different phases have to be distinguished , viz. , 1 , the transformation of lepidine into iodide of amyllepidyl-ammonium , C , o H9 N+ Cs H , l I= C0 H2 N I ; Lepidine .
Iodide of amyl .
Iodide of amyl-lepidyl-ammonium , the condensation under the influence of potash of two molecules of the compound into one molecule of a higher order , 2(C15120 N I ) +K O=C30 H39 N2 I+KI+H2 O Iodide of amyl-lepidyl-ammonium .
New iodide .
It became indispensable to verify these reactions by the analysis of additional compounds .
The green crystals dissolve with facility in boiling dilute hydriodic acid ; the colourless solution deposits on cooling yellow needles of remarkable beauty , the analysis of which has furnished the values of the formula C30 H4 N I2-= C30 H39 N2 I , H I. 'These crystals are isomeric with iodide of amyl-lepidyl-ammonium , from which , however , they are distinguished by all their properties They dissolve in cold water without decomposition , but on addition of alcohol they immediately assume a blue coloration , the original monacid compound being reproduced .
The same change takes place at 100 ?
; so that in preparing the compound for analysis it was necessary to dry it in vacuo .
In the facility with which the diacid compounds are converted into the monacid salts , this substance resembles rosaniline , which , as I have pointed out in a recent paper , forms likewise colourless acid salts of little stability .
The green iodide dissolves with equal facility in hydrochloric and hydrobromic acid , yielding perfectly colourless solutions , and giving rise to the formation of well-crystallized compounds , which contain , in addition to iodine , respectively bromine and chlorine .
On submitting the green iodide in alcoholic solution to the action of chloride of silver , the whole of the iodine is separated in the form of iodide of silver , a blue solution being obtained from which the monacid chloride crystallizes , on slow evaporation , in green metallustrous sharply-defined prisms of surpassing beauty .
This salt was found to contain Dissolved in hydrochloric acid , tis salt furnished a dicid compound Dissolved in hydrochloric acid , this salt furnished a diacid compound which , on evaporation in vacuo , separates in long straw-coloured needles .
The highly deliquescent character of this substance has hitherto prevented me from analysing it ; but if there was the slightest doubt of this compound having the composition Ca0 Ho N , Cl2=C30 H39 N , CI , H C1 , it would be dispelled by the analysis of a fine-yellow difficultly solu .
ble platinum-salt crystallizing in small well-defined rhombic plates , which falls directly on addition of dichloride of platinum to the alcoholic solution of the diacid chloride , containing a considerable amount of hydrochloric acid , and which , by analysis , was found to be represented by the formula C30 H4o N2 Cl , 2 Pt Cl2 .
The gold-salt is obtained by precipitating the solution of the acid chloride with trichloride of gold , when a yellow , scarcely crystalline precipitate is formed , which , dried in vacuo , contains C30 HI0 N2 C12 , 2Au C13 .
I have , moreover , prepared the monacid bromide , which forms beautiful metal-lustrous prisms easily crystallizable ; the diacid nitrate as a crystalline network , on evaporating a solution of the base in nitric acid in vacuo ; and , lastly , the acid sulpliate , which crystallizes in white , well-formed rhombic tables , very soluble in water , but insoluble in alcohol , by which it is not decomposed like the other diacid compounds .
I have refrained from multiplying the analytical evidences by the minute examination of these salts , because I was happy enough to observe a reaction which supported the interpretation of the results of analysis in an unequivocal manner .
Remembering the simple scission which I had formerly accomplished by exposing the iodide of tetrethylammonium to the action of heat , when the compound splits into iodide of ethyl and triethylamine , I was induced to submit the green iodide to distillation .
The green crystals rapidly fuse into a blue liquid , the surface of which presents a peculiar coppery lustre .
On raising the temperature , decomposition takes place , and in the receiver is condensed a mixture of lepidine and iodide of amyl , the reunion of which to iodide of amyl-lepidyl-ammonium may be prevented by collecting them in hydrochloric acid ; at the same time a gas is evolved , burning with a brilliant flame and readily absorbed by bromine , and which could easily be condensed by passing it through a serpentine surrounded with ice .
I was thus enabled to collect enough of the volatile hydrocarbon to determine its boiling-point , which proved it to be pure amylene .
If the heat be carefully regulated , the amount of charcoal remaining in the retort is comparatively small .
The interpretation of the phenomena observed is given in the following equation : C30 H39 N2 I= 2C1 H9 N+ C5 H , l I+C Hlo Green iodide .
Lepidine .
Iodide of Amylene .
amyl .
Here , again , I have had an opportunity of proving the presence in the crystals of a small quantity of the homologous chinoline compound ; for on submitting , after separating the iodide of 'amyl , the hydrochlorate of the volatilized base to distillation with potassa , and collecting apart the first quantity of the basic liquid which came over with the vapour of water , this substance proved by the platinum determination to be chiefly chinoline , while the portion of the base distilling last proved by the same mode of analysis to be pure lepidine .
The results obtained in these experiments furnish new illustrations of the tendency to molecular accumulation by which the ammonias and their derivatives are distinguished .
Only a few weeks ago I had the honour of submitting to the Royal Society a short account of this class , which is obtained as a secondary product in the manufacture of aniline .
The coloured derivatives of the bases of the chinoline series present in their composition considerable analogy with paraniline .
Aniline series .
C6 H7 N C6 H7N , HC1 Aniline .
Chloride .
C6 HN C6 HN1 HC1 C6 H7 N1 HC1 C6 , H , N C06H7N C6H,7N HC1 Paraniline .
Monacid chloride .
Diacid chloride .
Lepidine series .
C,5 H19 N2H,0 C51 H9 N , HC1 Hydrated oxide of amylChloride .
lepidyl-ammonium .
C15 H , , NH2 01 ?
C1511 N1 C1 C15 H19 N HC1 C15 H19 NH20 C15 H19 N C15 H19N HC1 Free blue base .
Green iodide , monacid .
Yellow iodide , diacid .
I have written the formulae of the coloured compounds so as to bring out their analogy with the paraniline salts-in fact , so as to characterize them as para-compounds of the amyl-lepidyl-ammonium salts , but I am far from attributing to these formulae any other value .
In fact the molecular construction of this new class of compounds remains to be established by further experiments .
The theory which ( in 1852 ) satisfactorily represented the constitution of the nitrogen bases then examined , requires an expansion to include the tinctorial ammonias added to our knowledge during the last decade .
The time for the enunciation of this amplified theory has not yet arrived .
Here only a few experiments may still be mentioned , which were made with the oxide corresponding with the salts described .
The action of oxide of silver upon the iodide dissolved in alcohol liberates the base , which , on evaporation of the alcohol , separates as an indistinctly crystalline deep-blue mass , moderately soluble in water , less soluble in anhydrous ether , easily soluble in alcohol .
Ether precipitates the base from its alcoholic solution ; I have not examined it .
Submitted to distillation , the free oxide gives rise to an oily base , which I naturally expected to be lepidine ; but the experiments which I have hitherto made with this substance appear to negative this assumption .
I have undertaken a more minute examination of the compound , because , if it be different , its study will probably throw some light upon the still uncertain constitution of the tertiary bases of the chinoline series , which I have frequently attempted to decipher .
It remained now only for me to examine the mode of formation of the remarkable compound the nature of which I have endeavoured to clear up .
With this view I have studied the action of iodide of methyl and amyl upon chinoline and lepidine , large quantities of which were kindly placed at my disposal by my friend Mr. David Howard .
The products obtained in this reaction I have not submitted to a minute examination , having satisfied myself that their principal phases are well illustrated by the equations which I have given for the formation of the substances produced by the action of iodide of amyl upon lepidine .
Nor have I followed out in detail the complicated secondary changes , and more especially the generation of the red colouring matter which is abundantly formed in these reactions .
I have nothing to add to the perfect description of these phenomena by the distinguished discoverer of this pigment .
In conclusion I may be allowed to express my best thanks to M. Menier : without the magnificent crystals furnished by his ateliers , I could not have even attempted to clear up this question .
Though proud of her office as guide of industry , science acknowledges without blushing that there are territories on which she cannot advance without leaning on the strong arm of her powerful companion .
Joint labours of this kind cannot fail to seal the pledge of alliance between industry and science .
|
112275 | 3701662 | On Some New Compounds Obtained by Nitrogen-Substitution, and New Alcohols Derived Therefrom | 418 | 420 | 1,862 | 12 | Proceedings of the Royal Society of London | Peter Griess | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0086 | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 29 | 651 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112275 | 10.1098/rspl.1862.0086 | http://www.jstor.org/stable/112275 | null | null | Chemistry 2 | 93.00827 | Astronomy | 4.143056 | Chemistry | [
-47.491188049316406,
-61.782867431640625
] | II .
" On some new Compounds obtained by Nitrogen-substitution , and new Alcohols derived therefrom .
" By PETER GRIESS , Esq. Communicated by Dr. HOFMANN .
Received December 18 , 1862 .
In the beginning of this year ( 1862 ) I pointed out* that diazoamidobenzol , when submitted to the action of nitric acid containing nitrous acid in solltion , is transformed into a new compound according to the equation CI2 H11 N3- , 2H NO +H NO3=2(C6 H1 N2 , 1 NO3 ) +2 H , 0 .
Diazo-amidobenzol .
New compound .
I have now found that this remarkable compound , the nitrate of diazobenzol , can be much more easily produced by the action of nitrous acid upon nitrate of aniline , C6 H7 N , H NO + N , =C,6 H4 , , N,0 +2H2 O. Nitrate of aniline .
Nitrate of diazobenzol .
This process has furnished me a considerable number of similarly conconstituted nitrogen-substituted derivatives , not only of monacid monamines , but also of diamines ; and it is to some of the bodies generated by means of the latter that I beg leave to call the attention of the Royal Society .
If a current of nitrous acid be passed into a cold solution of the nitrate of benzidine , a base which , by the researches of P. W. Hofmann , has been characterized as a well-defined diacid diamine , a new compound is produced , crystallizing from water in white needles , explosive like fulminate of mercury , the composition of which was established by the analysis of a platinum-salt containing C12 HE N , , 2HCl , 2PtC2 , .
The formation of this new substance is illustrated by the following equation : C12 112 N2+ 2H NO3 +2H N2 =C1 H6 N , 2II NO3 +4H 0 .
, _L___ , ?
JtJ Nitrate of benzidine .
New compound .
Of subordinate interest themselves , these substances deserve to be noticed on account of the numerous and often peculiar bodies arising from their decomposition .
Thus the tetrazo-compoundjust described , when boiled with water , splits according to the equation C12 H , N4 , 2H NO3+2H20= C12 H O , + 2N4+2H NO , .
Nitrate of tetrazo-compound , New substance .
The new non-nitrogenous substance thus obtained crystallizes in small sublimable plates .
Both formula and properties characterize it as a compound standing , like phenol , upon the boundary line between acids and alcohols : it furnishes a very extensive series of derivatives , which may be generally represented by the formula 2Phenyl-body 2H -I new compound , IHere I will only mention the chloride corresponding to the new alcohol ( acid ) .
It crystallizes in white volatile plates , which may be readily prepared by heating the above-mentioned platinum-salt with carbonate of sodium .
The reaction takes place at 100 ? .
C12 H N4 , 2H C1 , 2 PtCl C=012 H C12 + 2PtCIl +4 N. In conclusion , I may be allowed to state that nitrate of naphthylamin likewise yields an azo-compound .
This compound , Co1 N HNH N O , when submitted to the action of boiling water , undergoes a transformation analogous to that of nitrate of diazobenzol , C , H , N2 HNO3 + H2 0=C6 0+ 2N+ H NO3 , Nitrate of diazobenzol .
Phenol .
Clo H6 N2 H NO + H20= C H8 0+ 2N+ H NO , .
Nitrate of diazonaphthol .
New compound .
I have not yet analysed this new compound ; but both mode of formation and properties ( it crystallizes in white very fusible needles , possessing the odour of creosote ) leave no doubt that it is the alcohol of the naphthaline series which has so long eluded the researches of chemists .
|
112276 | 3701662 | On the Differential Equations of Dynamics. A Sequel to a Paper on Simultaneous Differential Equations. [Abstract] | 420 | 424 | 1,862 | 12 | Proceedings of the Royal Society of London | George Boole | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 5 | 51 | 1,880 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112276 | null | http://www.jstor.org/stable/112276 | null | 108,807 | Formulae | 92.050249 | Biography | 7.640359 | Mathematics | [
80.21573638916016,
-37.022953033447266
] | III .
" On the Differential Equations of Dynamics .
A sequel to a Paper on Simultaneous Differential Equations .
" By GEORGE BOOLE , F.R.S. , Professor of Mathematics in Queen 's College , Cork .
Received December 22 , 1862 .
( Abstract .
) Jacobi in a posthumous memoir* , which has only this year appeared , has developed two remarkable methods ( agreeing in their general character , but differing in details ) of solving non-linear partial differential equations of the first order , and has applied them in connexion with that theory of the differential equations of dynamics which was established by Sir W. R. Hamilton in the 'Philosophical Transactions ' for 1834-35 .
The knowledge , indeed , that the solution of the equation of a dynamical problem is involved in the discovery of a single central function , defined by a single partial differential equation of the first order , does not appear to have been hitherto ( perhaps it will never be ) very fruitful in practical results .
But in the order of those speculative truths which enable us to perceive unity where it was unperceived before , its place is a high and enduring one .
Given a system of dynamical equations , it is possible , as Jacobi had shown , to construct a partial differential equation such that from any complete primitive of that equation , i. e. from any solution of it involving a number of constants equal to the number of the independent variables , all the integrals of the dynamical equation can be deduced by processes of differentiation .
Hitherto , however , the discovery of the complete primitive of a partial differential equation has been supposed to require a previous knowledge of the integrals of a certain auxiliary system of ordinary differential equations ; and in the case under consideration that auxiliary system consisted of the dynamical equations themselves .
Jacobi 's new methods do not require the preliminary integration of the auxiliary system .
They require , instead of this , the solution of certain systems of simultaneous linear partial differential equations .
To this object , therefore , the method developed in my recent paper on " Simultaneous Differential Equations " ( Philosophical Transactions for 1862 ) might be applied .
But the systems of equations in question are of a peculiar form .
They admit , in consequence of this , of a peculiar analysis .
And Jacobi 's methods of solving them are in fact different from mine , though connected with it by remarkable relations .
He does indeed refer to the general problem of the solution of simultaneous partial differential equations , and this in language which does not even suppose the condition of linearity .
He says , " Non ego hic immorabor queestioni generali quando et quomodo duabus compluribusve sequationibus differentialibus partialibus una eademque functione satisfieri possit , sed ad casum propositum investigationem restringam .
Quippe quo preeclaris uti licet artificiis ad integrationem expediendam commodis .
" But he does not , as far as I have been able to discover , discuss any systems of equations more general than those which arise in the immediate problem before him .
It is only very lately that I have come to understand the nature of the relation between the general method of solving simultaneous partial differential equations , published in my recent memoir , and the particular methods of Jacobi .
But in arriving at this knowledge I have been led to perceive how , by a combination of my own method with one of those of Jacobi , the problem may be solved in a new and perhaps better , certainly a remarkable way .
This new way forms the subject of the present paper* .
Before proceeding to explain it , it will be necessary to describe Jacobi 's methods , to refer to my own already published , and to point out the nature of the connexion between them .
The system of linear partial differential equations being given , and it being required to find a simultaneous solution of them , Jacobi , according to his first method , transforms these equations by a change of variables ; he directs that an integral of the first equation be found ; he shows that , in virtue of the form of the equations and the relation which connects the first and second of them , other integrals of the first equation may be derived by mere processes of differentiation from the integral already found ; and he shows how , by means of such integrals of the first equation , a common integral of the first and second equations of the system may be found .
This common integral is a function of the known integral and certain variables , and its form is obtained by the solution of a differential equation between two variables-a differential equation which is in general non-linear , and of an order equal to the total number of integrals previously found .
An integral of the first two equations of the given system having been obtained , Jacobi shows that by a second process of derivation , followed by the solution of a second differential equation , an integral which will satisfy simultaneously the first three equations of the system may be found ; and thus he proceeds by alternate processes of derivation and integration till an integral satisfying all the equations of the given system together is obtained .
In these alternations , it is the function of the processes of derivation to give new integrals of the equations already satisfied ; it is the function of the processes of integration to determine the functional forms by which the remaining equations may in their turn be satisfied .
Jacobi 's second method does not require a preliminary transformation of the equations ; but the process of derivation , by which from an integral of the first equation other integrals are derived by virtue of the relation connecting the first and second equations , is carried further than in his first method .
It is indeed carried on until no new integrals arise .
The difference of result is , that the common integral of the first and second partial differential equations is determined as a function solely of the integrals known , and not as a mixed function of integrals and variables .
But its form is determined , as before , by the solution of a differential equation .
All the subsequent processes of derivation and integration are of a similar nature .
On the other hand , the method of my former paper applied to the same problem leads , by a certain process of derivation , to a system of ordinary differential equations equal in number to the number of possible integrals , and , without being individually exact , susceptible of combination into exact differential equations .
The integration of these would give all the common integrals of the given system .
All these methods possess , with reference to the requirements of the actual case , a superfluous generality .
A single common integral of the system is all that is required .
Now the chief result to be established in this paper is the following .
If , with Jacobi , according to his second method , we suppose one integral of the untransformed first partial differential equation to be found , if by means of this we construct according to a certain type a new partial differential equation , if to the system thus increased we apply the process of my former paper , continually deriving new partial differential equations until , no more arising , the system is complete , then , under a certain condition hereafter to be explained , a common integral of all the equations of the complete system , and therefore of the original system which is contained in it , may be found by the integration of a single differential equation susceptible of being made integrable by means of a factor .
But if the condition referred to is not satisfied , a new integral of the first partial differential equation must be found and the process repeated , with the certainty that sooner or later it will succeed .
As soon , then , as the condition is satisfied , a solution not , as by Jacobi 's methods , first of two of the partial differential equations of the given system , then of three , and so on , but of all at once , is obtained ; and this solution is obtained , not as in my former process , by the solution of a system of equations reducible to the exact differential form , but by that of a single differential equation reducible to that form .
The condition in question is grounded on the theoretical connexion which exists between the process of derivation of partial differential equations involved in my former method , and the process of derivation of integrals involved in Jacobi 's methods .
In the actual problem , and in virtue of the peculiar form of the partial differential equation given , these two processes are coordinate .
If each be carried to its utmost extent , then to each new partial differential equation arising from the one will correspond a new integral ( of the first partial differential equation ) arising from the other .
The theory now to be developed is founded upon the inquiry whether it is possible to satisfy the completed system of partial differential equations by a function of the completed system of the Jacobian integrals , i. e. to determine a common integral of the completed series of equations as a function of the completed series of integrals of the first equation .
The reader is reminded that by the completed series of integrals is meant , not all the integrals of the first partial differential equations that exist , but all that arise from a certain root integral by a certain process of derivation , together with the root integral itself .
Now the answer here to be established to this inquiry is the following .
The first of the partial differential equations necessarily will , and others may , be satisfied by the proposed function irrespectively of its form .
If the number of equations of the completed system which is not thus satisfied is odd ( this is the condition in question ) , the form of the function which will satisfy all is determinable by the solution of a single differential equation of the first order , capable of being made integrable by means of a factor .
Although the direct subject of this paper is the solution of partial differential equations of the first order , I wish it rather to be received as a slight contribution to that theory of the dynamical equations which was first published in the Philosophical Transactions , and which sug , gested to Jacobi the line of investigation which I here only seek to pursue a little further ,
|
112277 | 3701662 | On the Absorption of Gases by Charcoal.--No. I. [Abstract] | 424 | 426 | 1,862 | 12 | Proceedings of the Royal Society of London | Angus Smith | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 38 | 534 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112277 | null | http://www.jstor.org/stable/112277 | null | null | Thermodynamics | 40.947208 | Fluid Dynamics | 23.902213 | Thermodynamics | [
-22.0883846282959,
-46.36018371582031
] | " On the Absorption of Gases by Charcoal.-No .
I. " By Dr. R. ANGUS SMITH , F.R.S. Received December 27 , 1862 .
( Abstract .
) The following is a summary of the author 's observations:1 .
Charcoal absorbs oxygen co as to separate it from common air , or from its mixtures with hydrogen and nitrogen , at common temperatures .
2 .
Charcoal continues the absorption of oxygen for at least a month , although the chief amount is absorbed in a few hours , sometimes in a few seconds , according to the quality of the charcoal .
3 .
It does not absorb hydrogen , nitrogen , or carbonic acid for the same period .
4 .
Although the amount absorbed is somewhat in the relation of the condensibility of the gases by pressure , this is not the only quality regulating the absorption , of oxygen at least .
5 .
When it is sought to remove the oxygen from charcoal by warmth , carbonic acid is formed , even at the temperature of boiling water , and slowly even at lower temperatures .
6 .
Charcoals differ extremely in absorbing power , and in the capacity of uniting with oxygen , animal charcoal possessing the latter property in a greater degree than wood-charcoal .
7 .
Nitrogen and hydrogen , when absorbed by charcoal , diffuse into the atmosphere of another gas with such force as to depress the mercury three-quarters of an inch .
8 .
Water expels mercury from the pores of charcoal by an instantaneous action .
9 .
The action of porous bodies is not indiscriminate but elective .
Theoretical Considerations .
1 .
The elective nature of porous bodies may be closely allied to three properties:a .
The condensibility of the gases .
b. The attraction and perhaps inclination to combine .
c. The capacity of combination .
2 .
In either case the attraction which results in condensation of the gas is exercised at distances greater than the distances of atoms or molecules in combination .
3 .
The gases in porous bodies lie in strata , the outside and more distant being less attracted than the atoms nearer the solid body .
4 .
We cannot separate chemical from physical attraction ; but attraction may exist without its ultimate result ( combination ) , which is distinctly chemical .
5 .
It is exceedingly probable that as physical attraction moves onwards to chemical combination , it produces the phenomena which have been attributed to so-called masses .
Chemical affinity is supposed to involve an attraction which is purely chemical ; we have no proof of any such attraction as a separate power , we have only a proof of the combination .
Attraction may exist without the capacity of combining chemically , or , in other words , without chemical affinity .
Chemical affinity ( a very inappropriate term ) is only known by combination ; the previous attraction has never yet been shown to be of two kinds ; and it seems more in accordance with Nature to diminish than to increase the number of original powers .
|
112278 | 3701662 | On the Embryogeny of Comatula rosacea (Linck). [Abstract] | 426 | 428 | 1,862 | 12 | Proceedings of the Royal Society of London | Wyville Thomson | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 35 | 1,164 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112278 | null | http://www.jstor.org/stable/112278 | null | null | Paleontology | 70.559516 | Biology 3 | 14.504771 | Paleontology | [
-63.10614776611328,
26.069316864013672
] | " On the Embryogeny of Comatula rosacea ( Linck ) .
" By Professor WYVILLE THOMSON , LL. D. , F.R.S , E. , M.R.I.A. , F.G.S. &c. Communicated by Professor HUXLEY .
Received December 29 , 1862 .
( Abstract .
) After briefly abstracting Dr. W. Busch 's description of the early stages in the growth of the young of Comatula , the author details his own observations , carried on during the last four years , on the development and subsequent changes of the larva .
After complete segmentation of the yelk , a more consistent nucleus appears within the mulberry mass still contained within the vitelline membrane .
The external more transparent flocculent portion of the yelk liquefies and is absorbed into this nucleus , which gradually assumes the form of the embryo larva , a granular cylinder contracted at either end and girded with four transverse bands of cilia .
This cylinder increases in size till it nearly fills the vitelline sac , gradually increasing in transparency , and ultimately consisting of delicately vacuolated sarcode , the external surface transparent and studded with pyriform oil-cells , the inner portion semifluid and slightly granular .
The vitelline membrane now gives way , and , usually shortly after the escape of the larva into the water , the third ciliated band from the anterior extremity arches forwards at one point ; and in the space thus left between it and the fourth band , a large pyriform depression indi cates the position of the larval mouth .
At the same time a small round aperture , merely separated from the posterior margin of the mouth by the last ciliated band , becomes connected with the mouth by a short loop-like canal passing under the band , and fulfils the function of an excreting-orifice .
A tuft of long cilia , which have a peculiar undulatory motion , is developed at the posterior extremity of the body .
The larva now increases rapidly in size , assuming somewhat the form of a kidney bean , the mouth answering in position to the hilum .
It swims freely in the water , with a swinging semirotatory motion , by means of its ciliated bands and posterior tuft of cilia .
Shortly after the larva has attained its definite independent form , ten minute calcareous spicula make their appearance , imbedded within the external sarcode-layer of the expanded anterior portion of the larva .
The ten spicula are arranged in two transverse rings of five , the spicula of the anterior row symmetrically superposed on those of the posterior .
By the extension of calcareous network , these spicula rapidly expand into ten plates , which at length form a trellis enclosing a dodecahedral space , open above and below , within the anterior portion of the zooid .
Simultaneously with the appearance of these plates , a series of from seven to ten calcareous rings form a chain passing from the base of the posterior row of plates backwards , curving slightly to the left of the larval mouth , and ending by abutting against the centre of a large cribriform plate , which is rapidly developed close to the posterior extremity of the larva .
Delicate sheaves of anastomosing calcareous trabeculae shortly arise within these rings , and the series declares itself as the jointed stem of the pentacrinoid stage , the basal and first interradial plates of the calyx being represented by the already formed casket of calcareous network .
The skeleton of the Crinoid is thus completely mapped out within the body of the larva , while the latter still retains its independent form and special organs .
Within the plates of the calyx of the nascent Crinoid two hemispherical or reniform masses may now be detected , -one superior , of a yellowish , subsequently of a chocolate colour ; the other inferior , colourless and transparent .
The lower hemisphere indicates the permanent alimentary canal of the Crinoid , with its glandular follicle ; the upper mass originates the central ring of the ambulacral system , with its craca passing to the arms .
The body of the Crinoid is , how ever , at this stage entirely closed in by a dome of sarcode , forming the anterior extremity of the larva .
After swimming about freely for a time , averaging from eight hours to a week , and increasing rapidly in size till it has attained a lengh of from 1 to 2 millims. , the larva becomes sluggish , and its form is distorted by the growing Crinoid .
The mouth and alimentary canal of the larva disappear , and the external sarcode-layer subsides round the calcareous framework of the included embryo , forming for it a transparent perisom .
The stem now lengthens by additions of trabeculm to the ends of the joints .
The posterior extremity dilates into a disk of attachment .
The anterior extremity becomes expanded , then slightly cupped ; the lip of the cup is divided into five crescentic lobes corresponding to the plates of the upper ring ; and finally five delicate tubes , ceca from the ambulacral circular canal , are protruded from the centre of the cup , the rudiments of the arms of the Pentacrinoid .
At some stage during the progress of these later changes the embryo adheres , and at length becomes firmly cemented to some permanent point of attachment .
The author states his views as to the morphological and physiological relations of the larval zooid .
He believes that all the peculiar independently organized zooids developed from the whole or from a part of the segmented yelk in the Echinoderms , and which form no stage in the development of the perfect form of the species , must be regarded as assimilative extensions of sarcode , analogous in function to the embryonic absorbent appendages in the higher animals .
For such an organism the term " pseudembryo " is proposed .
In the Echinoderm subkingdom , although constructed apparently upon a common plan , these pseudembryos present considerable range of organization , from a somewhat complex zooid provided with elaborate natatory fringes , with a system of vessels which are ultimately connected with the ambulacral vascular system of the embryo , with a well-developed digestive tract , and in some instances with special nervous ganglia , to a simple layer of absorbent and irritable ' sarcode which invests the nascent embryo .
The pseudembryo of Comatula holds an intermediate position .
It resembles very closely in external form and in subsequent metamorphosis the " pupa stage ?
' of the Holothuridse , the great distinction between them being that in the Holothuridee the pupa has already passed through the more active " Auricularian " stage , while the analogous form in Comatula has been developed directly from the egg .
|
112279 | 3701662 | On Some Compounds and Derivatives of Glyoxylic Acid. [Abstract] | 429 | 430 | 1,862 | 12 | Proceedings of the Royal Society of London | Henry Debus | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 2 | 32 | 602 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112279 | null | http://www.jstor.org/stable/112279 | null | 108,805 | Chemistry 2 | 96.012258 | Biography | 2.205966 | Chemistry | [
-41.94752883911133,
-56.98710250854492
] | I. " On some Compounds and Derivatives of Glyoxylic Acid .
" By HENRY DEBUS , Ph. D. , F.R.S. Received December 31 , 1862 .
( Abstract .
) Glyoxylic acid contains one atom of oxygen less than oxalic acid , and may be considered as glycolic acid minus two atoms of hydrogen .
It therefore bears to these two acids the same relation that oil of bitter almonds does to benzoic acid and benzylic alcohol .
On another occasion* it has been shown to possess other properties in common with hydride of benzoyl .
Dilute nitric acid , for instance , oxidizes glyoxylic acid to oxalic acid , and hydrate of potash converts it into glycolic acid and oxalic acid .
The same reagents produce with oil of bitter almonds benzoic acid , benzoate of potash , and benzylic alcohol .
C,2203 + HNO3 = C , H2 04 +H NO , , Glyoxylic acid .
Oxalic acid .
C7H60 + HNO = C7H602 + HNO , , Hydride of Benzoic acid .
benzoyl .
2C2 , H203 +3KHO = C2 , H3KO+C , K,0 , 4 2H,0 , Glycolate of Oxalate of potash .
potash .
2(C7 H60 ) + KHO = C7H , KO , +C I-O .
Hydride of Benzoate of Benzylic benzoyl .
potash .
alcohol .
In the memoir of which this is an abstract certain properties of glyoxylic acid are described which still more intimately connect this body with the class of the aldehydes , so as to leave no doubt as to its position in the system of organic substances .
Glyoxylates and sulphites have a strong tendency to combine .
Glyoxylic acid expels one-half only of the sulphurous acid from a given quantity of sulphite of soda , and forms the substance represented by the formula Na HS3+ C , H Na O3 ; an excess of sulphurous acid , on the other hand , expels one-half of the acid in glyoxylate of lime , producing Ca HS 03 + C , H Ca 0 , .
These salts crystallize well and are very stable .
Sulphuretted hydrogen and glyoxylate of lime exchange sulphur and oxygen , water and a new compound , C , 2 Ca 5 } +31H30 , being the result .
The sulphur acid in the latter salt seems to bear to glyoxylic acid a relation similar to that in which triacetic acid stands to acetic acid .
Glyoxylic acid itself is decomposed by sulphuretted hydrogen , a new crystallizable acid being produced .
Ammonia forms definite compounds with glyoxylates .
The following of them were investigated:--two bodies formed from NH , and glyoxylate of lime , 3(C H Ca O ) , 2N H , , and 3 ( C , H Ca 3 ) , 2N H , + H[ 0 , one silver and one lead compound .
These derivatives are very unstable , but the products of their decomposition could not be obtained in a pure state .
Hydrogen in statu nascendi combines with glyoxylic acid and converts it into glycolic acid , C,2H,03 + H , = C , H,40 Glycolic acid .
This transformation was brought about by dissolving zinc in dilute glyoxylic acid .
Glycolic acid , glyoxylic acid , and oxalic acid therefore possess , as regards composition and some other essential properties , the same connexion as ethylic alcohol , acetic aldehyde , and acetic acid .
The differences between the two series arise from the greater number of oxygen-atoms in the molecules of the first three bodies .
|
112280 | 3701662 | On the Telescopic Appearance of the Planet Mars | 431 | 437 | 1,862 | 12 | Proceedings of the Royal Society of London | John Phillips | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0091 | null | proceedings | 1,860 | 1,850 | 1,800 | 7 | 69 | 2,137 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112280 | 10.1098/rspl.1862.0091 | http://www.jstor.org/stable/112280 | null | null | Astronomy | 42.3446 | Optics | 24.43392 | Astronomy | [
74.84593200683594,
20.47704315185547
] | II .
" On the Telescopic Appearance of the Planet Mars .
" By JOHN PHILLIPS , M.A. , LL. D. , F.R.S , F.G.S. , Professor of Geology in the University of Oxford .
Received February 5 , 1863 .
Notwithstanding the descriptions and drawings of Mars , for which we are indebted to eminent observers* , there remains much uncertainty as to the permanent boundaries of the bright and shady parts of the planet , to which respectively , on a first view , we attach , perhaps too readily , the idea of land and seas .
The extremely variable aspects under which this planet appears in its excentric orbit , the axis being inclined more than 30 ?
to the ecliptic , the different regions very unequally presented to incident light , and very unequally influenced by vicissitudes of heat and cold , may account for much of the uncertainty .
Other difficulties arise when the work of different instruments is compared ; for it is established that reflectors will on the whole give the best results for colour , while achromatics of fine quality discover more of detail than instruments of less perfect definition .
The author having devoted some evenings between the 27th of September and 13th of December 1862 to the examination of Mars with a 6-inch achromatic by Cooke , equatorially mounted , and moved by clockwork , at Oxford , presented to the Society some results of these observations combined with others , also made with achromatics , by Mr. Grove , Mr. Main , and Mr. Lockyer .
These various observations , made entirely without concert , were rendered comparable by a calculated reduction of each to the longitude on Mars corresponding to the epoch of each , according to one standard .
[ Tables of these reductions were given in the paper .
] The sketches were then arranged on sheets in the order of the computed longitudes ; and , in addition , two globes were exhibited , on one of which the main results of the author 's observations were drawn , the data for the other being supplied by Mr. Lockyer 's sketches .
He was also aided in the explanations by large drawings made with reflectors by Mr. De la Rue and Mr. Nasmyth .
From the author 's sketches , three , representing opposite hemispheres , and one intermediate quadrature , have been selected for engraving , -one central to the assumed meridian of 0 ?
or 360 ?
, the others to the meridians of 90 ?
and 180 ?
nearly .
See figs. 1 , 2 , 3 .
Fig. 1.-Mars as seen on the 27th of September and on several other occasions till the 13th of December .
( Longitude 0 ? .
) On considering the surface of the planet , either as seen in the telescope , or delineated on paper , we feel in some doubt as to the meaning of what we see .
Are the bright parts ( often seen of a red tint ) land , the darker parts ( often appearing of a greenish grey ) water ?
or , as in the moon , are the reflecting powers of different parts of a dry surface very unequal ?
Is there any considerable change in the aspect of the masses or boundaries between one epoch and another , so as to indicate atmospheric vicissitudes like those on Jupiter and our own planet ?
Taking the latter question first , the author found , on the experience of his observations during 74 days , that no material change took place in the main and prominent features about the longitude which he marks 0 ? .
Not that after this considerable interval the appearances remained exactly as at first : that was not , and could not be Fig. 2.-The appearance of Mars at longitude 90 ?
, with long oblique ridges south of the great boundary , and nearly or quite running into the northern land , here less broad than in fig. 3 : seen November 11th .
Fig. 3.-The llemisphere of Mars , opposite to fig. 1 : seen October 15th and 16th .
With a specially dark band expected to be the case , after the planet had increased his distance from the earth to nearly double that when the observations began .
Adding to his own the experience of Mr. Lockyer , whose observations began 35 days earlier , this inference , of permanence in the main boundaries of lights and shades , is extended to above 100 revolutions of Mars ; and on comparison of these with the earlier sketches of Madler , Herschel , Jacobs , and De la Rue , the conclusion appears to embrace the whole series of more than thirty years .
The author regards as one of the main features very firmly defined in the late opposition , the broad white or rather reddish band which from about 65 ?
of north latitude ( the north pole being invisible in these observations ) spreads up into large bright cloudlike prominences toward and beyond the equator , and retires into one principal and several smaller bays toward the pole .
From this bright space , which in many parts is sharply defined , a broad dusky tint spreads toward the south , partially relieved by half-lighted expansions with shades of various depths between .
The south pole itself is surrounded ( excentrically as it appears ) by a bright white mass , obviously glittering in the telescope .
This is believed to be snow ; and the effect of its whiteness is increased in most parts of its circumference by the contrast of a dark ring round it , which expands here and there into broader spaces .
Thus a great part of the northern area appeared in the late opposition bright , and often reddish , as if it were land , while a great part of the southern area was of the grey hue which is considered to indicate water , but relieved by various tracts of a tint more or less approaching to that of the brighter spaces of the northern hemisphere .
The principal boundary of light and shade , for the most part very well defined , ran obliquely across the equator of Mars , so as to reach latitudes from 20 ?
to 30 ?
north and south of that line .
This may perhaps be understood by the drawings selected for illustration , especially if compared with an orthographic projection of the latitudes* .
( Still better by means of the globes which accompanied the communication , constructed by the author , one from his own sketches , the other from those of Mr. Lockyer .
) Allowing the white spaces to be land , which reflects light as the moon in opposition , it seems a natural supposition that the shady spaces should be called sea ; and this may be supported by the obvious requirement of water somewhere on Mars , to agree with the alternate gathering and melting of the snow round the poles .
Still , every observer remarks no small resemblance of some of these shady tracts with particular parts of the unequally tinted grey surfaces of the moon .
A positive proof of ocean on the disk of Mars would be afforded by the star-like image of the sun reflected from the quiet surface* , or the more diffused light thrown back from the waves ; but nothing of this sort has been placed on record , nor is there such a variation in the appearance of these spaces from the centre toward the edges as to give any special reason for thinking them occupied by water .
Atmospheric vicissitudes , however , appear to be recognized in the somewhat variable aspect of many portions of the grey spaces ; for these , thougli not much changed in the situation of the masses of light or shade , are sufficiently inconstant in.their shapes and details to suggest the idea of a vaporous envelope , brooding over and about some parts more than others , and variable from one epoch to another .
The drawings of Mr. Lockyer supply the best evidence of these variations ; for Professor Phillips , except on a few occasions , confined his attention chiefly to the stronger and apparently more settled boundaries of light and shade .
The tints on the body of Mars were observed by each of the gentlemen named , but with different results .
To Mr. Nasmyth , with a large reflector , the 'land ' appeared of a decidedly red tint , the 'water ' green .
The 'land ' appeared red in some parts , but bright and almost silvery in other parts , to Professor Phillips , looking through his achromatic , which also showed the ' water ' of a grey or greenish tint .
No redness appeared in Mr. Lockyer 's instrument , which , like many others of excellent quality for astronomical research , is intentionally C over-corrected .
' Mr. Nasmyth saw the snow-patch on the south pole so distinctly bordered , as to give him the impression of its having a cliffboundary .
The south snow-patch did not appear to him to agree with the south pole of the planet , but , on the contrary , to be considerably excentric to it ; and he supposed this to be due to the relative distribution of land and water , influencing the position of the centre of greatest cold .
Only a faint glimmering of the snowy surfaces round the north pole was seen by any observer .
On the whole , the author of this paper concluded that , over a permanent basis of bright and dusky tracts on the surface of Mars , a variable envelope gathers and fluctuates , partially modifying the aspect of the fundamental features , and even in some cases disguising them under new lights and shades , which present no constancy , -a thin vaporous atmosphere probably resting on a surface of land , snow , and water .
Addendum .
Since the reading of the paper the author has been enabled , by the kindness of the Earl of Rosse , to examine a series of sketches of Mars during the late opposition , from the great telescopes at Birr .
These drawings , six in number , were made on July 22 , Sept. 14 , Sept. 16 , Oct. 6 , Oct. 29 , and Nov. 6 .
They confirm in a remarkable manner the conclusions already presented by the author , and suggest some interesting questions for further observation and study .
On the 22nd of July the southern snow was a large patch , meeting the limb by its diametral line .
It must then have had a radius of 500 miles at least : in the later observations it was reduced to less than half this measure .
One of the drawings nearly corresponds to longitude 180 ?
on the author 's scale , and represents the specially dark short band which distinguishes that aspect of the planet ( fig. 3 ) .
Two correspond nearly to fig. 1 , and contain the remarkable deep angular bay which extends so far towards the north pole .
In these and the re maining three drawings , general resemblances and special differences appear on comparison with the sketches of Prof. Phillips and Mr. Lockyer .
The differences affect principally the grey southern parts , and are remarkable enough to justify serious doubts whether any of our drawings of those parts are much to be trusted as representing permanent physical boundaries .
Nor should this be thought surprising ; owing to the high inclination of the axis of Mars to the plane of his orbit , the regions round each pole are presented alternately to the sun through periods somewhat less than our whole year .
The effect is seen in the vast outspread of snows round the cold pole , and the contraction of those white sheets to a small glittering ellipse round the warm pole .
The enormous transfer of moisture from one hemisphere to the other while the snows are melting round one pole and growing round the other must generate over a great part of the planet heavy storms and great breadths of fluctuating clouds , which would not , as on the quickly rotating mass of Jupiter , gather into equatorial bands , but be more under the influence of prominent land and irregular tracts of ocean .
|
112281 | 3701662 | On Thallium. [Abstract] | 437 | 440 | 1,862 | 12 | Proceedings of the Royal Society of London | William Crookes | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 40 | 1,030 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112281 | null | http://www.jstor.org/stable/112281 | null | 108,794 | Chemistry 2 | 57.385586 | Chemistry 1 | 20.336219 | Chemistry | [
-30.001174926757812,
-70.38170623779297
] | " On Thallium .
" By WILLIAM CROOKES , Esq. Communicated by Professor STOKES , Sec. R.S. Received February 5 , 1863 .
( Abstract .
) After discussing the occurrence and distribution of the new metal in different parts of the globe , the author proceeds to describe the method adopted by him for extracting it from its ore .
Thalliferous pyrites is distilled at a bright red heat , in quantities of about 1 cwt .
at a time , in cast-iron retorts .
The resulting sulphur , varying from 13 to 17 per cent. of the pyrites taken , is then dissolved in aqueous caustic soda , which leaves the sulphide of thallium as an insoluble black precipitate ; this is filtered off , dissolved in acids , and the thallium precipitated in the form of iodide .
This is then converted into sulphate , and the metal reduced from the solution by electrolysis .
It is obtained in the coherent form by fusion under cyanide of potassium .
The physical characteristics of thallium are then described .
In appearance it most resembles tin and cadmium , but has a distinct colour of its own ; it has a brilliant metallic lustre , and is susceptible of taking a very high polish ; it oxidizes in the air with almost the rapidity of an alkaline metal , but when coated with oxide , the metal may be freely handled and exposed to the air with scarcely any further change .
An oxidized surface applied to the tongue is very biting and caustic , and has a sweetish metallic taste .
It is the softest known metal admitting of free exposure to the atmosphere , being scratched by soft lead with the greatest ease .
It makes a dark blue mark upon paper , rapidly turning yellow , which in the course of a few hours nearly fades out , but can be restored with sulphide of ammonium .
It has little tenacity , is very malleable , and may be readily pressed into wire .
The specific gravity of thallium varies from 11881 to 11'91 , and it is probably capable of still greater condensation .
When freshly prepared , thallium wire is perfectly amorphous , but when kept in water it gradually assumes a superficial crystalline appearance : this effect is immediately produced when thallium in wire , ingot , or plate , tarnished or clean , is boiled in water .
Its melting-point is 550 ?
F. , being between bismuth and lead , and the metal does not become pasty before undergoing complete fusion .
Two pieces of clean metal weld together by pressure in the cold .
It begins to volatilize at a red heat , and boils below a white heat ; it may be distilled in a current of hydrogen .
It is a pretty good conductor of heat and electricity , and stands electro-chemically very near cadmium .
It is strongly diamagnetic , ranking in this respect near bismuth .
The alloys which thallium forms with different metals are next described .
Further details are given respecting the spectrum of thallium : the characteristic green line is perfectly single under a very high magnifving power and after refraction through nine heavy glass prisms ; and no new lines make their appearance at the temperature of the oxyhydrogen blowpipe , -although , with the electric spark , Dr. Miller has shown that several new lines come into existence .
The delicacy of the optical test for thallium is roughly estimated , the 5oIo 00oth of a grain being easily perceptible .
The atomic weight of thallium is given as 203 , being the mean of five experiments .
The author states , however , that this is not to be regarded as a final result .
The chemical properties of thallium are next described .
It does not decompose water even at the boiling-point , but remains bright under this liquid .
The superficial tarnish is a powerful base soluble in water , and reacting like an alkaline solution .
Melted in the air , thallium forms a readily fusible oxide , its behaviour resembling that of lead .
The formation of thallic acid and the properties of some of the thallates are described .
Sulphate , nitrate , the chlorides , sulphide , iodide , and other salts of thallium are described in detail .
The metal may be quantitatively determined by precipitation , either as protochloride , iodide , or platinochloride .
The position of thallium amongst elementary bodies is then discussed .
Although one or two of its properties show a resemblance to the alkaline metals , the author does not agree with continental chemists in classing it with this group , -numerous facts proving that its true position is by the side of mercury , lead , or silver .
The ready dehydration of its basic oxide ; the insolubility of its sulphide , iodide , chloride , bromide , chromate , phosphate , sulphocyanide , and ferrocyanide ; its great atomic weight ; its ready reduction by zinc to the metallic state ; its power of forming a strongly acid oxide ; and , according to Dr. Miller , the complexity of its photographic spectrum , -all prove that thallium cannot consistently be classed anywhere but amongst the heavy metals , mercury , silver , lead , &c. No weight is attached to M. Dumas 's argument in favour of thallium being related to potassium and sodium because its equivalent is rather near a figure obtained by adding twice the atomic weight of one metal to four times the atomic weight of the other .
The author shows that , by similar processes of addition , multiplication , or subtraction , it is not difficult to prove that thallium is related to any desired group of elements .
The author gives full analytical notes on thallium , showing where it would occur in the ordinary course of analysis , and detailing accurate methods of separating it from every metal with which it can be accompanied .
|
112282 | 3701662 | On the Effect of Temperature on the Secretion of Urea, as Observed on a Voyage to China, and at Hong Kong. [Abstract] | 440 | 441 | 1,862 | 12 | Proceedings of the Royal Society of London | Emil Becher | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 2 | 16 | 471 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112282 | null | http://www.jstor.org/stable/112282 | null | null | Biography | 28.964431 | Meteorology | 26.296265 | Biography | [
-44.233154296875,
-22.15456771850586
] | I. " On the Effect of Temperature on the Secretion of Urea , as observed on a Voyage to China , and at Hong Kong .
" By EMIL BECHER , M.D. , Assistant-Surgeon , Army Medical Staff .
Communicated by Dr. EDMUND A. PARKS .
Received January 20 , 1863 .
( Abstract .
) With a view to extend our knowledge of the physiological effects of temperature , with especial regard to the influence of tropical heat on the healthy system , Dr. Becher , with the liberal assistance of the Director-General , Army Medical Department , took advantage of a voyage to China ( round the Cape of Good Hope ) in 1857 , and a short residence at Hong Kong , in order to determine on himself the influence of the extreme variations of temperature incidental to that voyage , on the quantity of urine , urea , and chloride of sodium excreted during each twenty-four hours .
During a period of 163 days ( 100 days at sea , 63 days at Hong Kong during the change of monsoon ) , Dr. Becher collected the daily quantity of urine , and determined the amount of urea and NaCl by the volumetric method ( solutions of nitrate of mercury ) , and registered meteorological observations as accurately as circumstances would permit , observing all the time as constant a mode of living ( with regard to food , exercise , &c. ) as was practicable without undue restriction .
The whole of the observations , divided into the two periods indicated , are fully detailed in Tables , and graphically represented in Diagrams .
The results show a most remarkable relation between air-temperature and daily quantity of urea and NaCl , viz. a constant increase with the rising of temperature from 50 ?
-70 ?
, and an equally constant falling off with the further rise of temperature from 70 ?
-90 ? .
The physiological limit of the tropical zone , as marked by the sudden decrease in the quantity of urinary water , is constantly fixed at 76 ? .
Appended is an extract from a manuscript of Dr. Forbes Watson , containing a series of observations on the daily quantity of urine and the amount of solids therein excreted by a number of healthy soldiers in various temperatures during a voyage to India in 1850 .
These observations were made by Dr. Forbes Watson , who most kindly consented to their being added here , as far as they serve to illustrate the influence of temperature under otherwise constant conditions .
They are tabulated and graphically represented as much as possible on the same plan as those of Dr. Becher , and in their results show the most satisfactory harmony with the latter .
|
112283 | 3701662 | On Clinant Geometry, as a Means of Expressing the General Relations of Points in a Plane, Realizing Imaginaries, Reconciling Ordinary Algebra with Plane Geometry, and Extending the Theories of Anharmonic Ratios. [Abstract] | 442 | 443 | 1,862 | 12 | Proceedings of the Royal Society of London | Alexander J. Ellis | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 2 | 25 | 789 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112283 | null | http://www.jstor.org/stable/112283 | null | null | Formulae | 87.055441 | Fluid Dynamics | 9.29526 | Mathematics | [
66.3011703491211,
-26.223464965820312
] | II .
" On Clinant Geometry , as a means of expressing the General Relations of Points in a Plane , realizing Imaginaries , reconciling Ordinary Algebra with Plane Geometry , and extending the Theories of Anharmonic Ratios .
" By ALEXANDER J. ELLIS , B.A. , F.C.P.S. Communicated by ARTHUR CAYLEY , Esq. Received January 28 , 1863 .
( Abstract .
) The serious difficulties presented by " imaginaries " in plane geometry arise from treating the " principle of signs " as a matter of convention , and not as a particular case of a general operation , here termed a clinant , which consists in altering the length of a line in a given ratio , and rotating it through a given angle .
As the calculus of clinants furnishes a geometrical representation for every algebraical result , imaginaries disappear , and there is no longer any apparent disagreement between analysis and geometry .
Many theories , as , for example , those of anharmonic ratios , hitherto only established for points on a straight line , are also easily extended by means of clinants to embrace any points upon a plane .
The object of the present paper is to establish and illustrate these facts .
For this purpose it is divided into three distinct but closely connected parts .
Part I. shows that clinants obey the same laws of calculation as ordinary algebraical expressions , and explains their notation and geometrical construction .
This is illustrated by the solution of the problem of the determinate section generalized , and by a geometrical explanation of " imaginary " trigonometrical functions , applied to the discovery of the " imaginary " double rays in an homography .
Part II .
establishes the theory of stigmatics .
An index point , supposed to move from any origin into every point on a plane , is accompanied by one or more satellite points , termed stigmata , the relative position of the stigmata and index at any time being dependent on the relative position of the index and origin , according to some assigned law .
The locus of the stigmata , corresponding to each path of the index , forms a stigmatic curve .
The aggregate of these curves constitutes a stigmatic , which therefore consists of points conjugated with each other according to a characteristic law , ulti mately expressible by an equation between the clinant of the line connecting the index with the origin and the clinant of the line connecting the stigma and the index .
By elimination between two such equations , the common stigmata ( systigmata ) of two stigmatics , and by the condition of equal roots their coalescent systigmata , or homostigmata , may be determined .
These systigmata and homostigmata include , as particular cases , the points of " real " and " imaginary " intersection and contact of algebraical curves .
These generalities are illustrated by a consideration of the general stigmatic straight line and the central stigmatic circle .
The stigmatic straight line consists of stigmatic curves similar to the paths of the index , and their systigmata are the " double points " of similar figures .
The stigmata of a stigmatic circle are always harmonically conjugated with the extremities of its axis ( with which they always lie either on the same straight line , or the circumference of the same circle ) , and hence form an " involution " of points on a plane .
The construction of the systigmata and homostigmata of a stigmatic straight line , and stigmatic circle , furnishes a complete geometrical explanation and realization of the " imaginary intersections " of straight lines , with " real " and " imaginary " circles , " imaginary tangents " to such circles , and their polars and radical axes and common chords .
Part III .
contains an extension of the theories of anharmonic ratios from points on straight lines to any points in a plane , and explains and constructs the homography and involution of.such systems of points , with their double points , &c. Constant reference is made throughout this part to M. Chasles 's 'Geometrie Superieure , ' to show how his fundamental theories may be interpreted as conclusions in clinant geometry , to explain all cases of " imaginaries , " and to establish the fact that " real " and " imaginary " points are only two very particular cases of the general theory of conjugated points .
The whole memoir forms an introduction to a new and practical geometrical calculus , including and interpreting all analytical investigations on plane geometry .
|
112284 | 3701662 | Note on the Lines in the Spectra of Some of the Fixed Stars | 444 | 445 | 1,862 | 12 | Proceedings of the Royal Society of London | William Huggins|William Allen Miller | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0095 | null | proceedings | 1,860 | 1,850 | 1,800 | 2 | 19 | 666 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112284 | 10.1098/rspl.1862.0095 | http://www.jstor.org/stable/112284 | null | null | Astronomy | 46.175496 | Atomic Physics | 26.870722 | Astronomy | [
20.72968101501465,
-34.016937255859375
] | III .
" Note on the Lines in the Spectra of some of the Fixed Stars .
" By WILLIAM HUGGINS , Esq. , F.R.A.S. , and WILLIAM ALLEN MILLER , M.D. , LL. D. , Treasurer and V.P.R.S. Received February 19 , 1863 .
The recent detailed examination of the solar spectrum , and the remarkable observations of Kirchhoff upon the connexion of the dark lines of Fraunhofer with the bright lines of artificial flames , having imparted new interest to the investigation of spectra , it has appeared to the authors of the present note that the Royal Society may not consider a brief account of their recent inquiry upon the spectra of some of the self-luminous bodies of the heavens unworthy of attention , although the investigation is as yet far from complete .
After devoting considerable time to the construction of apparatus suitable to this delicate branch of inquiry , they have at length succeeded in contriving an arrangement which has enabled them to view the lines in the stellar spectra in much greater detail than has been figured or described by any previous observer .
The 'U 7-L1 LAL r1 apparatus also permits of the immediate comparison of the stellar spectra with those of terrestrial flames .
The accompanying drawing " X x ; u I > §§ ?
Ii 1 % -f j " y ?
'1'0 1|\1 r iminA , 1-l 11 111 shows with considerable accuracy the principal lines which the authors have seen in Sirius , Betelgeux , and Aldebaran , and their position relatively to the chief solar lines .
Without at present describing in detail , as they propose to do when the experiments are completed , the arrangements of the special apparatus employed , it may be sufficient to state that it is attached to an achromatic telescope of 10 feet focal length , mounted in the observatory of Mr. Huggins at Upper Tulse Hill .
The object-glass , which has an aperture of 8 inches , is a very fine one by Alvan Clark of Cambridge , U.S. ; the equatorial mounting is by Cooke of York , and the telescope is carried very smoothly by a clock motion .
It may further be stated that the position in the stellar spectra corresponding to that of Fraunhofer 's line D , from which the others are measured , has been obtained by coincidence with a sodium line , the position of which in the apparatus was compared directly with the line D in the solar spectrum .
The lines in the drawings against which a mark is placed have been measured .
Addendum.-Since the foregoing Note was presented to the Royal Society , the authors have learned that a paper on the same subject , accompanied by diagrams of the spectra of the Moon , Jupiter , Mars , and several of the fixed stars , by Mr. L. M. Rutherfilrd , has appeared in the January Number of the ' American Journal of Science ' for the current year .
The method of observing finally employed by Mr. Rutherfurd much resembles that adopted by the authors of this Note .
They therefore desire to add that , during the past twelvemonth , they have examined the spectra of the Moon , Jupiter , and Mars , as well as of between thirty and forty stars , including those of Arcturus , Castor , a Lyrae , Capella , and Procyon , some of the principal lines of which they have measured approximatively .
They have also observed 3 and y Andromede , a , ,3 , e and r Pegasi , Rigel , j Orionis , 3 Aurigae , Pollux , y Geminorum , a , y and e Cygni , a Trianguli , e , and n Ursae Majoris , a , / 3 , y , e and j Cassiopeiee , and some others.-[Feb .
21 , 1863 .
]
|
112285 | 3701662 | On Skew Surfaces, Otherwise Scrolls. [Abstract] | 446 | 448 | 1,862 | 12 | Proceedings of the Royal Society of London | A. Cayley | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 2 | 26 | 859 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112285 | null | http://www.jstor.org/stable/112285 | null | 108,806 | Formulae | 91.514941 | Headmatter | 6.210625 | Mathematics | [
64.62924194335938,
-33.19728088378906
] | I. " On Skew Surfaces , otherwise Scrolls .
" By A. CAYLEY , F.R.S. Received February 3 , 1863 .
( Abstract .
) It may be convenient to mention at the outset that in the paper " On the Theory of Skew Surfaces , " Camb .
and Dubl .
Math. Journ. vol. vi .
pp. 171-173 ( 1852 ) , I pointed out that upon any skew surface of the order n there is a singular ( or nodal ) curve meeting each generating line in ( n-2 ) points , and that the class of the circumscribed cone , or what is the same thing , the class of the surface , is equal to the order n of the surface .
In the paper " On a Class of Ruled Surfaces , " Camb .
and Dubl .
Math. Journ. vol. viii .
pp. 45,46 , ( 1853 ) , Dr. Salmon considered the surface generated by a line which meets three curves of the orders m , n , p respectively : such surface is there shown to be of the order =2mnp ; and it is noticed that there are upon it a certain number of double right lines ( nodal generators ) ; to determine the number of these , it is necessary to consider the skew surface generated by a line meeting a given right line and a given curve of the order m twice ; and the order of such surface is found to be =--m(m-1)h , where h is the number of apparent double points of the curve .
The theory is somewhat further developed in Dr. Salmon 's memoir " On the Degree of a Surface reciprocal to a given one , " Trans. R. Irish Acad. vol. xxiii .
pp. 461-488 ( read 1855 ) , where certain minor limits are given for the orders of the nodal curves on the skew surface generated by a line meeting a given right line and two curves of the orders m and n respectively , and on that generated by a line meeting a given right line and a curve of the order m twice .
And in the same memoir the author considers the skew surface generated by a line , the equations whereof are ( a,..3t , l)m=O ( al,..]t , l)n=0 , where a,. .
al,. .
are any linear functions of the coordinates , and t is an arbitrary parameter .
And the same theories are reproduced in the Treatise on the Analytic Geometry of three Dimensions , " Dubl .
1862 .
I will also , though it is less closely connected with the subject of the present memoir , refer to a paper by M. Chasles , " Description des Courbes a double Courbure de tous les ordres sir les surfaces reglees du troisieme et du quatrieme ordre , " Comptes Rendus , t. liii .
( 1861 , 2 ' Sem .
) , pp. 884-889 .
2K The present memoir ( in the composition of which I have been assisted by a correspondence with Dr. Salmon ) contains a further development of the theory of the skew surfaces generated by a line which meets a given curve or curves : viz. I consider , -lst , the surface generated by a line which meets each of three given curves of the orders m , n , p respectively ; 2nd , the surface generated by a line which meets a given curve of the order m twice , and a given curve of the order n once ; 3rd , the surface which meets a given curve of the order m three times ; or , as it is very convenient to express it , I consider the skew surfaces , or say the " scrolls , " S(m , n , p ) , S(m2 , n ) , S(m3 ) .
The chief results are embodied in the Table given after this introduction , at the commencement of the memoir .
It is to be noticed that I attend throughout to the general theory , not considering otherwise than incidentally the effect of any singularity in the system of the given curves , or in the given curves separately : the memoir contains , however , some remarks as to what are the singularities material to a complete theory ; and in particular as regards the surface S(m3 ) .
I am thus led to mention an entirely new kind of singularity of a curve in space-viz .
, such a curve has in general a determinate number of " lines through four points " ( lines which meet the curve in four points ) ; it may happen that of the lines through three points , which can be drawn through any point whatever of the curve , a certain number will unite together and form a line through four ( or more ) points , the number of the lines through four points ( or through a greater number of points ) so becoming infinite .
|
112286 | 3701662 | Researches on the Refraction, Dispersion, and Sensitiveness of Liquids. [Abstract] | 448 | 453 | 1,862 | 12 | Proceedings of the Royal Society of London | J. H. Gladstone|T. P. Dale | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 6 | 81 | 2,104 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112286 | null | http://www.jstor.org/stable/112286 | null | 108,799 | Chemistry 2 | 48.248786 | Optics | 22.458421 | Chemistry | [
0.7581280469894409,
-34.20743179321289
] | II .
" Researches on the Refraction , Dispersion , and Sensitiveness of Liquids .
" By J. H. GLADSTONE , Ph. D. , F.R.S. , and the Rev. T. P. DALE , M.A. , F.R.A.S. Received February 5 , 1863 .
( Abstract .
) This communication contains the results of some inquiries which were started by the authors in a previous paper " On the Influence of Temperature on the Refraction of Light " * .
The same apparatus had been employed , but some modifications were introduced in the method of observation , which are described ; and the amount of probable error from different sources was determined .
The liquids experimented on were either prepared or purified in Dr. Gladstone 's laboratory , or were specimens reputed to be pure , and lent for the purpose of this inquiry by Prof. Hofmann , Prof. Williamson , Prof. Frankland , Drs. Warren De la Rue and Hugo Muller , Mr. Buckton , Dr. Odling , Mr. A. H. Church , Mr. C. Greville Williams , and Mr. Piesse .
The data are collected in two long tables forming two appendices : the first containing the refractive indices of the lines A , D , and H , of 78 specimens at two or three different temperatures ; the second , the refractive indices of all the more important lines for 61 of these liquids , and 10 others at the temperature of the room when the observations were made .
Five points were investigated , and the following are the results arrived at with respect to each point .
I. The relation between the change of refraction ( sensitiveness ) and the change of volume by heat.-The uniform testimony of about 90 different liquids examined was that both refraction and dispersion diminish as the temperature increases .
The following Table will suffice as an example , showing as it does that the different rays are more sensitive in the order of their refrangibility : Refractive Indices .
Liquid .
Temp. A. B. D. E. F. G. H. Bisulphide of 1 11 ?
C. 16142 1-6207 1-6333 1-6465 1-6584 16836 1-7090 Carbon ... . .
36 ?
-5 1-5945 1-6004 1-6120 1-6248 1'6362 1-6600 1-6827 Difference ... ... 0-0197 0-0203 0-0213 0-0217 0-0222 0-0236 0-0263 , This change of refraction by heat was compared with the known or ascertained change of volume in bisulphide of carbon , water , methylic , ethylic , and amylic alcohols , ether , acetone , acetic acid , formic , acetic , and butyric ethers , methylic and ethylic iodides , salicylate of methyl , bromoform , benzole , xylole , cumole , nitrobenzole , hydrate of phenyl , the rectified oils of turpentine and Portugal and eugenic acid , and in every case it was found that the refractive index minus unity , multiplied by the volume , gave very nearly a constant at different temperatures .
Now every refractive index contains at least two coefficients : the one of refraction , which is represented by the theoretical limit of the spectrum ; the other of dispersion , for which the difference between the refractive indices of H and A may be taken as the exponent .
The refractive index , minus unity ( ~1 ) , is termed by the authors the " refractive energy " of the substance , and this multiplied by the volume ( , t--1 ) , or divided by the density , is termed the " specific refractive energy .
" It was not found as a rule that the theoretical limit of the spectrum gave more truly a constant than the line A ; but the difference is within experimental errors .
The empirical law was therefore expressed as follows:-The refractive energy of a liquid varies directly with its density under the influence of change of temperature , or , in other words , the specific refractive energy of a liquid is a constant not affected by temperature .
Yet the influence of dispersion renders this not absolutely accurate in the observed numbers , for the change of dispersion does not follow the same law , the spectrum contracting in some cases much more , and in other cases much less rapidly than the volume increases ; indeed no relation is as yet discoverable between the change of dispersion and that of density .
II .
The refraction and dispersion of mixtures of liquids.-This question has engaged the attention of several experimenters , only one of whom , however , M. Hoek , has offered a solution .
His formula depends on '2-1 .
Yet most of the results recorded were equally well explained on the supposition that the specific refractive energy of a mixture is the mean of the specific refractive energies of its components .
It was clearly desirable to test this in some cases where the refractive indices of the liquids mixed were very wide apart .
Fortunately , bisulphide of carbon and ether , substances almost at the opposite limits of the scale , were found to mix without condensation ; and another good experiment was obtained with aniline and alcohol , on mixing which , however , some diminution of volume occurs .
In both these cases the experimental numbers were slightly below those deduced from the mean of the specific refractive energies , the discrepancy being beyond the limits of probable error ; yet no other formula could be devised which would give a nearer approximation to the indices actually observed .
III .
The refSraction , disper sion , and sensitiveness of different members of homologous series.--Many such series were examined , and the results are tabulated , the refractive index of A and the length of the spectrum or dispersion being reduced , if necessary , to 20 ?
C. , and the sensitiveness being taken for the 10 degrees rising above 20 ?
C. ; the specific refractive energy , dispersion , and sensitiveness also form part of the Tables .
Methylic , ethylic , amylic , and caprylic alcohols are the first series examined , and it is found that on ascending the series the refraction increases ; the dispersion does so still more rapidly , while the sensitiveness remains nearly the same .
Other homologous series of the same group , such as the iodides , compound ethers , or mercury compounds , were also examined , and they all agree in exhibiting a progressive change in refraction and dispersion with the advancing members of the series ; but in which direction and to what extent depend on the other substances with which the compound radical is combined .
Yet , if we regard not the actual indices , but these , minus unity , divided by the density , a pretty regular increase is found to take place as the series advance .
The following Tables exhibit this : SSpecific Refractive Energy .
Radical .
I|iI l| Methyl ... ... C2 H3 *4105 -2359 3905 ... 389 .
1707 3727 Ethyl .
C4 H5 4482 -2614 '4127 '3905 -4127 4402 '3502 ' 2112 -3876 Propyl ... ... C ... .
4333 Butyl ... ... .
C ... 4402 | Amyl ... . .
CO Hl '4895 *3213 4492 -4432 '4527 -4724 '4306 CEnanthyl ... C14 H15 ... '4750 ... ... ... ... ... 5499 Capryl ... .
C H7 '5096 ... ... ... ... ... ... ... 5522 Laurostearyl C1 H ... ... 4890 Specific Dispersion .
Ether of Mercury Stannic Radical .
Alcohol .
Iodide .
Acid .
Acetate .
Cd Comp Hydride .
Acid .
Compd .
Compd .
Methyl ... ... ... ... 163 209 168 ... 140 256 Ethyl ... ... ... ... 190 218 174 174 170 268 Propyl ... ... ... ... ... ... . .
191 Butyl ... ... ... ... ... .
191 Amyl ... ... ... ... . .
212 224 198 198 ( Enanthyl ... ... ... ... ... ... . .
241 Capryl ... ... ... ... ... ... ... . .
237 Other groups of homologous bodies were also examined .
Benzole , toluole , xylole , cumole , and cymole gave nearly the same numbers , and no regular progression .
Pyridine , picoline , lutidine , and collidine showed an augmentation of the specific refractive energy , but a diminution of the specific dispersion with the advancing series .
Chinoline and lepidine ( which proved to be the most refractive organic liquid known ) showed an increase of each of the optical properties by the addition of C2 HI .
Thus the influence of the added increment on the rays of light differs in different groups , just as it does in respect to the boiling-point .
IV .
The refraction , dispersion , and sensitiveness of isomeric liquids.-Several of the liquids , isomeric with the different members of the benzole series , were examined ; some proved to be identical in all optical properties ; others sensibly the same in actual refraction and dispersion , though slightly different in density ; some again identical in density , but differing in optical properties ; while other isomeric bodies differed slightly in each of these respects .
Several hydrocarbons of the type C20 H16 , from essential oils , seemed to be identical in actual refraction , notwithstanding slight differences of their density .
In dispersion , too , there were some variations ; but not in sensitiveness .
Other hydrocarbons , however , of the same ultimate composition , but differing considerably in physical properties , differed also optically .
Compound ethers , as valerianic ether and acetate of amyl , which contain the same number of carbon , hydrogen , and oxygen elements , though differently arranged , are optically identical , as was partially shown by Delffs some years ago .
Aniline and picoline , each empirically C , H7 N , are totally different .
The conclusion arrived at is that isomeric bodies are sometimes widely different in these optical properties ; but that in many cases , especially where there is close chemical relationship , there is identity also in this respect .
V. The effect of chemical substitution.-By observing the amount of change in the optical properties which results from a replacement of one element by another , the chemical type remaining the same , it seemed possible to arrive at a knowledge of the influence of the individual elements on the rays of light transmitted by them .
Of the immense number of data required for the perfecting of such an inquiry , the following are afforded by the experiments already made .
The replacement of hydrogen by a compound radical , aniline-amylaniline ; and water , alcohol , ether ( according to Williamson 's theory ) .
Of hydrogen by oxygen-alcohol , acetic acid ; ether , acetic ether ; and carvene , carvole , eugenic acid .
Of hydrogen by peroxide of nitrogen-benzole , nitrobenzole , dinitrobenzole ( in solution ) ; glycerine , nitroglycerine ; and amylic alcohol , nitrate of amyl .
Of hydrogen by chlorine-benzole , chlorobenzole , terchlorobenzole ; and the substitution of chlorine by bromine-terchloride of phosphorus , terbromide of phosphorus ; chloroform , bromoform ; and bichloride of chlor-ethylene , bibromide of chlor-ethylene , bibromide of brom-ethylene .
When hydrogen is replaced by some other body , there is generally an increase of the actual refraction and dispersion ; but this is due to the increased weight , hydrogen having a very low actual , but a very high specific influence on the rays of light .
In each of the five instances of two substitution-products , as , for instance , cllorobenzole and trichlorobenzole , the lower one always retains in its optical properties an intermediate position between the original substance and the higher product .
These experiments on substitution sufficed to show , as the examination of isomeric bodies had done , that the special influence exerted on the rays of light by the elements of a compound is greatly dependent on the manner of their combination .
The following is given as a generalization approximately , if not absolutely true:-Every liquid has a specific refractive energy composed of the specific refractive energies of its component elements , modified by the manner of combination , and which is unaffected by change of temperature , and this refractive energy accompanies it when mixed with other liquids .
|
112287 | 3701662 | On the Change of Form Assumed by Wrought Iron and other Metals When Heated and Then Cooled by Partial Immersion in Water | 453 | 472 | 1,862 | 12 | Proceedings of the Royal Society of London | H. Clerk | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0098 | null | proceedings | 1,860 | 1,850 | 1,800 | 20 | 389 | 5,490 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112287 | 10.1098/rspl.1862.0098 | http://www.jstor.org/stable/112287 | null | null | Measurement | 75.524541 | Chemistry 1 | 13.487936 | Measurement | [
28.57858657836914,
-70.69025421142578
] | III .
" On the Change of Form assumed by Wrought Iron and other Metals when Heated and then Cooled by partial immersion in Water .
" By Lieut.-Col. H. CLERK , R.A. , F.R.S. Received February 9 , 1863 .
Origin of the Experiments.-A short time ago , when about to shoe a wheel with a hoop-tire , to which it was necessary to give a bevel of about xths of an inch , one of the workmen employed suggested that the bevel could be given by heating the tire red-hot and 1863 .
] 453 then immersing it one-half its depth in cold water .
This was tried , and found to answer perfectly , that portion of the tire which was out of the water being reduced in diameter .
The tire was 3 inches wide , inch thick , and 4 ' 2 " in diameter .
As this result was curious and not generally known , I considered it desirable to institute some further experiments in order to try how far , by successive heatings and coolings , this change of form could be augmented , and also whether the same effect could be produced on other metals than wrought iron .
Mode of carrying out the Experiments.-The experiments were made on cylinders of wrought iron of different dimensions , both hollow and solid ; immersed , some to one-half of their depth , others to two-thirds ; also on similar cylinders of cast iron , steel , zinc , tin , and gun-metal .
The specimens experimented on were all accurately turned in a lathe to the required dimensions , which were carefully noted ; they were then heated to a red heat in a wood-furnace used for heating the tires of wheels .
As soon as they had acquired the proper heat , they were taken out and immersed in water to one-half or two-thirds of their depth ( as stated in the experiment ) .
The temperature of the water ranged from 60 ?
to 70 ?
Fahr. The specimens were allowed to remain in the water about two minutes , in which time the portion in the air had lost all redness , and that in the water had become sufficiently cool to handle .
These alternate heatings and coolings were repeated till the metal showed signs of cracking or giving way .
The dimensions were noted after every five heatings .
The circumferences were measured in preference to the diameters , as the true circular form was liable to alter .
General Results.-It will be seen by an inspection of the figures that the general effect is a maximum contraction of the metal about one inch above the water-line ; and that this is the same whether the metal be immersed one-half or two-thirds of its depth , or whether it be nine , six , or three inches deep .
With wrought iron the heatings and coolings could be repeated from fifteen to twenty times before the metal showed any signs of separation ; but with cast iron after the fifth heating the metal was cracked , and the hollow cylinder separated all round just below the water-line after the second heating .
454 Cast steel stood twenty heatings , but was very much cracked all over its surface .
As respects the change of form of cast iron and steel , the result was similar to that in wrought iron , but not nearly so large in amount .
The cast iron did not return to its original dimensions , but the smallest diameter was about one inch above the water-line .
Tin showed no change of form , there being apparently no intermediate state between the melting-point and absolute solidity .
Brass , gun-metal , and zinc showed the effect slightly ; but instead of a contraction just above the water-line , there was an expansion or bulging .
The effect on wrought iron is best seen in the solid cylinder ( figs. 9 and 10 ) , where the displacement of particles just above the water-line appears to be compensated by the bulgings at the two extremities .
The specimens of wrought iron were submitted by Mr. Abel ( Chemist to the War Department ) to chemical analysis , and he informs me that he found nothing noteworthy in the composition of the metal ; nor was there any appreciable difference in the specific gravity of the metal taken from different parts of the specimen .
It appears therefore to be simply a movement of the particles whilst the metal is in a soft or semifluid state .
The following is an account of the experiments , which were carried out under the superintendence of Mr. Butter , Draughtsman of the Royal Carriage Department , to whom also I am indebted for the accompanying diagrams .
The exact dimensions of each specimen before and after heating are given in a tabulated form at the end of the paper , to facilitate comparison .
In figs. 22 and 23 the changes in form of the 9 " cylinders ( one immersed one-half , the other two-thirds its depth ) are shown in section after every five heatings ( half the full size ) .
Experiment .
1-A 4 ft. 2 in .
hoop-tire of 3 inches breadth and 3ths inch in thickness ( fig. 1 ) was heated and cooled by being immersed to half its depth in cold water five times , by which the effect shown in fig. 2 was produced .
1863 .
] 455 Fig. 1 .
~ ~~~~ ~-_~Fig .
2 .
One-eighteenth of full size .
The upper edge , or that cooled in air , had contracted 8 inches , or -2Ith its entire length , and slightly increased in thickness ; while the lower edge , cooled in water , had expanded '875 inch , making a difference between the two circumferences of 8'875 inches .
The breadth remained unaltered ( 3 inches ) , and kept perfectly straight .
Fig. 3 .
1_i I , : ! ?
: ' : _Li / L Vlll i ili Irilul liiiii ll , ll !
- , liN !
tuutttilt 2h !
tlttiillikikil KI Section showing the amount of contraction .
One-half the full size .
The dotted lines show the original form .
The quality of the iron was afterwards tested by pieces taken from the upper and lower edges , and also from the centre ; the fibrous -cEZR ----I=---1 ; 17-=1=-I ---- , - ; 2 ?
= ?
r== ; ; ; :__,.-_L-Ig---- ; -----'- ; ;:LrT ?
Sjc--------456 -------=- ... .
EIi condition had remained unchanged , the specific gravity had not altered appreciably , and there appeared to be no deterioration in any part of it .
Experiment 2.-Two hollow cylinders of wrought iron , 12 inches diameter and I inch thick each , and respectively 9 inches and 6 inches deep , were heated to redness , and cooled by half-immersion in cold water twenty times ; for effects see figs. 4 and 5 .
Fig. 4 .
Fig. 5 .
One-eighth of full size .
The 9-inch cylinder did not alter on the upper edge , cooled in air ; but the lower edge , cooled in water , contracted *6 inch , and the circumference , at about one inch above the water-line , was reduced 5*5 inches ; the internal surface had increased in depth '35 inch .
The small cylinder diminished it could not be welded , and was therefore riveted , of the same external dimensions as the 9-inch one of the foregoing experiment , was heated to redness and cooled by half-immersion ten times , in order to test the effect when the thickness of the metal was reduced as much as possible .
The upper and lower edges were not altered materially , while the greatest contraction took place on the water-line , instead of 1 inch above it as in the last experiment , and amounted to 3'5 inches .
The depth measured on the curve had increased 15 inch ( see fig. 6 ) .
Fig. 6 .
One-eighth of full size .
Experiment 4.--Two wrought-iron cylinders , exactly similar to those used in experiment 2 , were heated and cooled by being immersed to two-thirds their depth in water twenty times .
The upper edge of the large cylinder was reduced 2 ' 1 inches , and the lower edge '9 inch ; it contracted 5'9 inches at about an inch above Fig. 7 .
Fig. 8 .
] !
IT IPi T !
tI r-w , I WWL One-eighthl of full size .
the water-line , and the inside surface had increased in depth '35 inch ( see fig. 7 ) .
The upper edge of the small cylinder was reduced in circumference 3'6 inches and the lower edge '65 inch , while the greatest contraction at about one inch above the water-line was 4'6 inches ; and the internal surface had increased *15 inch in height ( see fig. 8 ) .
Experiment 5.-A solid cylinder of wrought iron , 3 inches in diameter and 6 inches deep , was heated and cooled by being immersed half its depth in water fifteen times .
The greatest contraction took place a little above the water-line and on the lower edge , being in each case '45 inch ; the upper edge was reduced only ?
1 inch .
Fig. 9 .
I I , if ---1 iiI ' II i/ / I I/ / One-half of full size .
The dotted lines indicate the original form .
A swell of metal took place on the two ends , but was greatest on the bottom , or that cooled in water , being '15 inch in height .
The fibre of the iron opened at the fifteenth cooling ( see fig. 9 ) .
Experiment 6.-A wrought-iron cylinder exactly similar to the last was cooled by being immersed to two-thirds its depth fifteen times .
The greatest contraction , amounting to *4 inch , took place a little above the water-line ; the upper edge was -05 inch smaller , and the lower edge '35 inch , while the swellings on the ends were nearly the same as in the last experiment ( see fig. 10 ) .
Fig. 10 .
One-half of full size .
The dotted lines indicate the original form .
The separation of the fibre took place at the fifteenth cooling .
Experiment 7.-Two flat pieces of wrought iron , each 12 inches long , 6 inches deep , and -5 inch thick , were heated and cooled twenty times , one being immersed to half , and the other to two-thirds its depth in water .
That immersed one-half had contracted or become indented on the ends fully '3 inch ; the other had similar indentations , but to only 460 one-half the amount .
They were both turned up into the form of an arc , had thickened on their upper edges , and increased 1 inch in thickness where the contractions on the ends took place ( see figs. 11 and 12 ) .
Fig. 1 .
ML .
_ _--Fig .
12 .
h ' One-fourth of full size .
Experiment 8.-Two hollow wrought-iron cylinders , 9 inches deep and 12 inches in diameter , were heated and cooled , one by simple exposure to air ( fifteen times ) , and the other by total immersion in water ( ten times ) No alteration occurred in the form of either* .
Experiment 9.-A solid cast-steel cylinder , of the same dimensions as that used in Experiment 5 , was heated and cooled by half-immersion twenty times .
The effect obtained was similar to that produced upon the solid wrought-iron cylinders , but the breaking up of the structure was different ( see fig. 13 ) .
The greatest contraction was slightly above the Fig. 13 .
W , L Fig. 14 .
( Top offig .
13 .
) Fig. 15 .
( Bottom of fig. 13 .
) - ... One-half of full size .
The dotted lines indicate the original figure .
water-line , and amounted to *38 inch ; the bulgings on the ends were *075 inch , being much less than on the wrought-iron cylinders .
point it weighed 50 lbs. 1'125 oz. , or 2'625 ozs .
heavier than it was at the commencement ; from the tenth to the fifteenth heating the accumulated scales peeled off , and the weight was gradually reduced to that stated above .
That which was cooled in water weighed 50 lbs. 12'5 ozs .
before the experiment , and 48 lbs. 14'5 ozs .
at its conclusion , giving a loss of 1 lb. 14 ozs .
, which was due to the action of the water peeling off the scale each time the cylinder was cooled .
46 Experiment 10.-A hollow brass cylinder , 6 inches long , 2 inches in diameter , and lg-th of an inch thick , was heated to redness and cooled by half-immersion thirty-four times .
The effect produced was the opposite to that which took place with the iron cylinders , being an expansion instead of a contraction at the water-line , the amount of which was * 75 inch , and it was also expanded on the lower edge ?
1 inch ( see fig. 16 ) .
Fig. 16 .
One-half of full size .
The dotted line indicates the original figure .
Experiment 11.-A hollow gun-metal cylinder was heated to redness and cooled twenty times by half-immersion .
The thickness of metal being greater than in the last experiment , the effect at the water-line was much less , but the lower edge had expanded ?
1 inch .
It began to crack all over at the last cooling .
Experiment 12.-A hollow tin cylinder was heated in linseed-oil which was brought to a temperature of 400 ?
Fahr. ; it was cooled by half-immersion in water five times .
2 The form was not altered in the least , though the heat was raised in the last instance to the melting-point , as shown by the lower part of the cylinder beginning to melt .
Experiment 13.-A hollow zinc cylinder was heated and cooled by half-immersion fifty times .
It was heated in a wood furnace , the degree of heat to which it was brought being regulated by the melting of a piece of tin which was conveyed at the same time with it into the furnace .
Several experiments with pieces of tin and zinc had been previously made , by means of which it was ascertained that in the same temperature tin melted in two-sevenths of the time requisite to melt zinc ; hence when the zinc cylinder and piece of tin were placed in the furnace together , the time occupied by the tin in reaching its melting-point was carefully noted , and the cylinder was left in the furnace as long again as the time thus observed ; by this means it was brought very nearly to its melting-point without incurring any danger of its actually melting .
The last five times , however , it was allowed to remain a little longer in the flame ; and the melting upon the top was retarded the last four times by placing a piece of iron upon it , which conducted heat from that part , allowing it to remain half a minute longer in the furnace .
The effect obtained was the same as that produced upon the brass cylinder ( Exp. 10 ) , or the opposite of what took place with iron ; an Fig. 17 .
464 [ March 5 , ( expansion of * 175 inch occurred upon the water-line , and of 115 inch upon the lower edge .
Experiment 14.-The hollow wrought-iron cylinder was heated to redness and cooled by half-immersion on its side , instead of on its end as in other experiments , twenty times .
The effect was a very complicated one ( see figs. 17 , 18 , and 19 ) ; the dotted lines show the original form .
Fig. 18 .
( Side view of fig. 17 .
) *-E , ~~~~~~~~~~~~~~~~~~~~~~~~~ Fig. 19 .
( Front view of fig. 17 .
) The three figures are one-sixth of full size .
1863 .
] 465 II I ?
i -2i Experiment 15.-A solid wrought-iron cylinder was heated to redness and cooled by half-immersion on its side twenty times .
The effect was of a similar nature to that of the last experiment ( see figs. 20 and 21 ) .
Fig. 200 Fig. 21 .
One-half of full size .
The dotted line indicates original figure .
Experiment 16.-A hollow cast-iron cylinder , the dimensions of which were the same as those of the deep cylinder of Experiment 14 , was heated to redness and cooled twice by half-immersion .
At the second cooling it fractured nearly all round , about an inch below the water-line .
It expanded all over , but the expansion was least about an inch above the water-line , i. e. it did not contract to its original dimensions .
Experiment 17.-A solid cast-iron cylinder , 3 inches in diameter and 6 inches deep , was heated and cooled five times by half-immersion .
At the fifth cooling it cracked across the bottom ; it also expanded 466 [ March 5 , throughout , and the expansion was least a little above the water-line , i. e. it did not contract to its original dimensions .
The subjoined figures ( half the full size ) show the changes produced on the 9-inch cylinders after every five heatings .
( Experiments 2 and 4 .
) Fig. 22 .
Fig. 23 .
12 " Cylinder , 9 " high , 1 " thick .
12 " Cylinder , 9 " high , 1 " thick .
Vide fig. 4 .
Cooled by '-immersion .
Vide fig. 7 .
Cooled by I-immersion .
No. 1 .
External surface , original form .
No. 1 .
External surface , original form .
2 .
, , , , after 5 coolings .
2 .
, , , , after 5 coolings .
3 .
, , , , 10 , , 3 .
, , , , , , 10 4 .
, , , , , , 15 , , 4 .
, , , , , , 15 , , 5 .
, , , ,,3 20 , , 5 .
, , , , , 20 p --I--- ' -- " ' -----'- ; -`--- ` Tabulated Statement of the Results of the Experiments .
Dimensions , in inches . ?
11 ?
a 1 ?
?ii Form of article , &c. X| ' 1a .
Wrought 5 Hoop-tire for a 4 ' 2 " wheel:iron .
External circumf .
of upper edge ... 155*5 147'5 8*0 do .
do .
lower edge ... 155'5 156'375 +0'875 Bevel of face ... ... ... ... ... ... ... .
90 ? ?
69 ? ?
21 2b .
Wrought 20 '12 " cylinder , 9 " deep and t " thick : iron .
Internal circumf .
of upper edge ... 37'6 37'6 0'0 do .
do .
contraction..i 37'6 32-1 --55 do .
do .
lower edge ... 37'6 37'0 -0'6 Depth , perpendicular ... ... ... ... ... 90 8-8 -0'2 do .
on curve , external ... ... ... 9'0 9'15 +0'15 , ^ do .
do .
do .
internal ... ... ... 90 935 +0'35 2e .
Wrought 20 12 " cylinder , 6 " deep and d " thick : iron .
Internal circumf .
of upper edge ... 37'6 36'9 --070 do .
do .
contraction ... 37'6 32*35 --5-25 do .
do .
lower edge ... 37'6 37-9 +0'30 Depth , perpendicular ... ... ... ... ... 6'0 5'7 --030 do .
on curve , external ... ... ... 6'0 6'05 +0 05 do do internal ... ... ... 66 30 6 030 +030 3d .
Wrought 10 .
12 " cylinder , " derep , thin sheet:iron .
External circumf .
of upper edge ... 38*40 38*40 0-00 ~ ; -~ " do .
do .
contraction ... 38-40 34'90 -3'50 do .
do .
lower edge ... 38 40 38'45 +0-05 Depth , on curve ... ... ... ... ... ... .
9 00 9-15 +0-15 4e .
Wrought 20 .
12"cylinder,9"deepand'"thick:iron .
External circumf .
of upper edge ... 40-90 38*80 --210 do .
' do .
contraction ... 40-90 35'00 -5'90 do .
do .
lower edge ... 40'90 40'00 --090 Depth , perpendicular ... ... ... ... ... 9'00 8'80 --020 do .
on curve , external ... ... ... 9'00 9'00 000 do .
do .
internal ... ... 9. .
900 935 +0'35 4f .
Wrought 20 12'cylinder , 6"deep and ' " thick:iron .
External circumf .
of upperedge ... 40'8 '37-2 -3-6 do .
do .
contraction ... 40*8 36*2 -4'6 ; ~~ : do .
do .
lower edge ... 40'8 40*15 --065 Depth , perpendicular ... ... ... ... ... 6'0 6'0 00 - ; do .
on curve , external ... ... ... 6-0 6'05 +0-05 do .
do .
internal ... ... ... 6-0 6'15 +0'15 5g .
Wrought 15 1 3 " cylinder , 6 " deep , solid:iron .
Circumference , upper edge ... ... ' 9'4 9'3 --01 do .
contraction ... ... 9'4 8 95 -0'45 do .
lower edge ... . .
94 8S95 -0'45 Bulge on upper end ... ... ... .
0 00 004 -004 f. erdo .
lower end ... ... ... ... ... 000 0*15 +-015 a For remarks see end of Table , p. 470 .
468 [ March 5 , TABLE ( continued ) .
Dimensions , in inches .
*S C. o0 o 6h .
Wrought 15 2 3 " cylinder , 6 " deep , solid:iron .
Circumference , upper end ... ... ... 9'40 9'35 -0*05 do .
contraction ... ... ... 9'40 9'00 --040 do .
lower edge ... ... ... 9'40 9-05 -0-35 Bulge on upper end ... ... ... ... ... 0'00 0 05 +0'05 do .
lower end ... ... ... ... ... 0'00 0-20 +0'20 7i .
Wrought 20 Flat piece , 12 " x6 " X:iron .
Length on curve , upper edge ... 12'00 10'75 -1*25 do do lower edge ... 12'00 12'10 -+010 Breadth , ends ... ... ... ... ... ... ... . .
6'00 5'75 -0-25 do .
centre ... ... ... ... ... ... .
6-00 6-00 0.00 Upper edge , out of straight ... ... 000 0060 +0-60 Indentation on ends ... ... ... ... ... 000 0'30 +0'30 7k .
Wrought 20 4 Flat piece , 12 " x 6 " X " : iron .
Length on curve , upper edge ... ... 1200 11'10 -0'90 do .
do .
lower edge ... ... 1200 12*20 +0-20 Breadth , ends ... ... ... ... ... ... .
6-00 5-87 --013 do .
centre ... ... ... ... ... ... ... 6-00 5.95 -0'05 Upper edge , out of straight ... ... 0'00 0'50 +0.50 Indentation on ends ... ... ... ... .
0'00 0'15 +0'15 8 .
Wrought 15 0 12 " cylinder , 9 " deep , " thick } N. iron .
10 total do .
do .
do .
9m .
Cast 20 4 3 " cylinder , 6 " deep , solid:steel .
Circumference , upper edge ... ... 9 03 8'93 -0'10 do .
contraction ... ... 9'03 8-65 -0'38 do .
lower edge ... ... 9'03 8'93 -0 ' 10 Depth , perpendicular ... ... ... ... ... .
600 6-10 +0'10 10 " .
Brass .
34 4 2 " cylinder , 6 " deep , -1 " thick : External circumf .
of upper edge ... 6-175 6-175 0-000 do .
do expansion ... 6 ' 175 6'350 +0-175 do .
do .
lower edge ... .
6'175 6'270 +-0095 11 ? .
Gun20 4 3 " cylinder , 6 " deep , - " thick:metal .
External circumf .
of upper edge ... 9*25 9'24 -0'01 do .
do .
on water-line ... 9'25 9'26 +0'01 do .
do .
of lower edge. .
9'25 9'38 +0-13 12 .
Tin , 51 2 " cylinder , 5 " deep , 4 " thick ... ... No effect .
13 .
Zinc .
50 3 " cylinder , 6 " deep , 4 " thick : External circumf .
of upper edge ... 9 525 9 575 +-0050 do .
do .
expansion ... 9-525 9700 -+0175 do .
do .
lower edge ... 9'525 9630 +0-105 !
et , predclr .
, ... ... '0 61 01 TABLE ( continued ) .
Dimensions , in inches . ?
g j id Form of article , &c. 99 14P .
Wrought 20 2 12 " cylinder , 9 " deep , 2 " thick:iron .
on External circumference of edges. .
40 65 39-86 --0-79 its do .
do .
centre. .
40-65 41,05 +-040 side .
Depth on curve , part cooledin air .
9 00 9 00 0 00 do .
do .
water-line .
9'00 8-25 --075 do .
do .
in water ... 9-00 8-80 -0-20 Swellofside , 1 " below W.L. ( ata , b ) 0'00 1'00 +1'00 Hollowofside , 4"above do .
( ate , d ) 0-00 0'40 +0-40 Longest ex. diam. 1 " below W. L. 12-94 14-275 +1-335 Shortest do .
at rt .
angles to W.L. 12-94 12-00 -0-94 Indentation of edges a little above water-line at e ... ... ... 000 0'45 +45 15q .
Wrought 20 l 3 " cylinder , 5a " deep , solid:iron .
on External circumference of edges. .
9-4 9'2 --0'2 its do do .
centre .
9-4 9-475 -+0075 side .
Depth along part cooled in air ... 5-375 5-150 -0-225 do .
do .
on W.L. 5-375 5-100 --0275 do .
do .
in water .
5-375 5-225 --0'150 Longest diam. at rt .
angles to W.L. 3-000 3-100 +0-100 Shortest do .
parallel with W.L. 3'000 2760 -0 240 and a little below it ... ... ... 16 .
Cast 21 12 " cylinder , 9 " deep , } " thick:iron .
External circumf .
of upper edge ... 40'90 41'05 +-015 do .
do .
least expansion 40'90 40-95 +0-05 do .
do .
of lower edge40-90 41-15 +0'25 17 .
Cast 53 3 " solid cylinder , 6 " deep:iron .
External circumf .
of upper edge ... 9-4 9'55 +0-15 do .
do .
least expansion 9'4 9-50 +0'10 do .
do .
of lower edge ... 9-4 9-55 +0-15 Remarks .
a The width was unaltered , and the thickness of the upper edge slightly increased .
Figs. 1 and 2 .
b Fig. 4 .
c Fig. 5 .
d Fig. 6 .
C Fig. 7 .
f Fig. 8 .
g The fibre opened at the fifteenth cooling .
Fig. 9 .
h The fibre opened at the fifteenth cooling after having exhibited a slight crack for two or three previous coolings .
Fig. 10 .
i The thickness of the metal at the indentation on ends increased -1 " .
Fig. 11 .
k The thickness of the metal at the indentation on ends increased similarly to the last .
Fig. 12 .
l Cooled in air 15 times .
Cooled in water 10 times .
m The ends became slightly rounded .
Fig. 13 .
n At the last cooling the lower end of the cylinder began to crumble away in the water .
Fig. 16 .
o The expansion of the lower end may probably be due to the cracking of the metal , which was greatest at that part .
P Figs. 17 , 18 , 19 .
There was an increased thickness of metal at e , q Figs. 20 , 21 .
470 [ March 5 , [ The cause of the curious phenomenon described by Colonel Clerk in the preceding paper seems to be indicated by some of the figures , especially those relating to hollow cylinders of wrought iron , which are very instructive .
Imagine such a cylinder divided into two parts by a horizontal plane at the water-line , and in this state immersed after heating .
The under part , being in contact with water , would rapidly cool and contract , while the upper part would cool but slowly .
Consequently by the time the under part had pretty well cooled , the upper part would be left jutting out ; but when both parts had cooled , their diameters would again agree .
Now in the actual experiment this independent motion of the two parts is impossible , on account of the continuity of the metal ; the under part tends to pull in the upper , and the upper to pull out the under .
In this contest the cooler metal , being the stronger , prevails , and so the upper part gets pulled in , a little above the water-line , while still hot .
But it has still to contract on cooling ; and this it will do to the full extent due to its temperature , except in so far as it may be prevented by its connexion with the rest .
Hence , on the whole , the effect of this cause is to leave a permanent contraction a little above the water-line ; and it is easy to see that the contraction must be so much nearer to the waterline as the thickness of the metal is less , the other dimensions of the hollow cylinder and the nature of the metal being given .
When the hollow cylinder is very short , so as to be reduced to a mere hoop , the same cause operates ; but there is not room for more than a general inclination of the surface , leaving the hoop bevelled .
But there is another cause of deformation at work , the operation of which is well seen in figs. 2 and 3 .
Imagine a mass of metal heated so as to be slightly plastic , and then rapidly cooled over a large part of its surface .
In cooling , the skin at the same time contracts and becomes stronger , and thereby tends to squeeze out its contents .
This accounts for the bulging of the ends of the solid cylinders of wrought iron and the rents seen in their cylindrical surface .
The skin at the bottom is of course as strong as at the sides in the part below the water-line ; but a surface which resists .
extension far more than bending has far less power to resist pressure of the nature of a fluid pressure when plane than when convex .
The effect of the cause first explained is also manifest in these cylinders , although it is less marked than in the case of the hollow cylinders , as might have been expected .
The tendency of the cooled skin of a heated metallic mass to squeeze out its contents appears to be what gives rise to the bulging seen near the water-line in the hollow cylinder of brass .
Wrought iron , being highly tenacious even at a comparatively high temperature , resists with great force the sliding motion of the particles which must take place in order that the tendency of the cooled skin to squeeze out its contents may take effect ; but brass , approaching in its hotter parts more nearly to the state of a molten mass , exhibits the effect more strongly .
It seems probable that even in the case of brass a very thin hollow cylinder would exhibit a contraction just above the water-line .
Should there be a metal or alloy which about the temperatures with which we have to deal was stronger hot than cold , the effect of the cause first referred to would be to produce an expansion a little below the water-line.--G .
G. S. ]
|
112288 | 3701662 | On the Influence of Temperature on the Electric Conducting Power of Thallium and Iron. [Abstract] | 472 | 475 | 1,862 | 12 | Proceedings of the Royal Society of London | A. Matthiessen|C. Vogt | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 4 | 67 | 1,181 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112288 | null | http://www.jstor.org/stable/112288 | null | null | Electricity | 32.070263 | Chemistry 2 | 31.450014 | Electricity | [
-6.203287124633789,
-74.0583724975586
] | I. " On the Influence of Temperature on the Electric Conducting Power of Thallium and Iron .
" By A. MATTHIESSEN , F.R.S. , and C. VOGT , Ph. D. Received February 12 , 1863 .
( Abstract .
) Thallium.-The experiments detailed in this paper were made with specimens of thallium lent to us by Mr. Crookes and Professor Lamy of Lille .
The values obtained for the conducting power , together with the formulae for the correction of the conducting power for temperature of the different specimens , were : For Mr. Crookes 's metal , 1st wire .
2nd wire at 0 ? .
X= 9-3640037936t + 000008467t ' ; 9 169 .
For M. Lamy 's first specimen , 2nd wire at 0 ? .
3rd wire .
X=9'419--0-039520t+ 0-00009656t2 ; 9-082 ; 9-223 .
Second specimen , 2nd wire at 0 ? .
X =9'054-0-034697t+0-00006554t2 ; 9-22.6 ; or as mean of all the determinations , some of which are not given here , X=9 1630-036894t+ 0-00008104t2 .
The conducting power of thallium therefore decreases between 0 ?
and 100§ 31-420 per cent. , which is a larger percentage decrement than that obtained for many other pure metals , namely 29'307 per cent.* Iron.-The specimens of iron experimented were , with two exceptions , lent us by Dr. Percy .
In the following Table we give the results obtained with them:(1 .
) Electrotype iron , deposited from solution of pure sulphate of iron .
The strips were very thin and porous ; we could not therefore obtain concordant values for the conducting power , but we were able to determine the percentage decrement in the conducting power between 0 ?
and 100 ? .
We have , for the above reason , taken the first observed conducting power equal 100 .
X100-0-51182t+0-0012915t2 , corresponding to a percentage decrement'of 38'262 per cent. ( 2 .
) No. 1 , annealed and cooled in hydrogen .
X= 100-0-51894t+0 0013415t2 , corresponding to a percentage decrement of 38*479 per cent. ( 3 .
) Electrotype iron , a strip cut from the same foil as No. 1 .
X= 100--051355t 0-0013221t2 , corresponding to a percentage decrement of 38'134 per cent. ( 4 .
) No. 3 , annealed in air .
X= 100050895t + 00002735t2 , corresponding to a percentage decrement of 38 160 per cent. ( 5 .
) This , as well as Nos. 6 , 7 , 8 , were specimens of iron which have been analysed .
They were all hard drawn .
X= 15719 --0074370t+0000 1763t2 , corresponding to a percentage decrement of 36'070 per cent. ( 6 .
) X= 15'672--0074045t+ 0'0001761t2 , corresponding to a percentage decrement of 36'010 per cent. ( 7 .
) X= 14'2690'064133t + 00001456t2 , corresponding to a percentage decrement of 34'742 per cent. ( 8 .
) X= 12-342-0-055894t+0'0001379t2 , corresponding to a percentage decrement of 34 ' 117 per cent. ( 9 .
) Strip of iron , heated in a current of hydrogen at a red heat for two hours .
This , as well as Nos. 10 , 11 , 12 , were hardened .
X= 14'673-0-067999t+0 0001597t2 , corresponding to a percentage decrement of 35'459 per cent. ( 10 .
) As No. 9 , heated for three hours under sugar charcoal in a current of hydrogen ; the carbon taken up was 0'99 per cent.\= 10-6540'044560t + 000009 789t2 , corresponding to a percentage decrement of 32'637 per cent. ( 11 .
) As No. 9 , heated for four hours under sugar charcoal in a current of hydrogen ; the carbon taken up was 0'933 per cent. X=9'925-0'040097t + 000009168t2 , corresponding to a percentage decrement of 31'163 per cent. ( 12 .
) As No. 9 , heated for three hours under sugar charcoal in a current of hydrogen ; the carbon taken up was 1'06 per cent. X= 9-457 0037573t + 0'00008642t2 , corresponding to a percentage decrement of 30'592 per cent. ( 13 .
) Thin music wire , melted with one quarter of its weight of peroxide of iron under a flux of plate glass .
X=13-381 -0'056829t+0'0001230t2 , corresponding to a percentage decrement of 33'278 per cent. ( 14 .
) A piece of narrow watch-spring .
X=8-565 -0029099t+0'00005383t2 , corresponding to a percentage decrement of 27*689 per cent. ( 15 .
) Commercial iron wire .
X= 13'7720058970t 0-0001 242t2 , corresponding to a percentage decrement of 33'801 per cent. From the results obtained , it is obvious that the higher the conducting power the higher the percentage decrement in the conducting power between 0 ?
and 100 ? .
This has been proved to be the case with about 100 alloys with which we have experimented .
We have also found that we may deduce the conducting power of a pure metal from an impure one when the impurity does not reduce the conducting power more than , say , 10 to 20 per cent. According to our experiments , the percentage decrement in the conducting power of an impure metal between 0 ?
and 100 ?
varies in the same ratio as the conducting power of the impure metal at 100 ?
, compared with that of the pure metal at 100 ? .
Thus , from specimens Nos. 5 , 6 , 7 , 9 , 13 , and 15 , the conducting power of pure iron was found to be at 0 ?
= 16'725 .
In conclusion , we give the values found for specimens of cobalt and nickel wire lent to us by Professor Wohler .
They were as follows : Cobalt wire .
X= 12-9300-035521t+0-00004887t2 , corresponding to a percentage decrement of 23'692 per cent. Nickel wire .
X= 12-222-0-040787t+0-000 7088t2 , corresponding to a percentage decrement of 27'573 per cent. Although these metals were said to be chemically pure , the results obtained seem to indicate that they are not so , having probably taken up some impurities in the process of fusion .
The following Table of the conducting powers of pure metals shows the place which the metals treated of in this paper take in the series .
Conducting power at 0 ? .
Silver ( hard drawn ) ... ... ... ... 100-00 Copper ( hard drawn ) ... ... . .
99.95 Gold ( hard drawn ) ... ... ... ... 77-96 Zinc ... ... ... ... ... ... .
2902 Cadmium ... ... ... ... ... ... . .
23 72 Cobalt* ... ... ... ... ... ... . .
17-22 Iron* ( hard drawn ) ... ... ... . .
1681 Nickel * ... ... ... ... ... .
13-11 Tin ... ... ... ... ... ... ... ... 12-36 Thallium ... ... ... ... .
9'16 Lead ... ... ... ... ... ... ... 8-32 Arsenic ... ... ... ... ... ... 4*76 Antimony ... ... ... ... ... ... 4-62 Bismuth ... ... . .
1-245
|
112289 | 3701662 | On the Amyloid Substance of the Liver, and Its Ultimate Destination in the Animal Economy. [Abstract] | 476 | 480 | 1,862 | 12 | Proceedings of the Royal Society of London | Robert McDonnell | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 5 | 52 | 2,186 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112289 | null | http://www.jstor.org/stable/112289 | null | null | Physiology | 32.982918 | Biology 3 | 25.726604 | Physiology | [
-56.79118347167969,
-30.52906608581543
] | II .
" On the Amyloid Substance of the Liver , and its ultimate destination in the Animal Economy .
" By ROBERT MCDONNELL , M.D. Communicated by WILLIAM BOWMAN , Esq. Received February 13 , 1863 .
( Abstract .
) After briefly referring to the discovery of the amyloid substance of the liver , and the earlier history of the subject , the author examines the facts which have induced Dr. Pavy to conclude that this substance is not normally transformed into sugar during life .
The author being led , after a careful repetition of Dr. Pavy 's experiments , to concur in his views , asks , If then the amyloid substance of the liver be not converted into sugar , what becomes of it ?
what is its normal destination in the animal economy ?
It is the object of the memoir to attempt to answer this question , which , it must be admitted , is one of the greatest delicacy ; nevertheless there appears on the whole to be evidence that the amyloid substance met with in the liver is on its way upwards towards the more exalted or complex immediate animal principles ; that , in fact , the process of healthy assimilation tends , if the expression may be used , to promote it from the rank of ternary ( hydrocarbonous ) to that of quaternary ( azotized ) compounds ; and that its conversion into sugar is to be looked upon as a deviation from this progressive course-a dissimilative instead of an assimilative process .
In order to establish this view it became necessary1st .
To investigate the chemical and physiological relations of the amyloid substance , not only of the liver , but of other organs and tissues , and to test the very interesting results , which are for the most part due to M. Charles Rouget .
2ndly .
To compare the portal and hepatic blood with each other , and with arterial and venous blood derived from other sources ; and 3rdly .
To consider the relations to each other of the different functions performed by the liver .
For if it be true , as Lehmann , Brown-Sequard , and others have asserted , that the fibrine and much of the albumen of the portal blood vanishes in the liver , and that at the same time that it destroys these azotized compounds it forms its non-azotized amyloid substance , and excretes bile containing so little nitrogen that it need hardly be taken into account , are we not , from the consideration of these functions , led to infer that the nitrogen which leaves the liver by no other outlet may go forth in the hepatic blood in union with the amyloid substance thus changed into a new azotized principle ; -that thus the liver is a great bloodmaking organ , in which there is constantly going on a reconstruction of certain ingredients of the blood ; that in it the fibrine , &c. , which has done its work , is disintegrated , the hydrocarbons of the bile abstracted , and the nitrogen combined with the amyloid substance , which , instead of being normally changed into sugar , emerges from the liver a constituent principle of the protoplasma , from the bosom of which ( to use the words of Bernard with reference to the foetal tissues ) organic evolution is to be accomplished ?
Of the existence of the Amyloid Substance of Bernard in the Placenta and other Organs and Tissues .
The cells of the placenta contain , during the earlier stages of embryonic life , animal dextrine , having characters identical with those of the amyloid substance of the liver ; its presence may be readily demonstrated under the microscope .
Bernard has discovered it in the placentae of rabbits , guinea-pigs , &c. He also made the very interesting observation that the multiple placentulae of the ruminants do not contain any amyloid substance , but that in this class of animals this substance is found in certain cells of the amnion .
The presence , however , in the amnion or the placenta , of epithelial cells containing amyloid substance , is a fact quite secondary to the general fact that this substance enters largely into the constitution of most of the tissues of the embryo .
Its existence does not indicate a new function of an organ doing temporarily the duty of the liver , but it indicates a new fact with regard to the development of certain structures and a new property of tissue .
During embryonic life a great part of the foetal tissues are found to be so impregnated with amyloid substance , that it appears to be the formative material from which these tissues are evolved ; and , in fact , it would seem to be related to their growth and development , as starch is to the growth and development of the tissues of vegetables .
In the skin of the chick in ovo , and of the foetuses of rabbits , cats , guinea-pigs , sheep , oxen , pigs , it is readily demonstrated ; it is seen by the addition of acidulated tincture of iodine , and is most abundant at the points where the aggregation of epithelial cells shows that the feathers and hairs are about being developed .
The horny structures contain it plentifully ; in the bill , the hoof , and the claws it exists in large proportion .
From the hoof of a foetal calf of about four months enough may be obtained , by the alcoholic solution of potash , for chemical examination and fermentation .
The muscular tissues of the foetus are full of it ; from 20 to 50 per cent. can be extracted from the muscles of foetal calves of from three to seven months by the aid of the alcoholic solution of potash .
Having arrived , by a repetition of Dr. Pavy 's ingenious experiments , at the conclusion that the amyloid substance of the liver is not normally changed into glucose , and finding on examination the accuracy of the facts concerning the physiological relations of the amyloid substance to the foetal and other tissues , discovered by M. Charles Rouget , and investigated by Bernard himself , the question presents itself , May it not be that the liver does for the adult what divers tissues do during the development of the foetus ?
May not this great organ form , with the help of the amyloid substance secreted in its cells , a nitrogenous compound , just as the muscles of the foetus convert the amyloid substance contained in them into the highly nitrogenous material of muscular tissue ?
May not , in fact , the amyloid substance of the liver be the basis of an azotized protoplasma forming a constituent of the blood of the adult animal , as the amyloid substance of muscle is the basis of the material from which the evolution of muscular tissue is accomplished ?
Even a superficial consideration of the functions performed by the liver leads one to answer these questions in the affirmative .
For if it be true that the blood which enters the liver is rich in fibrine and albumen , and that these materials are so completely changed within this organ that little or none of them leave it by the hepatic vessels , what becomes of them ?
It is true their hydrocarbonous constituents may be thrown out as bile .
But what of the nitrogen contained in them ?
If it does not escape by the bile-ducts , it has no other mode of exit save by the hepatic vessels .
The author conceives it to be reunited with the hydrocarbonous amyloid substance , and to leave the liver as a newly-formed proteic compound , partly perhaps as globuline , and partly as material , in its reactions resembling caseine in some respects , in others albuminose , and which is fully described in the memoir .
These considerations lead to the necessity of investigating the several distinct functions of the liver:1st .
As to its action on the fibrine and albumen of the blood .
2nd .
As to the constitution of healthy bile ( so far as its azotized elements are concerned ) .
3rd .
As to the relative composition and characters of the blood which enters and of that which leaves the liver .
The author adds his testimony to that of Lehmann and BrownSequard as regards the fibrine-destroying function of the liver ; he attempts to show that , in proportion to the amount of fibrine which disappears in the liver , the quantity of nitrogen eliminated in the form of bile is very small indeed , but that the blood in passing through the liver becomes greatly enriched in colourless corpuscles , and that it contains more abundantly than other blood an azotized compound , resembling what has been described by some authors as blood-caseine .
This material , although resembling , is not identical with caseine ; it can be obtained from the serum of blood abstracted by a peculiarly contrived instrument ( a drawing of which accompanies the paper ) from the vena cava , close to the mouths of the hepatic veins .
Whatever may be its precise chemical composition and characteristics , whether it is to be regarded as a form of albumen , or albumen-peptone ( albuminose ) , or caseine , it is enough to state , that during active digestion the blood which leaves the liver contains a proteic compound , that it is richer in this compound than arterial blood , and that this latter is richer in it than ordinary venous blood , or than that of the portal vein .
At the same time the blood of the hepatic veins contains a far larger quantity of colourless blood-corpuscles than the portal blood .
A microscopic examination of these kinds of blood shows that the colourless corpuscles are from five to ten times more numerous in the former than in the latter .
Physiologists are so familiar with this fact , as well as with the chief peculiarities of the colourless corpuscles of hepatic blood , that it is unnecessary to dwell upon the circumstances which have induced some of the most distinguished among them to regard as the most important function of the liver , the formation , or at least the rejuvenescence , of the blood-corpuscles .
Dr. Carpenter conceives that the appearance of the colourless corpuscles of the blood may be regarded as a phenomenon analogous to the development of cells in the albumen of seeds in the vegetable kingdom .
He also supposes that these cells aid in the conversion of crude alimentary matters into proximate principles .
Additional support is given to each supposition by the notion that these colourless cells stand in close relationship to the material formed in the liver , so closely resembling dextrine of vegetable origin .
It is true that there is nothing novel in the view that the liver is a great blood-forming organ , or rather that it is an organ in which certain components of the blood are disintegrated , while from some of the matter so disintegrated a constant reconstruction of the blood is going forward ; yet it is certain that , not long since , physiologists would have been unwilling to admit that materials constituted as the colourless blood-cells or caseine could be formed within the liver from a substance resembling starch taking to itself nitrogen derived , as one may say , from the retrogressive metamorphosis of tissue .
It is very improbable that , looking to the liver alone , such a conclusion would have been arrived at .
The consideration , however , of the physiological relations of the amyloid substance ( of Bernard ) , as regards the development of the azotized tissues of the foetus , - the fact that it is , so far as they are concerned , a protoplasma , which , by taking to itself nitrogen , terminates in the evolution of fully-formed nitrogenous tissues , -prepares one to consider the idea that the liver evolves its proteic compounds during adult life by a somewhat similar process .
To M. Charles Rouget we unquestionably owe the observation of the fundamental facts which lead to the foregoing conclusions ; yet the author hopes that the recapitulation of facts in this communication will be found worthy of the consideration of physiologists ; for he conceives that not only is the view of the subject which he has ventured to adopt in harmony with a great number of hitherto unexplained circumstances , but that it gives a solution more satisfactory than any yet given of certain pathological phenomena which it would be out of place to speak of here .
|
112290 | 3701662 | Supplement to a Paper on the Differential Equations of Dynamics. [Abstract] | 481 | 481 | 1,862 | 12 | Proceedings of the Royal Society of London | George Boole | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 1 | 7 | 208 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112290 | null | http://www.jstor.org/stable/112290 | null | null | Formulae | 92.087481 | Biography | 3.939629 | Mathematics | [
80.29478454589844,
-37.082298278808594
] | III .
Supplement to a Paper " On the Differential Equations of Dynamics .
" By Professor GEORGE BOOLE , F.R.S. Received February 9 , 1863 .
( Abstract .
) It is shown in the general paper that if an integral of any one equation of the peculiar system of ( partial differential ) equations there discussed be found , then if a certain numerical result of subsequent and always possible operations prove odd , an integral of the entire system can be found by the solution of a single differential equation of the first order .
It is shown in the paper now sent that , when the above numerical result is even * , we can reduce the original system of partial differential equations into a new system , fewer in number by unity at least , and of the same general character , so as to admit of a repetition of the same procedure .
Thus the common integral sought will finally be given either by the solution of a single differential equation of the first order , or by finding one integral of the single partial differential equation , which , in the most unfavourable case conceivable , will remain at last .
|
112291 | 3701662 | On Peculiar Appearances Exhibited by Blood-Corpuscles under the Influence of Solutions of Magenta and Tannin | 481 | 491 | 1,862 | 12 | Proceedings of the Royal Society of London | William Roberts | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0102 | null | proceedings | 1,860 | 1,850 | 1,800 | 11 | 132 | 3,628 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112291 | 10.1098/rspl.1862.0102 | http://www.jstor.org/stable/112291 | null | null | Biology 3 | 46.972461 | Biology 2 | 18.040909 | Biology | [
-62.742889404296875,
13.848319053649902
] | 1 .
" { On Peculiar Appearances exhibited by Blood-corpuscles under the influence of Solutions of Magenta and Tannin .
" By WILLIAM ROBERTS , M.D. , Physician to the Manchester Royal Infirmary .
Communicated by Dr. SHARPIEY , Sec. R.S. Received February 18 , 1863 .
The object of the following paper is to give an account of certain observations which seem to indicate that the cell-wall of the vertebrate blood-disk does not possess the simplicity of structure usually attributed to it .
It is well known that the blood-corpuscles , when floating in their own serum , or after having been treated with acetic acid or water , * Also when odd , but then not required .
appear to be furnished with perfectly plain envelopes , composed of a simple homogeneous membrane , without distinction of parts .
But , as will appear from the observations here to be related , when the blood is treated with a solution of magenta ( nitrate of rosanilin ) or with a dilute solution of tannin , the corpuscles present changes which seem irreconcilable with such a supposition .
Attention is first asked to the effects of -magenta .
When a speck of human blood was placed on a glass slide and mixed with a drop of a watery soluition of magenta* , the following changes were observed .
The blood-disks speedily lost their natural opacity and yellow colour ; they became perfectly transparent , and assumed a faint rose colour ; they also expanded sensibly , and lost their biconcave figure .
In addition , a dark-red speck made its appearance on some portion of their periphery .
The pale corpuscles took the colour much more strongly than the red ; and their nuclei were displayed with great clearness , dyed of a magnificent carbuncle-red .
Many of the nuclei were seen in the process of division , more or less advanced ; and in some cells the partition had resulted in the production of two , three , or even four distinct secondary nuclei .
These appearances were first observed in freshly-drawn blood from the finger .
Subsequently blood from the horse , pig , ox , sheep , deer , camel , cat , rabbit , and kangaroo was examined in like manner .
The effect on the red corpuscles ( to which all the observations hereinafter recorded are exclusively confined ) was in each instance the same as in human blood .
The nucleated blood-disks of the oviparous classes , when treated similarly , yielded analogous results .
The coloured colntents were forthwith discharged ; the central nucleus came fully into view , and assumed a deep-red colour ; the corpuscles expanded , they lost something of their oval form , and approached nearly , or sometimes quite , to a circular outline .
Lastly , there appeared on the periphery a dark-red macula , of a character and position resembling that seen on the mammalian blood-disk .
Such a macula was detected in the fowl , in the frog , and in the dace and minnow , Owing , however , to the large quanltity of molecular matter floating in the serum , and which was coloured by the magenta , difficulties were found in preparing specimens which carried conviction that the macula in question was not an adhering granule .
It was also found that it required a nice adjustment of the relative quantities of the solution and of the blood to bring , it out .
It was only when the right proportions were hit , and especially when the disks were made to roll over in the field of the microscope , that the existence of a coloured particle organically connected with the cell-wall could be satisfactorily made out .
The best specimens were prepared from human blood drawn in the fasting condition , and from the blood of a kitten two days old .
From well-prepared specimens of human blood the following particulars were gathered ( see fig. 1):-Nearly every disk possessed the parietal macula ; it could be distinctly recognized in nine-tenths of them ; and in several of those in which it was not at first visible , it came into view as the corpuscles revolved in the field .
The macula was clearly situated in the cell-wall , and not in the interior of the corpuscle .
Usually it appeared as if imbedded or set in the rim of the disk , like the jewel in a diamond ring ; but sometimes it occupied various positions on the flat surfaces , and when so placed , the spot was difficult or impossible to detect .
It commonly presented a thickly lenticular shape ; sometimes it was square , and occasionally in appearance vesicular ( fig. 1 , A , a ) .
In some instances , and especially in long-kept specimens , the particle was seen to stand out on the outline of the disk like an excrescence .
Fig. 1 .
A6 ' lbld B.olslotetd ihm et A. Humanl blood .
B. Fowl 's blood treated with magenta .
Still more rarely , instead of a spot , a thick red line ran round the circumference for a quarter or a third of its extent ( fig. 1 , A , 6 ) .
As a rule it was extremely minute , covering generally not more than a twentieth or thirtieth of the circumference ; but there was a considerable variation in its magnitude and distinctness .
Very rarely two specks could be seen ; but the occurrence of adhering granules rendered the verification of this point extremely difficult .
This description applies , so far as the iniquiry has yet been prosecuted , to the mammalian blood-disk generally , making allowances for differences in size .
In the camel the macula occupied indifferently any part of the oval outline .
Among the oviparous classes , the blood of the fowl , frog , dace , and minnow has been most fully examined ( see fig. 1 , B ) ; but the blood of the sparrow , duck , goose , and turkey was also searched , as weli as that of the newt and carp .
In all of these a tinted particle appeared , more or less constantly , in the cell-wall , when the corpuscles were treated with magenta * The presence of a central nucleus in these classes caused the macula to be invisible more frequently than in mammalia , inasmuch as it suffered eclipse when situated over or under the central nucleus .
In the fowl , dace , and minnow it was fouLnd easy to bring out the parietal macula ; in the fish two spots were not unfrequiently seen .
The macula was situated indifferently on any part of the periphery ; and sometimes it projected from the surface .
When happily prepared the specimens were even beautiful .
The central nucleus was dyed of the finest red ; and on the delicate outline of the cell-wall hung the red parietal macula , offering a not altogether fanciful resemblance to the astronomical figures representing the moon coursing in its orbit round the earth .
At this stage of the inquiry it was conceived that an improved demonstration might be obtained by fixing the dye with a mordant , and then subjecting the corpuscles to a lavatory process , so as to get rid of the floating granules which so much interfered with the view .
For this purpose a solution of tannin ( which is one of the mordants for magenta used in the arts ) was employed ; and some advantage was found therein .
When a solution of tannin , of 3 grains to the ounce of water , was added to blood that had already been dyed with magenta , it was found that the parietal maculae had their colour intensified , and that they became more conspicuous objects .
The investigation was , however , not pushed any further in this direction , for it was found that tannin alone produced an even more remarkable effect than magenta .
To this effect I now desire to draw particular attention .
When a solution of tannin , of the strength of 3 grains to the ounce , was applied to human blood , or to that of the horse , ox , sheep , pig , or cat , the blood immediately became turbid ; and when a drop was placed under the microscope the corpuscles were found greatly changed , as represented in fig. 2 .
Fig. 2 .
Human blood after the action of tannin .
a. Double pullulation .
b , b. Hooded modification .
c. Outline of the cell seen continuously through the pullulation .
d. Bursting of the pullulations independently of destruction of the cell .
Each corpuscle appeared to have thrown out a bright , highly refractive bud or projection on its surface .
The projections were usually about a fourth part of the size of the corpuscle on which they were fixed ; but they varied considerably .
Some were only minutebright specks in the cell-wall ; others were half or even twothirds as large as the corpuscle itself .
Very rarely ( in mammalian blood ) two such projections were seen ; and as rarely a corpuscle was devoid of any .
The projections were commonly round or dome-shaped , bordered with a deeply refractive outline .
Frequently a minute , apparently vesicular body could be seen within this outline , and then the projection presented a curiously hooded aspect ( fig. 2 , 6 , b ) .
In a urinary deposit from a lad twelve years of age , containing pus and blood , nearly every blood-disk presented the hooded appearance after the addition of tannin .
The blood of the fowl , turkey , duck , and goose showed exactly analogous phenomena with the same reagent ( see fig. 3 ) .
Fig. 3 .
Blood of fowl after the action of tannin .
The projection had sometimes the hooded character with a vesicular body within ; sometimes the projection offered no such distinction of parts .
It was situated indifferently on any part of the periphery .
In all the birds examined a second projection was as rare as in mammalia .
Of fish , the dace , minnow , and carp were examined .
T'he tanninsolution produced a similar effect to that seen in the fowl-with this difference , that a large number of corpuscles had two projections instead of one .
In the carp double and single projections occurred in about equal proportions ; in the minnow double projections were all but universal .
The second projection was situated sometimes at the opposite pole of the disk , sometimes in near proximity to its fellow , or at any point between .
Very rarely , a third projection was seen in the dace .
In the blood of the frog there was a strong tendency to the indefinite mnultiplication of the projections ; two , three , four , and even five would rise in succession on the surface of the disk .
It appeared , too , not unfrequently as if the entire outer membrane of the cell was detached from the parts beneath and raised into eight or ten unequal elevations , giving the outline of the disk an irregularly crenate appearance * .
The formation of these singular projections , or pullulations , on the blood-disks could be watched without difficulty by placing a drop of the tannin-solution benieath the covering glass , and permitting a little blood to insinuate itself into the solution inder the microscope .
As the blood flowed in and mingled with the tannin , the corpuscles were observed gradually to enlarge , and then sudldenly , without previous warning , to shoot out the projection .
As a rule , it does not appear to grow afterwards .
The phenomenon was finely seen in the defibrinated blood of the fowl after it had been allowed to sink through a column of syrnp ( sp. gr. 1025 ) in a test-tube .
Fowl 's blood washed in this way was mixed , in a little glass , with about five times its volume of the tannin-solution , and a drop immediately put under the microscope .
The disks first enlarge and become rounded , and the central nucleus comes into view .
In thirty or forty seconds the pullulation begins ; and each corpuscle , with instantaneous rapidity and without previous sign , throws out its bud .
The disk itself suffers not the least disturbance during this act ; it preserves its symmetry unchanged , as if it had no concern , beyond that of proximity , with the sudden apparition on its surface .
No visible rupture of the cell-wall took place .
The circular out .
line of the latter could sometimes be distinctly followed through the projection ( fig. 2 , c ) ; and as the altered corpuscles revolved in the field of the microscope , the projection appeared to be organically connected with it , but to form no part of its cavity .
In the human blood-disks the application of acetic acid , soon after the tannin , caused , on two occasions , the pullulations gradually to subside , and finally to disappear , and then the disk resumed its original circular outline .
I failed to produce this " redux " effect in the fowl ; and did not always succeed with human blood , probably because the change produced by the tannin had gone too far .
The modification noted under the term " hooded " appearance depends , I believe , upon secondary conditions of concentration and quantity of the tannin-solution in comparison to the blood .
When the hooded condition has been watched in the act of occurrence , it was noticed that the outer hood was shot out first , and instantly after this the highly refractive vesicular body made its appearance within .
The contents of the hood ( excluding the vesicular body ) appeared usually to refract the light like the body of the cell , or even less strongly ; sometimes , however , more strongly .
The effect of tannin did not cease with the production of the elevations just described .
At first the cells and their projections preserved their elasticity ; but after a while ( a few minutes , or several hours , according to the proportions used ) the corpuscles and their projections became solid , and they could be cracked by pressure under the microscope like starch-granules .
More slowly the same destruction overtook the corpuscles spontaneously ; and this significanit fact was observed in the course of it:-sometimes the cell ruptured before the projection , the latter persisting as a bright granule amid or near the debris ; sometimes , on the other hand ( in the horse ) , the projection broke up before the disk to which it was attached .
In this latter case , the hood ( if there were any ) broke up first into a scattered nebula of granular appearance , and then the nucleolus-like body withini burst into three or four bright fragments ( fig. 2 , d ) .
This train of events seemed to remove all doubt as to the complete isolation of the projection from the cavity of the disk .
Last of all , the disk itself began to crack ; in a few days all my specimens were thus destroyed .
In addition to magenta and tannin the following substalnces were tried , but they did not produce phenomena in the least analogous with the foregoing:-gallic acid , ferrocyanide of potassium , santonine , sulphate of magnesia , alcohol and water , solutions of carbolic acid , of atropine , morphia , iodine , sugar , gum , glycerine , and infusion of coffee .
A solution of picric acid produced the appearance of a parietal particle like that brought out by magenta , except that it was not coloured .
An exactly similar appearance was on one occasion observed in blood-corpuscles in the urine of a patient with acute Bright 's disease .
When magenta was applied after the process of pullulation had taken place , the projections were found to take the dye strongly , and especially the vesicular body within the hood .
By this proceeding beautiful and remarkable objects for microscopical examination were obtained .
In the fowl , dace , and minnow the projection was tinted earlier than the central nucleus-probably from its more ready access to the pigment .
The explanation of these appearances presents great difficulties , and in the present state of the inquiry can only be offered provisionally .
The effect of the magenta-solution is not merely to tint , and so render visible a very minute body .
In watching the effect of magenta , the first thing observed is that the natural yellowish colour of the disk is discharged , and that a faint rose tint is assumed in its stead .
The disks at the same time lose their biconcave shape .
The parietal macula is rather " brought out " than revealed , and the action of the solution is , to a very great extent , of a simply osmotic character .
The action of the tannin-solution is likewise in the main of a similar nature , but modified in some very peculiar manner .
Its first operation is to cause the corpuscle to enlarge byimbibition , and this goes on progressively until at length the cell is destroyed .
If the solution be strong , this destruction supervenes at once .
The tannin also unites with the cell-contents and coagulates them , imparting to the corpuscle , finally , a solid consistence .
The conditions of the imbibition are disturbed by the previous application of magenta ; for no pullulation , or at most only traces , occurs when the corpuscles are treated first with magenta and then with tannin .
The bearing of these observations on the current views respecting the structLLre of the vertebrate blood-disk is important .
They seem to warrant the inferences drawni in the two following paragraphs : 1 .
The exact identity of the appearances produced in the blooddisks of the ovipara with those observed in the mammalian corpuscles lenids strong support to the view that these corpuscles are homologous as wholes ; and that the mammalian blood-disk is not the homologue of the nucleus of the coloured corpuscle of the ovipara , as was conceived by Mr. Wharton Jones .
2 .
The observations likewise lead to the belief that the envelope of the vertebrate blood-disk is a duplicate membrane ; in other words , that within the outer covering there exists an interior vesicle which encloses the coloured contents , and , in the ovipara , the nucleus .
Dr. Ilensen* of Kiel had already in 1861 convinced himself , from wholly different observations , that the blood-corpuscles of the frog possess such a structure .
On this view the blood-corpuscle is anatomically analogous to a vegetable cell , and the inner vesicle corresponds to the primordial utriele .
The present observations indicate , by direct proof , a duplication at only one or , at most , two points in the blood-disks of mamimals and birds .
Nevertheless certain appearanices , occasionally observed , favour the notion of a complete duplication ( fig. 1 , 6 ) .
The aclmission of this hypothesis , however , scarcely removes the difficulties sufficiently to permit a tenable explanation to be offered of the appearanees described in this paper .
Yet , as it may prove suggestive to some other inquirer , I will not suppress what appears to me the explanationi least open to objections .
It might be conceived that the cells enlarged by imbibition , until at length the less distensible inmner membranie gave way , and permitted an extravasation of a portion of the cell-contents betweeni it and the outer membrane , its own continuity being in the meanwhile instantaneously restored by cohesion of the ruptured borders-t .
In this way a microscopic drop of the cell-cointents would be lodged between the outer and inner membrane , and completely severed from the general cell-cavity .
The peculiar modification spoken of as the " hooded " appearance might be due to imbibition of fluid between this microscopic drop and the outer envelope .
The chief difficulties in the way of this explanation arise out of the differences of nature which appear to exist between the projection and the general cell-contents of which it is supposed to be a detached portion .
The projection refracts light much more highly than thie cell-contents ; it also is deeply dyed by magenta , whereas the cellcontents are only very feebly so .
In conclusion , it may be added that important advantages may be expected from the use of magenita in histological researches .
Its inert chemical character , its prodigious tinting power , and its solubility in water eminently fit it for such a purpose .
It will probably prove of especial use in bringing into sight objects which otherwise evade the visual organs from their absolute colourlessness and transparency , and from the equality of their refraction with the medium in which they exist .
|
112292 | 3701662 | On Quinidine, and Some Double Tartrates of the Organic Bases | 491 | 501 | 1,862 | 12 | Proceedings of the Royal Society of London | John Stenhouse | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0103 | null | proceedings | 1,860 | 1,850 | 1,800 | 11 | 166 | 3,581 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112292 | 10.1098/rspl.1862.0103 | http://www.jstor.org/stable/112292 | null | null | Chemistry 2 | 96.692546 | Agriculture | 1.644847 | Chemistry | [
-50.9758186340332,
-54.85183334350586
] | II .
" On Quinidine , and some Double Tartrates of the Organic Bases .
" By JOIIN STENHOUSE3 , LL. D. , F.R.S. Received February 23 , 1863 .
Quinidine , as is well known , was first observed by Henry and Delondre , and likewise by Sertuerner , in what is called the " quinidine " of commerce , which consists chiefly of a mixture of quinidine , quinine , and resinous matters obtained from the mother-liquors of the suilpbate-of-quinine manufacture .
Van Heijningen , however , was the first person who succeeded in separating quinidine , which he called ( 3-quinine , from this mixture and in obtaining it in a pure and crystalline state .
He likewise ascertained that quinidine was isomeric with quinine .
Its action on polarized light was studied by Pasteur , who observed that its solution in absolute alcohol produces deviation to thie right , while a similar solution of quinine produces rotation to the left ( Buchardat ) .
As comparatively few of the salts of quinidine have hitherto been analysed , and those chiefly by Van Ileijningen , I was iniduced to prepare a few more of them , and likewise to examine the action of iodide of ethyl upon the alkaloid itself .
I am indebted for the quinidine which I employed for this purpose to Mr. John Elliott Howard of Stratford .
It was perfectly white , and consisted of large , well-defined crystals .
Before using it , however , I recrystallized it out of alcohol .
The quinidine gave a green colour with chlorinewater and ammonia , and the solutions of its salts all exhibited a fluorescent power almost equal to that of quiniine .
A solution of its sulphate likewise yielded Hierapath 's so-called sulphate of iodoquinidine , crystallizing in long quadrilateral prisms possessing a deep garnet-red colour and the other well-known characters of that salt .
*343 gramme of pure quinidine , dried at 1000C .
, gave *9315 gramme carbonic acid and '238 gramme water .
This corresponds to 74 04 per cent. of carbon and 7'71 per cent. of hydrogen .
The formula C4L H24 N2 04 requires 74-08 and 7-4 per cent. Quinidine Platinum-salt , C401124 N2 04 , 21 Cl + Pt C1 , .
-On the addition of bichloride of platinum to a solution of hydrochlorate of quinidine , an immediate precipitate takes place if the solution be cold and concentrated ; but if dilute or hot solutions be employed , it only crystallizes out after some time .
It is very insoluble both in cold and in hot water , but crystallizes from boiling dilute hydrochloric acid in brilliant but irregularly-formed crystals , which decomposed when heated to about 2000 C. , evolving a peculiar aromatic odour somewhat resembling that of hawthorn..485 gramme of this salt , when dried at 150 ?
C. , on ignition gave *1995 gramme of metallic platinum .
This corresponds to 26f66 per cent. The formtula C40 24 N2 04 , 21 Cl + 2Pt Cl , requires 26 81 per cent. Both quinidine and its platinum-salt were first analysed many years ago by Baron Liebig ; but as he employed amorphous quinoidine for this purpose , Gerhardt supposes that he operated on a mixture of the three isomeric alkaloids , quinidine , quiniicine , and quinine .
Quinidine Gold-salt , C40 2 , N , 0 , , 21 C1+ 2Au Cl,.-The goldsalt is prepared by dissolving quinidine in hydrochloric acid and adding excess of terchloride of gold , when it falls as a bright yellow powder .
This salt appears to be decomposed by boiling with water , turning brown and apparently fusin , .
It is therefore necessary to precipitate it in the cold .
Well washed and dried in vacuo , oln heatino to 1000 it lost about -5 per cent. , probably hygroscopic water ; when further heated to 1150 , it fuised , turned browni , and began to decom .
pose .
'3575 gramme of gold-salt dried at 100 ?
gave *14 gramme of metallic gold .
This is equivalent to 39 15 per ceint .
The formula o04 02 04 , 211 C+2Au C13 requires 39'2 per cent. Nihtrate-of-Silver Salt of Quinidinie , 0C4 , 12 , N 04 , Ag NO , .
This was prepared by adding , nitrate-of-silver solution to any alcoholic solution of quinidine ; the mixture becamne semisolid from precipitation of the above salt in the form of minute n-eedles .
These were thrown on a filter and thoroughly washed with cold water , in which they are scarcely at all soluble .
The compound was then recrystallized from hot water slightly acidulated with nitric acid ; after filtration it separates , on cooling , in beautiful silky needles , which , on being freed from the mother-liquor and dried between bibulous paper , htave almost the lustre of metallic silver , such as is produced on igniting its organic salts .
It partially decomposes every time it is recrystallized , but much more so when spirit is substituted for water , the solution becoming black from reduced silver .
*40 1tgramme of the salt , dried at 100 ?
, gave 115 chloride of silver , corresponding to '08656 gramme of metallic silver .
This gives 21'59 per cent. According to the formula 020 " 24 N2 04 , Ag NO6 , theory requires 21 86 per cent. Mercuro-hydrochlorate of Quinidcine , C40H124 N204 , 21-1Cl+ Hg Cl. -On mixing solutions of hydrochlorate of quinidine and chloride of mercury , the above salt is precipitated as a white powder .
It is slightly soluble in cold water , much more so in hot , especially when acidulated with hydrochloric acid ; but it cannot be conveniently crystallized from this menstruum , as it sometimes separates in resinous masses .
By far the best solvent from which to crystallize is boiling alcohol , in which it is readily soltuble , separating in nacreous scales as the solution cools .
It fuses at 100G under water , but not when dry .
'626 gramme of the above salt , dried at 1000 , yields *507 chloride of silver , which gives of chlorine 20'04 per cent. The formula C40 1124 N2 04 21101 + Hg Cl requires 20'00 per cent. Zinco-hydr-ocklorate of Quinidine , C01H24 , N20,4 21 HC1+2ZaC1 .
A moderately strong solution of chloride of zinc , containing a slight excess of hydrchloric acid , is poured into an alcoholic solution of quinidine , when the double salt precipitates as a granular powder .
It is very slightly soluble either in hot or in cold water , but dissolves readily in dilute hydrochloric acid and in spirit of 50 per cent. , from which latter it crystallizes in a form very similar to that variety of carbonate of lime known as " dog-tooth " spar .
The specimen analysed was crystallized from dilute hydrochloric acid and dried at l00 ? .
-447 gramme gave *4825 gramme chloride of silver , equal to 1193 of chlorine .
This corresponds to 267 per cent. of chlorine .
The formula C40 1124N 2 04 211 Cl+2Zn Cl requires 26X65 per cent. Basic Chloride-of-Zinc Salt , C41124N2 04 , HCI+ZnC1.-The neutral salt described above appears to lose a portion of its hydrochloric acid and chloride of zinc after repeated crystallizations .
A solution of the salt so treated deposits , upon slow evaporation , crystals of considerable size , consisting of hexagonal plates and 'prisms .
After drying at 1000 , these were sul)mitted to analysis ; the zinc and quilnidine were precipitated together by carbonate of soda , and asfter washing well with water , the quinidine was removed by boiling alcohol ; the residuary oxide of zinc was them again washed with water , and ignited in the usual way..7335 gramme of the salt yielded *0680 grarnme of oxide of ' zinc , equivalent to *05456 of metallic zinc , or 7-44 per cent. The formula C 40 -1 N2 04 , 2H C1 +2 Zn Cl requires 12 2 per cent. The formula C40 H121 N2 O , , E Cl + Zn Cl requires 7-58 per cent. Oxalate of Quinidine , C040 1-2 .
N2 01 I-I C2 OV 11O.-The oxalate of quinidine is formed by exactly nieutralizing oxalic acid by quinidine .
It consists of very small brittle crystals , which are almost insoluble in cold , but comparatively soluble in hot water , from which it crystallizes again on cooling .
After being purified by two recrystallizations and dried at 1000 , it was submitted to analysis .
-206 gramme gave -502 carbonic acid and *133 water ; this corresponds to 66 45 per cent. of carbon and 7-17 of hydrogen .
The formula C40 1124 N204,0 1020 04+110 requires 66-67 per cenit .
carbon and 6-88 per cent. hydrogen .
This is evidently , therefore , the neutral oxalate , and differs wholly in appearance and properties from the acid oxalate , C00 H , 2 04 , 120408 + 2Aq , obtained by Van Ileijningen .
Picrate of Quinidine.-Quinidine dissolves in a boiling and not too concentrated solution of picr'ic acid ; but it separates on cooling , not in crystals , but as a resinouis mass .
When dissolved in hot alcobol , it is deposited by evaporation of the solution in resinous nodules , thus very closely resemlbling , the corresponding salt of quiiiiine .
Action of Iodide of Ethyl on Quinidine.-Iodide of ethyl attacks quinidine very readily , so that if the two substances ( the former being in excess ) be heated together in a flask furnished with a perforated cork and lonw tube to condense the iodide of ethyl , combination quickly ensues , and in half an hour the reaction is complete .
Water is then added and the excess of iodide distilled off , the residue dissolved in diluite alcohol , filtered , and allowed to crystallize .
On cooling , the solution becomes semnisolid , from separation of the iodide of ethyl-quinidine in the form of long silky needles .
These are well washed with cold water , in which they are almost insoluble , and then recrystallized from boiling dilute spirit , washed , dried at l00 ?
, and submitted to anialysis .
-5600 gramme yielded -2735 gramme iodide of silver , equivalent .
to -1478 of iodide , or 26 39 per cent. The formula 410 2JN20 4}J requires 26-46 per cent. of iodine .
Platinum-salt of Ethyl-quinidine , Co II N 0 ?
I C1 } 2Pt C12 .
4 IL 2 t24 11c On treating the foregoing iodide with chloride of silver the chlorine replaces the iodinie , tand we obtain chloride of ethyl-quinidine in solution and iodide of silver .
The latter is separated by filtration , and the solutioni , niow free from iodine , is precipitated by the addition of bichloride of platinum .
The platinum-salt separates as a paleyellow powder , almost insoluble either in hot or in cold water , and but sparingly soluble in boiling dilute hydrochloric acid , from which it separates almost completely on cooling .
The specimen analysed was simply washed with water and dried at 100( .
*537 gramme gave 137 metallic platinum , corresponding to 25 61 per cent. 2N The formula C 11H N 04C4 H11c0 2 Pt C12 requires 25'86 per cent. Hydrated Oxide of Ethyl-quinidine .
On treating the iodide of ethyl-quinidine with oxide of silver in slight excess , a solution of the hydrated oxide is obtained .
It is very bitter to the taste , readily attracting carbonic acid from the air , and is of course highly alkaline to test-paper .
On evaporation it does not crvstallize .
Action of Iodlide of E thyl on Ilydrcated Oxide of Etthyl-quinidine .
-When iodide of ethyl and a strong solution of hydrated oxide of ethyl-quinidine are made to react upon each other in a sealed tube at the temperature of 100 ?
, a mass of crystals are produced after digestion for about an hour .
These were extracted from the tube , washed with a little water , dried between folds of filtering-paper , and recrystallized from dilute alcohol .
On analysis , they proved to be nothing more than reproduced iodide of ethyl-quinidine .
*4435 gramme gives 2165 of iodide of silver , correspolnding to *117 of iodine , or 26-38 per cent. The formula C4 215 2"4 } I requires 26A46 per cent. From these experiments it appears that quinidine contains no replaceable hydrogen , and in this respect it agrees with quilline and cinchonine , the alkaloids with which it is associated .
Double Tartrate of Quinidine and Antimony , C40 121N2 04 11 C IH 0 SbO , 8 '0 120 When an excess of quinidine in powder is added to a cold saturated solution of tartar-emetic , and heat applied so soon as the mixture begins to boil , the quinidine pretty rapidly dissolves , whilst at the same time a quantity of oxide of antimony is precipitated .
The solution is filtered whilst boiling , and on cooling the double tartrate of quiniidine and antimony is deposited in very lonig fine silky nleedles , often more than an inch in length .
Any excess of quinidine which has been employed , together with the oxide of antimony which has been precipitated , remains upon the filter .
The double tartrate is but slightly soluble in cold water , but dissolves easily in hot , from which it may readily be crystallized .
It is also very soluble in boiling spirit of wine , from which it is deposited , almost completely on cooling , in tufts of slender needles .
The douible tartrate of quilnidine and antimony was very carefuilly examined for potassa by precipitating the antimoniy by means of suiphuretted hydrogen ; it then left lno perceptible residue on ignition , and a drop of bichloride of platinum gave no precipitate .
It therefore could not contain potassa .
Analysis.-Dried in vacuo over sulphuric acid , it retains , appareitly uncombined , from 5 to 1 per cent. of water , which it loses at the temperature of 1000 .
The salt dried in vacuo gave the following results I. 0 3850 gramme gave 6750 gramme carbonic acid and 1780 gramme water .
II .
2375 gramme gave 4175 gramme carbonic acid and 1270 gramme water .
III .
*5380 gramme gave *1398 gramme of antimolnious acid , Sb 04 .
The compounds , after two recrystallizations and drying at 1000 , gave the following results : IV .
*5815 gramme gave 1P0100 gramme carbonic acid and 2550 gramme water .
V. '5110 gramme gave *893 gramme carbonic acid and -224 gramme water .
VI .
*7195 gramme substance gave *1949 gramme tersulphide of antimony .
This was dried in vacuo and contained 1P3 per cent. of water ; therefore 17195 gramme is equal to *7101 dried at 1000 .
Theory .
-I .
I. II .
IV .
V. C48 = 288 .
47-28 47-8 47-94 47-36 47-66 H29 = 29 .
4176 513 5 94 4-87 4-87 N2= 28. .
4596 ?
o0 8 144..2363 Sb = 120-3 19-74 2053 1961 609-3 100-006 In order to ascertain that the residue upon the filter , in addition to undissolved quinidine , contained precipitated teroxide of antimony , it was washed with hot alcohol and dissolved in strong hydrochloric acid .
This solution gave the characteristic reactions of anti .
money with water and sulphuretted hydrogen .
The mother-liquor , which was quite neutral to test-paper , and from which as much as possible of the quinidine-salt had been separated by concentrationi , was treated by sulphuretted hydrogen to separate the antimony , and was tested for potassa and for tartaric acid , both of which it was found to contain .
The reaction may therefore be represented by the following equation:2 Sb ?
2 }C II4 012+ 040 " -121 N2 04+'l0 C40 , H21 N2 0411 c1 ?
K c142 ?
b. Sb 0 , C8ifI012 + 84 8 24 12 +b 03In order to colnfirm this view of the comiiposition of the salt , some acid tartrate of quinidine was prepared by taking a solution of tartaric acid , dividing it equally into two portions , nieutralizing the one with quinidine , and then adding the other .
This solution was then boiled for some hours with excess of freshly-precipitated oxide of antimony , filtered , and allowed to cool , when the same beautiful salt made its appearanice , idelntical in all its properties with the compounld formed by boiling tartar-emetic with quinidine .
It will be obvious from these results that tartar-emetic , when boiled with quinidine , undergoes a somewhat sinigular and unexpected decomposition , neutral tartrate of potassa and the double tartrate of quinidine and antimony being , formed , while one-half of the antimony of the original salt is precipitated as oxide .
From this and the subsequently to be described double tartrates , the tersulphide of antimony which is precipitated has a light yellow or pale orange colour , and , after being lolng washed with boiling water , still contains some of the base , probably in the state of a salt .
This portion of the alkaloid may , however , be abstracted from the tersulphide of anltimony by digesting it with hot alcohol .
In order to confirm the fact that the compound contained quinidine and not -an altered base , as it may be observed from the analyses given above that the carbon in the double tartrates is somewhat too high , the antimony was removed from a portion of the salt by means of sulphuretted hydrogen , the base precipitated by amnmonia , well washed with water , and crystallized out of spirit ; it was them obtained with the usual crystalline form assumed by quinidilne , viz. 4-sided prisms , and gave the characteristic reactioni with chlorine-water and ammonia .
A platinum-salt also was prepared in the usual way , which , recrystallized from dilute hydrochloric acid , gave the following analytical result : *411 gramme gave *1075 gramme metallic platinum ; this corresponds to 26 16 per cent. C E24 N O , 2H C1 +2 Pt Cl requires 26-81 per cent. The Tartrate of St2ychnine and Antimony , GII1NO H ~CH 0 42 22 24 Sb02 8 It 212 was likewise prepared by adding strychlline to a boiling solution of tartar-emetic .
The same solution of the alkaloid and precipitation of oxide of antimony were observed as in the case of quitnidine .
Oa cooling , the double tartrate was deposited in very brittle needles , much less soluble in water than the corresponding quinidine-salt .
It occasionally crystallizes in leafy plates .
The following results were obtained in the analysis of the salt dried at 100 ?
:I .
*3365 gramme gave *6005 gramme carbonic acid and 133 gramme water .
II .
*6000 gramme gave *148 gramme Sb 04 .
III .
5495 gramme gave *1375 gramme Sb 0 , .
Theory .
---I~~ .
It .
MI .
c0o = 300..48 44 48*7 127 = 27. .
4-36 4-39 N2 = 28. .
4-52 018 = 144. .
23 26 Sb = 120(3. .
19'42 19-47 19'76 100 00 This corresponds with the formula C42 1-122N2 04 11 ~CH 0 Sb ? ?
84 12 ' Some of this salt was also decomposed by sulphuretted hydrogen and treated in the manner described in the case of the quinidine .
It was then obtained in quadrilateral prisms with pyramidal summits , and gave the usual reactions with sulphuric acid and bichromate of potassa .
A platinum-salt of the recovered alkaloid was also prepared and analysed .
Dried at 1000 , -630 gramme gave *1150 grainme of mietallic platinum .
This is equivalent to 18 26 per cenit .
The formula C 42 1122 N204 , 11 1 , Pt Cl12 requires 18527 per cent. Taritrate of Brucine and Antimony , 04 , lla N2081 }C WA 0 Sb02 j84 12 ' The salt was prepared in a precisely similar manner .
It formed short and excessively brittle crystals .
Analysis seems to assign to this salt the same conistitution as those containing quiniidine and strychnine , as may be seen by the following results : I. *284 gramme brucine compoulnd gave 5000 gramme carbonic acid and *1 185 gramme water .
1I .
*4845 gramme yielded These numbers corresponid to the formula C48 H 22N SbO22 C40 17 NO8 H cno SbO 08 81 12 ' Theory .
, ~~ ~ ~~1 .
Ir .
C48 3 288. .
46'43 46 46 1-122 = 22. .
354 31676 N= 14..2-2 .
Sb = 120 3. .
19'39 -l985 022 =1 76. .
28'37 620'3 99'98 It is very remarkable that corresponiding crystalline double tartrates are not obtained by boiling tartar-emetic with many of the other organic bases .
The following have been tried , but unsuccessfully : Quinine .
Aniline .
Cincholiine .
Theimie .
Cinchonidine .
Piperine .
Furfurilie .
|
112293 | 3701662 | Researches into the Chemical Constitution of Narcotine, and of Its Products of Decomposition.--Part I. [Abstract] | 501 | 505 | 1,862 | 12 | Proceedings of the Royal Society of London | A. Matthiessen|George Carey Foster | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 5 | 91 | 1,554 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112293 | null | http://www.jstor.org/stable/112293 | null | null | Chemistry 2 | 94.730186 | Optics | 2.171847 | Chemistry | [
-54.21194839477539,
-60.882110595703125
] | I. " Researches into the Chemical Constitution of Narcotine , and of its Products of Decomposition."-Part I. By A. MATTHIESSEN , F.R.S. , and GEORGE CAREY FOSTER , B.A. Received February 26 , 1863 .
( Abstract .
) An abstract of a considerable portioni of this paper has already appeared in the form of a preliminary notice* of the first results obtained .
The most important additional facts now communicated are the following : The anialysis of five additional specimens of narcotine has confirmed the accuracy of the formula 22 H23 NO7 , which the authors adopted for this base in their previous notice .
The mean results of all their analyses ( ten determinations of carbon and hydrogen and four determinations of nitrogen ) give for the composition of narcotine , Carbon ... ... ... ... ... 63-78 Hydrogen .
576 Nitrogen ... ... .- .
3-32 Oxygen.27'14 100-00 The formula 22 H23 NO ' corresponds to Carbon ... ... ... ... . .
63 92 Hydrog , en ... ... ... ... .
557 Nitrogen ... ... ... ... 3.39 Oxygen.27 12 100-00 The authors had previously stated that mneconin , opianic acid , and hemipinic acid were all decomposed by boiling concentrated hydriodic acid , with evolution of iodide of methyl. .
They now find that hydrochloric acid acts similarly on these bodies , evolving with each of them chloride of methyl .
They suggest the name hypoyallic acid for the acid 0 11 O , formed by the action of hydriodic acid on hemipinic acid* , in order to recall the fact of its containing one atom of oxygen less than gallic acid , C ' H16 O5 .
They obtained the same product by the prolonged action of hydrochloric acid on hemipinic acid ; but by a shorter action an intermediate product was obtained , which , according to a single analysis , appears to contain H8 H8 0 Calculated .
Found .
-C ... ... ... .
96 ... 57'14.5665 H8 8 ... ... . .
4-76 ... ... . .
517 4 ... 64 ... 3810 ... . .
8180_4 ... ... . .
68 .
10000 This substance is an acid of much greater stability than bypogallic acid ; it crystallizes in long , thin , transparent prisms , which are anhydrous , and are almost insoluble in cold water , slightly soluble in boiling water , but dissolve more readily in alcohol and ether .
At X Proc. Roy .
Soc. vol. ; i. p. 58 .
about 200 ?
C. this acid sublimes unchanged , and it may be heated to 245 ' without melting or becoming coloured ; it dissolves in strong sulphuric acid , and is precipitated urnaltered on addition of water .
It gives no coloration with sesquichloride of iron ; with nitrate of silver it gives a white precipitate which slowly blackens on boiling .
Its formation from hemipinic acid may be expressed by the equation C"O110 0I1 C+=E0O2++C GE13 Cl+C8 118 0 ' .
Hemipinic acid .
This substance has the composition of methyl-hypogallic acid ; but its great stability , as compared with hypogallic acid , makes it appear improbable that such is its true constitution .
Nascent hydrogeni evolved from sodium-amalgam and water , or from zinc and dilute sulphuric acid , converts opianic acid into rneconin , C"O 1-0 " ( } ' + 1_12 C"10 11 " '+ 112 0 Opianic acid .
Mecoriin .
Hemipinic acid is unaltered by nascent hydrogen .
Aqueous hydrochloric acid decomposes cotarnine at 140 ?
C. into chloride of methyl , and a substance which the authors call hydrochlorate of cotarnamic acid and represent by the formula " J1 Hl3 NO ; , HCl , supposing it to be formed according to the following equation : 12,113 NO3 + 11 ' 0+2 IICl=C " l13 NO ' IIC1 + CH3 Cl. Cotarnirie .
Hydrochlorate of cotarnamic acid .
The formula proposed does not agree perfectly with the results of several anialyses , which are accordant among themselves , and is given as provisional only .
Calculated .
Found rw ~~~~~(meanl ) .
C " .
132 ... .
1 50'87 ... .
49-98 H".14 ... .
540 ... .
5.70 N 14 ... .
5 40 571i 0 ' 64 ... .
24-65 ... .
24-61 Cl ... 35 ... .
13 68 ... .
1 4300 Cll 11NO1,3C4 ... .
259 5 ... .
100 00 ... .
100 00 This body crystallizes in small silky nieedles of a pale yellow colour ; it is partially decomposed , losing hydrochloric acid , when dissolved in pure water , but dissolves unchanged in water containing a trace of free hydrochloric acid .
Alkalies , or alkaline carbonates or sul .
phites , throw down from the aqueous or acid solution an oran , gecoloured granular precipitate ( cotarnamic acid ?
) free from hydrochloric acid ; this precipitate dissolves in excess of alkali , giving a solution which quickly becomes dark brown by exposure to air ; with hydrochloric acid , it regenerates the originial crystalline compound ; it dissolves slightly in water , with a bright oraiige colour that is visible even in very dilute solutions .
The slightly acidulated solution of the hydrochlorate is pale yellow when pure , but acquires a deep .
green colour in the air .
A few drops of uitric acid added to a hot solution cause it to appear of an opake crimson colour by reflected light , though the liquLid is still transpareint when examined by transmitted light .
Nitrate of silver added in quantity more than sufficient to precipitate the chlorine is quickly reduced .
The compound acquires a fine crimson colour when evaporated nearly to dryness on the water-bath , with a slight excess of dilute sulphuric acid .
Hydriodic and diluted sulphuric acids decompose cotarnine at a high temperature in the same way as hydrochloric acid .
The products so formed have not been isolated , but were converted into hydrochlorate of cotarnamic acid .
The authors conclucde by offering some suggestions towards the interpretation of the results they have obtained .
Only the most important points discussed by them will be briefly indicated here .
They suppose that when opianic acid is converted into meconin by the action of nascent hydrogen , or into meconin and hemipinic acid by the action of potash * , a substance containing C " II " 0 ' may possibly be the immediate product of the reaction , and that this body-bearing the same relation to mieconin that glycol , C ' IF ' 02 , does to oxide of ethylene , C E4 0 , or maninite , C. 1I O ' , to mannitan , C'1 -may give rise to meconin by subsequent loss of the elements of water .
Making this supposition , the two reactions in question may be represented by the equations ( 1),. .
10uClo 45 + I2 =cl " O12 0 Opianic acid .
IHypothetical hydrate of meconin .
( 2 ) 2 ( C " 1I10 0 ' ) +H0= C"O H12 0 ' + Co 1100 o6 Opianic acid .
Hypothetical Hemipinic hydrate of meconin .
acid .
Thus viewed , both transformations appear strictly analooous to the known transformations of oil of bitter almonds and many other substanices ; e. g. , ( 1 ) .
7 H. C 10 , +1 -2 _ 407 I9 0 ( Friedel ) Oil of bitter Benzylic almonds .
alcohol .
( 2). .
2(C7 1160 ) + 112 o0 C HI 0+ ?
C EIs 02 ( Cannizzaro ) Oil of bitter Benzylic Benzoic almonds .
alcohol .
acid .
and may be regarded as supporting the views of Berthelot , who has suggested that opianic acid ought to be classed as an aldehyde rather than as a true acid .
With regard to the constitution of hemipinic acid , the authors suppose that it may be a dimethylized derivative of a bibasic but tetratomic acid , c8 IF 06 ( analogous to tartaric acid , Co 116 06 ) , the two atoms of methyl occupying the places of the two atoms of hydrogen , which , though outside the radical , are incapable of being replaced by metals : hemipinic acid would thus be comparable to Wurtz 's ethyllactic acid , the body at one time described by Butlerow as valerolactic acid .
An analogy is further pointed out between the derivatives of malic acid and the substances obtained from cotarnine .
This alnalogy becomes apparent on comparing the two following series of formulae Cotarnic acid el .
l H12 C0 ' 11 O ' Malic acid .
( ?
) Cotarnamic } .
f1 H13 NO ' C " HI NO4 Aspartic acid .
lIydrochlorate ~ ' ldohoaeo of cotarnamic } C " HI " NO'6 .
CI1 C 11HN4 .
HCi { Hydrochlorate of acid ... ... .{ aspartic acid .
Cotarnine , or f Malanile , or phemethyl-cotarC 0 " I11 ( CH-3 ) NO3 C 114 ( 06 1 ) NO ' nyl-malimide nimide ... .
J The authors initend to colntinue their experiments .
|
112294 | 3701662 | Postscript to a Paper Read January 15, 1863, on the Formation of Fibrin from Albumen | 505 | 507 | 1,862 | 12 | Proceedings of the Royal Society of London | Alfred Hutchison Smee Jun. | fla | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 32 | 837 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112294 | null | http://www.jstor.org/stable/112294 | null | null | Chemistry 2 | 58.72845 | Physiology | 18.449939 | Chemistry | [
-59.18086624145508,
-28.09428596496582
] | II .
Postscript to a Paper read January 15 , 1863 , " On the Formation of Fibrin from Albumen .
" By ALFRED HUTCHISON SMEE , Jun. Communicated by ALFRED SMEE , Esq. , F.R.S. Received March 2 , 1863 .
Since the paper was read before the Royal Society the following additional facts have been elicited .
Fibrin was obtained from 1863 .
] 505 serum when subjected to oxygen gas , when acetic acid was added to it , although another portion of the same serum had refused to yield it without that addition .
In this experiment the acetic acid should be added until the serum is either neutral , or produces a slightly acid reaction on test-paper .
Care must be taken in these experiments to prevent the temperature rising too high , for a coagulation then takes place .
If blood-cells be present in the serum , the addition of acetic acid attacks the cells in preference to the alkalies of the serum ; and on subsequent exposure to a temperature of 100 ?
F. during the period it is under the influence of oxygen , the whole is transformed into a semisolid mass .
It is a curious fact that serum which has been placed on a dialyser for the removal of the salts by Graham 's method was not improved in its power of producing fibrin , over serum which had not been submitted to that treatment previous to its oxidation .
On the other hand , albumen purified from salts by Graham 's method , and then subjected to the influence of oxygen , yielded the largest amount of fibrin .
By this method it is most probable that I should have been able to have transformed the whole of the albumen into fibrin , had not an accident unfortunately brought the experiment to a termination .
Nevertheless , although the experiment was not continued long , half the albumen was changed into fibrin .
When experimenting upon albumen nearly free from alkalies and alkaline salts , great care must be taken to keep the temperature as low as possible .
I found that a temperature between 80 ?
and 90 ?
F. was the best , for above 98 ?
the albumen had a very great tendency to coagulate .
WThen albumen was placed in a tube which contained about an equal bulk of oxygen , and in which a platinized platinum wire had been inserted extending the whole length of the tube , to facilitate the action of the oxygen on the albumen , and which tube was subsequently sealed and placed in a water-bath of 98 ?
F. , no fibrin made its appearance even after the lapse of 36 hours , but in its place a small quantity of an amorphous material subsided to the bottom of the tube .
When , however , a tube of similar size was filled with albumen having free access to the air , and then placed on the same water-bath for an equal length of time , on the surface of the albumen which this tube contained small masses of 506 fibrin were formed , which had an appearance identical with that of blood-fibrin under the microscope , giving a conclusive proof to my mind that , during the formation of fibrin by the action of oxygen on albumen , a volatile constituent is formed and carried off by the excess of oxygen which passes into the albumen in solution .
The following are the chief physical and chemical properties of the fibrin artificially formed by the action of oxygen on albumen : It has a lighter specific gravity than albumen , being always found floating on the surface of the albumen , provided it is free and not entangled or attached to the side of the vessel or platinized platinum wire that has been inserted in the albuminous solution .
It has a fibrinated appearance under the microscope , and is capable of being teased out into filaments in the same manner as bloodfibrin .
Acetic acid completely dissolves it after some time .
Soda and potash cause it to swell up and dissolve .
Concentrated solution of ammonia , after the lapse of some hours , causes the fibrin to swell up in a gelatinous mass , similar to that which occurs when blood-fibrin is submitted to the same reagent .
A hot or cold solution of nitrate of potash does not dissolve it when it is digested in that menstruum for some hours .
With Millon 's test it becomes of a brick-red colour .
With nitric acid a bright yellow colour became visible .
Fibrin heated with hydrochloric acid gave a blue colour , and subsequently dissolved , giving a blue tint to the liquid .
An acid solution of acetate of lead caused both blood-fibrin and fibrin artificially prepared to swell up and become translucent after digestion for a certain period .
|
112295 | 3701662 | On Diffusion of Vapours: A Means of Distinguishing between Apparent and Real Vapour-Densities of Chemical Compounds | 507 | 511 | 1,862 | 12 | Proceedings of the Royal Society of London | J. A. Wanklyn|J. Robinson | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0106 | null | proceedings | 1,860 | 1,850 | 1,800 | 5 | 53 | 1,113 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112295 | 10.1098/rspl.1862.0106 | http://www.jstor.org/stable/112295 | null | null | Chemistry 2 | 45.801606 | Thermodynamics | 42.94401 | Chemistry | [
-23.671682357788086,
-51.225250244140625
] | III .
" On Diffusion of Vapours : a means of distinguishing between apparent and real Vapour-densities of Chemical Compounds .
" By J. A. WANKLYN and J. ROBINSON , Esq. Communicated by Dr. FRANKLAND .
Received March 10 , 1863 .
The density of the vapour given off when a chemical compound is heated is not necessarily the vapour-density of that chemical com pound ; sometimes it is only the mean density of the products of decomposition .
Some of the best-known substances , such as hydrated sulphurous acid , ammoniacal salts , and pentachloride of phosphorus , suffer decomposition when they are vaporized , and thus have an apparent vapour-density , which is in reality nothing more than the mean density of the products of their decomposition .
We recognize such cases-in which the apparent is not the real vapour-density-by making a diffusion-analysis of the vapours .
This method of solving questions of the kind was proposed by one of us two years ago* .
In carrying it out practically , it was resolved from the first not to diffuse through a porous diaphragm , but to recur to Graham 's original method , namely , to let our vapours diffuse through a simple aperture or through a short tube .
Independently of the experimental difficulties attending the use of a porous diaphragm at high temperatures , there is a fatal objection to it , founded upon the inconclusiveness of the results obtained in such a way .
Our resolve to avoid porous substances was not by any means shaken by Pebal 's memoirt on the diffusion of chloride-of-ammonium vapour through asbestos ; for what is more likely than that a finely-divided silicate ( a salt of an acid of indefinite capacity of saturation ) should decompose ammoniacal salts at elevated temperatures ?
The apparatus used in our experiments is of the sinplest kind .
It is represented in the drawing , and consists of two glass flasks , the necks of which do not fit air-tight : the narrow tube proceeding from the upper one is fused to the flask .
The lower flask is for the reception of the vapour to be operated upon ; the upper flask is for the atmosphere into which the vapour is to be diffused .
The atmoPlayfair and Wanklyn on Vapour-densities , Transactions of Roy .
Soc. of Edinburgh , 1861 , vol. xxii .
part 3 .
p. 458 .
In this paper it was proposed to extend to vapours what had previously been applied to gases .
One of the earliest , perhaps the earliest example of a precise diffusion-analysis of a gas was given by Frankland in his research upon the isolation of ethyl ( see Quart .
Journ. Chem. Soc. vol. ii .
p. 285 , 1850 ) .
After describing his diffusion-apparatus and its use in the case of ethyl , Frankland proceeds , " This method might in almost every case be employed with advantage to determine whether or not any specimen of gas be simple or mixed .
" t Ann. de Ohim .
et de Phys. January 1863 .
sphere of dry air , or other suitable gas , is kept constantly renewed by the transmission of a slow stream of gas , which enters the upper fbntodI bb / r flask by the narrow tube above , and passes out by the space between the two necks , which , as we have said , do not fit air-tight .
When in use , the whole apparatus is kept at a temperature above the condensing-point of the vapour by means of an air-bath .
After a diffusion has gone on for a sufficient length of time the apparatus is allowed to cool , and the contents of the lower flask are analysed , by which means it is seen whether diffusion has effected any alteration in the composition of the vapour .
We have used a lower flask of about 500 cubic centimetres capacity , with a mouth 10 millimetres in diameter ; the capacity of the upper flask was 100 cubic centimetres .
The first substance taken for experiment was sulphuric acid , which is converted at high temperatures into vapour of sulphuric anhydride and vapour of water .
Inasmuch as vapour of water is lighter than vapour of sulphuric anhydride , the former should diffuse more rapidly than the latter .
Accordingly , the residue after diffusion should be richer in sulphuric anhydride than the acid before diffusion .
In one experiment we took an acid composed of 95 Mono-hydrated sulphuric acid .
5 Water .
100 1863 .
] 509 2o After diffusion for an hour at about 520 ?
C. , the residue was composed of 60 Mono-hydrated sulphuric acid .
40 Sulphuric anhydride .
100 In another experiment we took an acid containing 99 Mono-hydrate .
1 Water .
100 and after diffusion for a shorter time at 445 ?
C. found the residue to consist of 75 Mono-hydrateo 25 Anhydride .
100 In both cases the residues after diffusion fumed strongly on exposure to the air , and consisted partly of crystals and partly of liquid .
The substance next submitted to diffusion was pentachloride of phosphorus , which is decomposed by heat into terchloride and free chlorine .
The pentachloride which we used gave no reaction with iodide of potassium and starch , and therefore contained no free chlorine ; it gave no precipitate with corrosive sublimate , and therefore contained no terchloride of phosphorus .
An analysis of it gave Percentage of chlorine=846 7 The formula requires ... 85 13.In one experiment we diffused into carbonic acid gas* for threequarters of an hour at about 300 ?
C. , and afterwards dissolved the contents of the lower flask in water , and precipitated with corrosive sublimate , with the addition of a little hydrochloric acid .
'0175 gramme of calomel was obtained .
In another experiment ( also into carbonic acid ) the time of diffusion was two hours , temperature 300 ?
C. , quantity of calomel obtained '0285 gramme .
These two results leave no doubt as to the existence of terchloride of phosphorus in the residue after diffusion ; for the reduction of corrosive sublimate to calomel cannot be otherwise explained .
Moreover , the presence of free chlorine in the diffused gases was shown by the reaction with iodide of potassium and starch .
We are continuing this research , and hope to lay before the Society the results of an examination of the most prominent cases of so-called abnormal vapour-density .
|
112296 | 3701662 | On a Simple Formula and Practical Rule for Calculating Heights Barometrically without Logarithms | 511 | 517 | 1,862 | 12 | Proceedings of the Royal Society of London | Alexander J. Ellis | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0107 | null | proceedings | 1,860 | 1,850 | 1,800 | 7 | 104 | 2,187 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112296 | 10.1098/rspl.1862.0107 | http://www.jstor.org/stable/112296 | null | null | Formulae | 36.231859 | Astronomy | 26.430855 | Mathematics | [
62.37751388549805,
-2.398818254470825
] | IV .
" On a Simple Formula and Practical Rule for calculating Heights baronietrically without Logarithms .
" By ALEXANDER J. ELLIS , B.A. , F.C.P.S. Commnunicated by Dr. NEIL ARNOTT , F.R.S. Received February 23 , 1863 .
The following formula and table for calculating heights barometrically without logarithms will be found to give the same results as Laplace 's formula up to 30,000 feet , andc the table can be readily extended if required .
Let L degrees be the mean latitude of the two stations , I =2 6257cos2L , G=1+0 0026257cos2L , R=20888629 , the number of feet in the earth 's radius .
At the lower station .
H feet , its height above the sea , H"t=12 H R , B units of any kind , height of barometer , uncorrected , Bt.1 1 % 5 ) 3 3 .
$p3 3 , corrected , A-deg .
Fahr. , A ' deg. Cent. , A"l deg. Reaum .
, temperature of air , M , , 7}Mr , , I , Mit , , , , P , , of mercury .
Jt the upper 8tation .
It , It " , 6 , bs6a ) a , a " M , m , m " in the same sense .
Then h-H1= [ 52400 B-b + e-2-35 .
( M-m ) ] 836 +A a B+6~~~~~~0 + 001 .
( h-Hi ) l+h"-H " , .
X O. ( a ) where M-mk=0 , when B , 6=B ' , b6 , and 2 35 ( M-m)=4.23 .
( Ml-mr)=5'29 .
( M1'-m"l ) 836+A+a-500+A'+a ' 400+A"f+a"t 900 500 400 The numbers c , 1 , hft , Hlf are to be taken from the table on the next page , as will appear by the following examples .
2o Ex. 1 .
Height of Mont Blanc above Geneva from the observations of MM .
Bravais and Martins , August 29th , 1844 .
Af 193 B 729-65 mm. M ' 18 6H 1335-33 af7-6 b 424 05 min4-2 L 46 500 0 B+b 1153170 22 81 O09 511-7 B-Z 305 60 x4 23 x 142 p 96-4 q 13 305-6x52400 + 1153 7 141l181 x 511 7 .
500 =13880'0 =14448 5 272-9 c for 1300 10 8 A " for 15000 1 61-6 diff. for 880 12 diff. for 800 ' 103 6 -p P9 -H " for 150l , E 141181 18-7 -q h-H=14459 0 difference of level .
Result by Laplace 's formula 14459-4 .
Table of Corrections .
Feet .
c Diff. for h " + Diff. for LLI 100 feet .
H"l100 feet .
_+ 11000 030 06 0 05 0 ?
0 ?
00 900 2265 2000 + 0-3 0-20 0-20 0-2 5 85 2-61 3000 2-3 0 -41 0-43 0-02 10 80 2-49 4000 6-4 0 72 0477 0 04 15 75 2229 5000 13-6 72 P2 0-04 20 70 2-03 6000 2434 0854 1 72 0056 21 69 iP97 7000 39-8 2-07 2-35 0'07 22 68 1-91 8000 60 5 2768 3-06 0-08 23 67 1P84 9000 87-3 3-35 3-88 0 09 24 66 1-77 10000 120-8 4-16 4.79 0 10 25 65 1P70 11000 162 45 04 5 79 0 11 26 64 1-63 12000 212-8 6-01 6-89 0-12 27 63 1-56 13000 272 9 707 0'13 28 62 1-48 14000 343-6 8-27 9 38 0 14 29 61 1340 15000 426-3 8 55 10 77 0.14 30 60 1-33 16000 521-8 9-55 12-26 0 16 31 59 1-24 17000 631-6 10-98 13-84 0-16 32 58 1-16 80 ?
00 675566 1240 15 51 0'17 33 57 1P08 19000 8997 1 14635 17-28 0 18 34 56 0.99 20000 1059-6 16-05 19-15 0219 35 55 0.91 21000 1239-9 20123 21 11 0 21 36 54 0-82 22000 1442-2 223 23-17 0-21 37 53 0173 23000 1667-8 22556 23133 0-22 38 52 0-64 24000 1919-2 25714 27-58 0'23 39 51 0 55 25000 2198-8 27396 29792 0 24 40 50 0 46 26000 2508-8 31400 32-36 0 24 41 49 0 37 27000 2852 3 37-96 34'90 0n26 42 48 0-27 28000 3231 9 41399 37-53 0-27 43 47 0.18 29000 3651*8 41-99 40-26 0-28 44 46 0 09 30000 4115-4 4636 4309 45 45 000 ... ... .409.45 45.00 Ex. 2 ' .
Rush 's balloon ascent , September 10th , 1838 ( see Meteorological Papers by Admiral FitzRoy , No. 9 , p. 19 ) .
A 60 Bt 30 496 in .
E0a5 bf 10-830 L 52 836 B ' ?
+ ' 41b326 1 0-64 901 B'--6 ' 19 666 x 27 q 17-3 19 666x52400 ?
* 41-326 27116x901 .
900 =24935-8 =27146 1 2198'8 c for 25000 34'9 kf for 27000 1814 diff.for-65 03 diff. for 100 27116-0 1821-q h-11=27164-0 Laplace 's formula gives the same result .
As the British highlands do not exceed 5000 feet in altitude , and lie near the parallel of 561 north latitude , the corrections will nearly destroy each other .
The following simple rule will therefore suffice for calculating all British heights : " Multiply the difference of the barometers by 524 , and divide the product by the sum of the barometers , retaining three decimal places .
Multiply this quotient by the sum of the temperatures of the air increased by 836 , and divide the product by 9 , keeping one decimal place .
For aneroid and corrected mercurial barometers , the quotient is the height in English feet .
For uncorrected barometers , subtract 21 times the difference of the temperatures of the mercury .
" Ex. 3 .
Height of Ben Lomond ( see Col. Sir H. James 's Instructions for taking Meteorological Observations , App. ) .
A 59-0 B 29'890 in .
M 60'8 a 47-8 6 26'656 m 49 3 836'0 B+b 56 546 M-m I1F5 942'8 B-b 3'234 x 22 28'7 3'234 x 524 *.56'546 x 942'8 *-9-28'7=3110'5=h-H .
The height by Laplace 's formula is 3110 8 , by levelling 3115'8 .
The accuracy of the presenit formula is only initended to be tested by Laplace 's , and it will be wrong to at least the same extent .
Very good results may also be obtained by neglecting 11 " , which is always very small , and transposing the terms h1 ' and -2 35 ( M-m ) ; thus h-I=(52400O j+c +h " ) 8369+A+a +001 .
( h-H)-2:(M-m ) , where 2is writteil for 2335 to compensate for omitting to multiply the latter by ( 836 ?
A+ a ) +900 .
This approximate form gives rise to the following practical rule for determining heights under 10,000 feet , embodying so much of the Table of corrections as is necessary for that purpose .
" , Multiply the difference of the barometers by 52400 , and divide by the sum of the barometers .
If the number of clear thousands in the quotient be 1 , 2 , 3 , 4 , 5 , 6 , 7 , 8 , 9 , 1 0 , add 0 , 0 5 , 2 7 , 7 2 , 14-8 , 26-1 , 42 2 , 63,6 , 91P2 , 125-6 and 0-2 , 0 5 , 0)8 , 1 1 , 16 , 2-1 , 2'9 , 31 for every additional hundred .
Then multiply the result by the sum of the temperatures of the air increased by 836 , and divide the product by 900 .
To this quotient add for lat ... .
0 , 10 , 20 , 30 , 32 , 34 , 36 , 38 , 40 , 42 , 44 , ,subtract for lat. 90 , 80 , 70 , 60 , 58 , 56 , 54 , 52 , 50 , 48 , 46 the numbers ... .
2-6 , 2 5 , 2 0 , 1P3 , 1P2 , 1 0 , 0 8 , 0 6 , 0 5 , 0 3 , 01 for every clear thousand it contains .
For alneroid and corrected mercurial barometers this result is the height in English feet .
For uncorrected mercurial barometers , subitract 2-a times the difference of the temperatures of the mercury .
" The barometers may be expressed in any units .
If the temperatures are expressed in degrees Centigrade , use. .
500 , 500 , 412 .
degrees Reaumur , use ... ... . .
400 , 400 , 52 , in place of. .
836 , 900 , 212 , which are only suited for degrees Fahrenheit .
The rule and the other numbers remain unaltered , and the result is in English feet .
" Ex. 4 .
Height of Guanaxuato in Mexico .
A 77 5B 30-046 M 77a L 21 a 70 36 23-660 m 70 31 2-0 836-0 B+b 53-706 M-m 7-2 x 6-8 983-8 B-b 6-386 21 q 13-6 p 18-0 6 386 X 52400 '53'706 6260 5x 9838 +900 =623017 =6842 5 26 & 1 for 6000 136 q 317 diff. for 230 181 0-p 6260 5 h-H=6838 1 Result by Laplace 's formula 6838 2 .
These results are obtained by transforming Laplace 's formula as , follows .
The original expression in the Me'c .
Cel .
vol. iv .
p. 293 , reduced to English measures and the present notation , is h-H=60158-71.(1+0-002845 cos 2L ) .
836 + A+ ) F !
h-HIVI _ Ii II x jI + og+o ) ( log log ) ?
j+I.0868589jJ which Deleros has transformed ( in 'Annuaire Meteorologique de la France ' for 1849 ) to the equivalent of h-H= 60158171 x [ log B-log Z-0 0000389278 .
( M-m ) ] x 836+A+a xGx Il h-H+52251 1* 900 it + Rj The last factor may be split into the two ( 1+ 52251 ) * ( 1+hi ) without sensible error .
Then , since 60158'71 x ( I+ 251)=60309l19 and 60309-19 x 0'0000389278=2-34770 , if we put h-il for the product of the three first factors on the right-hand side in ( c ) , we find h-H= [ 60309 19 .
( log B-log b)-2 34770 .
( M-m ) ] .
836+A+a h2 ~~~~900 d+ hoH X 26257 cos 2L+ RH-il ' Putting 2-35 for 2-34770 , and 1 , h " , II " for their values , this form ( d ) will be identical with ( a ) , provided that 60309 19 .
( log B-log 6 ) = 52400 .
B-6+e Now putting B-b=yB , we have B-b yIy1 y2+ 1 y3+ 1 y4 +* * ) Z B-6 .
y+y -y B+6 2-y 2 log B-log 6=log1 ( =.+ 1y2+ 1y3+ 1y4+ 4 )=(d ) where it is the modulus of the tabular logarithms , and 12 8 always a colnvergent series as y is always a proper fraction , and small when y is small , as it is for moderate heights .
Hence 6030919 .
( logB-log 6)=6030919 x 2pu , -b +60309 19.pd =52384B+ +c ' .
The constant 52384 has been changed to 52400 to facilitate calculation and to divide the correction for the first two thousand feet , and c ' has consequently been altered to c , the tabular values of which were calculated as follows .
Put =52400Bb=52400 .
2Y B+62 whence 2x 52400+x.(f ) Then ( e ) becomes x+c=60309 19.(logB-logb)=-60309 19log(I-y ) .
( g ) Make x successively = 1000 , 2000 , &c. up to 30,000 , and find the corresponding values of y from ( f ) and c from ( g ) .
As the differences in the values of c are not uniform , slight errors may arise from neglecting second differences in interpolation , but they can scarcely even affect the result by a single unit , and may therefore be safely disregarded .
Laplace 's formula itself cannot be depended on within much larger limits .
The Table of corrections and tranlsformation of Laplace 's formula here given allow of the following simplification in the logarithmic calculation of h-H .
Let log n= log [ log B-log 6-0 00004 .
( M-m ) ] +I18261420+log(836 ?
A+a ) =log [ log B-log 6-0000007 .
( M ' -m/ n ) ] + ?
2 0814145+log(.500+AAf a ' ) =log [ log B -log 6-0O00009 .
( M"f imn ) ] +0 1783245 + log ( 400 + A"f + a " ) , then h-I-I=n+ *001 .
nl+h"/ -H"l , where 1 8261420+log900=2-0814145+log,500 =21783245 + log 400= 47 7803845 =log 60309-19 .
This form requires less previous preparation , avoids the logarithms of numbers near to unity as 1+ 00 A 1 ) , and allows of the use of foreign data to obtain the result in English feet , so that it only becomes necessary to reduce the height of the lower station to EDglish measures .
|
112297 | 3701662 | Bessel's Hypsometric Tables, as Corrected by Plantamour, Reduced to English Measures and Recalculated | 517 | 517 | 1,862 | 12 | Proceedings of the Royal Society of London | Alexander J. Ellis | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0108 | null | proceedings | 1,860 | 1,850 | 1,800 | 1 | 4 | 92 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112297 | 10.1098/rspl.1862.0108 | http://www.jstor.org/stable/112297 | null | null | Biography | 58.813158 | Tables | 30.790513 | Biography | [
65.75043487548828,
6.525728225708008
] | V. " Bessel 's Hypsometric Tables , as corrected by Plantamour , reduced to English Measures and recalculated .
" By ALEXANDER J. ELLIS , Esq. Communicated by Dr. NEIL ARNOTT .
Received February 23 , 1863 .
These Tables , with the preliminary explanations respecting their correction and reduction , have been , by direction of the Council , cornmunicated to Admiral FitzRoy for insertion in the " Meteorological Papers published by Authority of the Board of Trade , " and will appear in the twelfth Number of the series .
|
112298 | 3701662 | On Ozone. [Abstract] | 517 | 523 | 1,862 | 12 | Proceedings of the Royal Society of London | E. J. Lowe | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 6 | 97 | 2,260 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112298 | null | http://www.jstor.org/stable/112298 | null | null | Chemistry 2 | 35.655556 | Chemistry 1 | 17.832938 | Chemistry | [
21.070220947265625,
8.773078918457031
] | 1 .
" On Ozone .
" By E. J. Lows , Esq. , F.R.A.S. , F.L.S. Communicated by Sir J. F. W. HErSCHEL , Bart. Received March 16 , 1863 .
( Abstract .
) This paper consists of two parts , viz. -1 .
On the precautions necessary in ozone observation , and on certain corrections requisite before the actual amount can be determinedo 2 .
The discovery of dry ozone powders as a substitute for the ordinary tests ; an investigation into the ozone paper tests of M. Schinbein and Dr. Moffat , the determination of a proper formula for the tests , with an account of various observations and experiments made on the subjecte PART I : At the last Meeting of the British Association I read a paper on the precautions and corrections requisite in order that a more perfect knowledge of ozone might be obtained .
These precautions comprise uniformity of observation , each observer using the same box and the same tests , suspended at the same height , and as nearly as possible placed under the same circumstances .
The corrections necessary are --lst , For the velocity of the air ; 2nd , for the height of the barometer ; 3rd , for temperature ; 4th , for the hygrometrical state of the air ; 5.th , for elevation above the ground .
1 .
Velocity of the Air.-The greater the speed the more ozone will be apparent , and this seems to be owing more to the increased velocity of the air than to a greater proportion of ozone .
2 .
Height of the Barometer.-It is found that during the last four years , With the barometer at 281 inches the amount of ozone was 5*7 , g.3 29 , , 9 , , 3.5 30 , , , ) , , 301 , 0*4 A law as regards ozone and pressure is clearly apparent ; but as the barometer falls for wind , the excess at low pressures is no doubt partly due to the increased velocity of the air .
There is more ozone with the wind between W.S.W. and S.S.E. than when between N.N.W. and E.N.E. , and the barometer is half an inch lower with S.W. winds than with N.E. winds .
3 .
Temperature.-Temperatures between 30 ?
and 40 ?
will give less ozone than when between 40 ?
and 50 ?
, and the latter less than when between 50 ?
and 60 ? .
The same holds good when the ozone box is artificially warmed .
This does not extend to very high temperatures , because the great dryness of hot weather is against the action of ozone on the tests .
4 .
2'oisture.-Increase of moisture up to a certain point is favourable to the colouring of the tests , beyond which it operates unfavourably ; for when the air is completely saturated with moisture , the effect of ozone is at its minimum .
5 .
Altitude.-The higher the test is hung the darker will be the colour obtained .
The difference is as 4 to 6 between 4 feet and 35 feet above the ground .
There are yet several other circumstances to be mentioned : I. Hour of the Day.-The difference between the ozone readings at night and in the daytime areIn June and July an excess at night of 01 In August and September , , 0'4 In October and November , , 05 In December and January , , 08 In February and March , , 07 In April and May , , 07 the average excess of the summer months being only one-half of that which occurs in winter , 2 .
Direction of the Wind.-There is most ozone with the wind between S. and S.W. , and least when between N. and N.E. 3 .
Protection of the test from light.-It is absolutely requisite that the test should be in a dark box ; and no box has been found to answer so well as that constructed by myself , and known as Cs Lowe 's Ozone box , " an account of which has been furnished to the Royal Society* and to the British Association .
This box , if freely exposed , and made to veer with the wind , so as always to present the opening to the direct current , is everything that could be desired .
The foregoing observations will be sufficient to show that precautions are requisite in these records , and that certain corrections are necessary before we can declare whether ozone is present in a certain fixed amount , or whether it changes from hour to hour .
These corrections have yet to be found out ; those for the height of the barometer and the force and direction of the wind will be considerable .
PART II .
The ozone tests heretofore used have appeared to me to be unsatisfactory , and , on close examination , I found them to be faulty in many respects .
The paper used had a glaze upon it , which prevented the solution from penetrating it ; substances , moreover , ha d been used in its manufacture which acted injuriously on the tests .
Again , the starch of commerce was found to be impure ; it is manufactured with lime , sulphuric acid , and chlorine , substances fatal to these tests .
The iodide of potassium was also impure ; and there has been a want of uniformity in the proportions of starch and iodide of potassium employed by different observers .
Having found out that the starch of commerce was impure , I procured a jar of wheat-starch in the wet state before any chemicals had been used .
This was steeped in distilled water , which was changed every two days until quite sweet to the taste , and , although by a long process , a chemically pure starch was thus obtained .
Sir John Herschel suggested trying other vegetable starches ; I therefore made starch from rice , potato , sago , and wheat .
I obtained chemically pure iodide of potassium from Mr. Squire of Oxford Street , who forwarded me two samples made expressly for these experiments , the one prepared with water , the other crystallized several times from alcohol .
On the recommendation of Dr. R. D. Thomson , 15 grains of prepared chalk have been added to each ounce of air-dried starch to prevent it from becoming sour from any moisture that might be contained in it ; subsequent observations have proved that this is absolutely requisite for uniformity of effect , as the intensity of action depends upon the amount of water contained in the starch , which is apparent from the following experiment : Tests made with air-dried starcha .
Without further drying became coloured in 5 minutes .
F3 .
After further drying by fire-heat for 1 minute became coloured in 7 minuteso y. After further drying by fire-heat for 3 minutes became coloured in 9 minutes .
B. After further drying by fire-heat for 10 minutes became coloured in 13 minutes .
e. After further drying by fire.heat for 30 minutes became coloured in 20 minutes .
r. With chalk added became coloured in 20 minutes .
With regard to the calico or paper used for the tests , both stained when impure .
However , Mr. Joseph Sidebotham of the Strine Works prepared for me some chemically pure calico , and I was also enabled to procure a very porous chemically pure paper , both of which answer perfectly .
Having succeeded with the-ozone slip tests , I tried as a first experiment a mixture of 10 parts of starch to 1 of iodide of potassium as a " dry-powder test ; " this , when well mixed in a mortar , was bottled ready for use .
A small portion was placed in the open air , and ten minutes ' exposure showed that powder tests were an undoubted success , being more sensitive than the test slips .
My next determination was what strength would colour quickest , and accordingly a number of strengths were prepared , varying in the proportions from 1 of iodide of potassium and 1 of starch up to I of iodide of potassium and 30 of starch , the starch used being made from wheat .
From these experiments it was found that the proportion of 1 of iodide of potassium to 5 of starch was invariably the darkest , the degree of darkness diminishing in either direction when other strengths were used ; thus 1 of iodide of potassium to 4 of starch , or 1 to 5 ?
, were neither so dark as with a strength of 1 to 5 .
On repeating these experiments with potato-starch , the proportion that coloured soonest was 1 to 2 } ; and this second series of experiments proved that with each starch a special formula is requisite .
My next experiments were with the view of ascertaining the effect of various acids and chemical substances on the ozone powder tests .
For this purpose I procured a number of cups for solutions , and small pill-boxes to hold the powder tests , and these were placed together under separate bell-glasses .
The result was that the following coloured the powder tests very rapidly:-Hydrochloric acid , nitric acid , nitrous acid , chloride of lime , phosphorus , iodine ( in scales ) iodine ( dissolved in alcohol ) , carbonate of iron on which sulphuric acid was poured , carbonate of iron on which glacial acetic acid was poured , limestone on which sulphuric acid was poured , limestone on which glacial acetic acid was poured , matches lighted under the bell-glasses .
The following did not colour the tests:-Sulphuric acid , glacial acetic acid , carbonate of lime , carbonate of iron , ammonia , matches not lighted .
The substances used in the manufacture of ordinary starch of commerce gave the following : Chloride of lime coloured the tests instantaneously .
Sulphuric acid did not colour the tests .
Lime did not colour the tests .
Lime and sulphuric acid mixed coloured the tests rapidly .
There are advantages in the powders over the ordinary tests .
They are more sensitive , and therefore more rapidly acted upon ; they retain their maximum colour , not afterwards fading , as with the tests of Schinbein and Moffat .
( However , my calico and porous-paper tests are not nearly so liable to fade , owing to the solution penetrating into the fabric used , instead of being merely a surface-covering .
) There is also a more important advantage still to be mentioned from the use of powders .
By the aid of powder tests we shall ascertain what colours the tests ; in the experiments it was found that a different colour was imparted to the powder , and that the colour penetrated deeper with some substances and acids than with others , so that differences of effect took place , from which the different materials used might be recognized .
Thus:1 .
Iodine , although coloured a brown-black , was merely a surface colouring , below the powder remained colourless .
2 .
Phosphorus , bluish black on the surface only , below almost colourless .
3 .
Chloride of lime , deep brown on the surface only , the powder below slightly yellow .
4 .
IHydrochloric acid , grey-pink on the surface only , the powder beneath orange .
5 .
Nitric acid , dark-red brown extending slightly into the powder , beneath that colourless .
6 .
Carbonate of iron with glacial acetic acid , yellowish brown to the thickness of cardboard , below that buff .
7 .
Limestone with sulphuric acid , pale brown to the thickness of cardboard , beneath .
slightly coloured .
8 .
Carbonate of iron with sulphuric acid , black to the depth of a quarter of an inch .
9 .
Nitrous acid , dark brown more than the eighth of an inch deep , beneath yellowish brown .
10 .
Nitric acid mixed with exposed ozone powder , blue-black to the sixth of an inch deep , below that reddish brown .
1 .
Nitric acid mixed with unexposed ozone powder , blue-black to the sixth of an inch deep , below that reddish brown .
These experiments may require some modification , yet they point out the fact that striking differences are apparent , differences which must open up a new method of investigating ozone .
Not only have the tests hitherto used been made without due regard to the pureness of the chemicals and fitness of the material used , but the paper box in which they have been kept is not sufficient for their perfect preservation ; a dark , dry , air-tight box is essential and this should not be opened in a room where there is iodine , chlorine , nitric acid , phosphorus , hydrochloric acid , or other chemicals likely to be injurious to the tests .
I am now manufacturing the tests , which will be distributed by Messrs. Negretti and Zambra , and I have constructed a proper box in which in future they will be sent .
|
112299 | 3701662 | On the Equations of Rotation of a Solid Body about a Fixed Point. [Abstract] | 523 | 524 | 1,862 | 12 | Proceedings of the Royal Society of London | William Spottiswoode | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 2 | 8 | 243 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112299 | null | http://www.jstor.org/stable/112299 | null | 111,999 | Formulae | 76.52001 | Fluid Dynamics | 18.863221 | Mathematics | [
58.55112075805664,
-32.10578918457031
] | II .
" On1 the Equations of Rotation of a Solid Body about a fixed Point .
" By WILLIAM SPOTTISwooDE , M.A. , F.R.S. Received March 21 , 1863 , ( Abstract .
) In treating the equations of rotation of a solid body about a fixed point , it is usual to employ the principal axes of the body as the moving system of coordinates .
Cases , however , occur in which it is advisable to employ other systems ; and the object of the present paper is to develope the fundamental formule of transformation and integration for any system .
The integrals found areP-=:a l_ O cos am ( , / ( S+ ) ^O co .
sin am ( 7k'-(S+O)h t+f ) ; = / S2)H0 am ( , --/ C1 k_-(s + )h t +f ) where 0 , 01 , 02 are the roots of the cubic ( S +0)3S(S+0)2+S(S+0)-v=0 , V being the determinant of the system A , B , C , -F , --G , -H , S the sum of A , B , C , and S that of the corresponding inverse quantities .
Moreover P1 , q1 , r1 are linear functions of p , q , r ( the components of rotation about the axes for which A , B , C , &c. are calculated ) , the coefficients of which are determined in the paper itself .
|
112300 | 3701662 | On the Fossil Human Jawbone Recently Discovered in the Gravel near Abbeville | 524 | 529 | 1,862 | 12 | Proceedings of the Royal Society of London | William B. Carpenter | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0111 | null | proceedings | 1,860 | 1,850 | 1,800 | 6 | 53 | 1,959 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112300 | 10.1098/rspl.1862.0111 | http://www.jstor.org/stable/112300 | null | null | Geography | 45.638427 | Headmatter | 28.637534 | Geography | [
-55.91258239746094,
53.05344772338867
] | III .
" On the Fossil Human Jawbone recently discovered in the Gravel near Abbeville , " in a Letter to the President , by W. B. CARPENTER , M.D. , V.P.R.S. Received April 16 , 1863 .
University of London , Burlington House , W. April 16 , 1863 .
DEAR MR. PRESIDENT , -I esteem it a privilege to have it in my power to communicate , through you , to the Royal Society some particulars of the important discovery just made by M. Boucher de Perthes , of a human maxilla in one of the gravel-beds near Abbeville also yielding the now well-known flint implements .
Having been informed of this discovery a few days since , whilst staying in Paris , I became additionally desirous of carrying out my previous intention of stopping at Abbeville on my way homewards ; and accordingly , after a short visit to Amiens , -which gave me the opportunity of disinterring for myself a small but well-characterized flint implement from the gravel-pit of St. Acheul , -I proceeded on the afternoon of Monday last to Abbeville , where I was received with the greatest kindness and attention by M. Boucher de Perthes .
The history of his discovery is given in the following extract from the local journal 'L'Abbevillois , ' by which it will be seen that the specimen in question was removed by M. Boucher de Perthes himself from the bed in which the first indications of it had been found by the workman employed in that part of the excavation:"A la fin de mars dernier , le terrassier Halatre , travaillant a cette career , vint lui apporter avec un silex taille un petit fragment d'os qu'il y avait egalement recueilli .
Ayant debarrasse ce fragment du sable qui le couvrait , M. de Perthes aper9ut un dent fort endomtnagee , mais qu'il n'en reconnut pas moins pour un molaire humaine .
" II suivit immediatement Halatre a Moulin-Quignon , v4rifia la place d'oW venait la hachette et la dent , s'assura que cette place etait net de tout infiltration ou introduction secondaire et fit continuer la fouille .
" Elle no produisit ce jour-la aucun resultat nouveau .
" Convaincu que quelqu'autre debris du corps d'ou provenait cette molaire devait se trouver la , M. Boucher de Perthes recom .
manda aux terrassiers de no rien derarger de ce qu'ils pourraient remarquer pendant son absence , mais de le prevenir sans retard .
En effet , le 28 mars le terrassier Vasseur vint lui dire que quelque chose ressemblant a un os paraissait dans le bane .
" Rendu sir les lieux , M. de Perthes trouve le terrain comme l'avait dit Vasseur .
L'extremite de l'os enferme dans sa gangue se montrait d'environ deux centimetres .
" Voulant l'avoir entier , M. de Perthes fit , a l'aide d'une pioche , degager les alentours et , a sa grande satisfaction , il put le retirer du bane sans le rompre .
" I1 no s'etait pas trompe dans ses previsions .
La dent avait annonce la tate , et dans le morceau qu'il venait d'extraire , il reconnut un machoire humaine.-Un grand problem etait resolu .
" A quelques centimetres de ce fossile humain , le premier peut-etre dont la position geologique eut ete aussi nettement constatee , car , par un autre circonstance heureuse , les temoins ici no manquaient pas , etait un hache en silex egalement engagee dans le bane , d'oi , sir l'invitation de M. Boucher de Perthes , M. Oswald Dimpre , jeune archeologue et dessinateur habile bien connu des savants qui ont visit Abbeville , l'enleva mais non sans s'aider aussi de la pioche .
" Un chose qui frappa tous les spectateurs , ce fut la parfaite identite de patine ou de couleur de cette machoire , des silex taille 's et des cailloux roules , avec le bane qui les contenait , couleur brune , presque noire , contrastant singulierement avec la teinte jaune ou grise des banes superienrs et la craie blanch sir laquelle elle repose .
" Mesure prise de chacune des couches superieures , la machoire fossile etait ainsi que les hachettes a4 metres 52 centimetres * de la superficie et tout pres de la craie .
" Ce bane de Moulin-Quignon , place ' sir le plateau qui domnine la vallee , se trouve a 30 metres au-dessus du niveau de la Somme et de la mer. " The particulars I have now to communicate as the result of my own personal examination should , I think , most completely satisfy any unprejudiced person that , on the one hand , the specimen cannot have been a " plant " contrived by the workman , and , on the other , that it could not have found its way into the bed in which it was discovered by any disturbing agency subsequent to the original deposition of that bed * .
When M. Boucher de Perthes had the kindness to place in my hands this precious fragment-which consists of the right half of the lower jaw , containing three teeth-I was immediately struck with its almost black colour , its solidity , and its weight : all these peculiarities ( which are in marked contrast to the characters of the bones ordinarily found in these gravel-pits ) being obviously due to one and the same cause , viz. metallic ( ferruginous ?
) infiltration .
The ordinary flints , and the flint implements obtained from the same deposit , several of which are in the museum of M. de Perthes , are all of them characterized by a like depth of ferruginous tint , which is not seen in any of those taken from any other part of the same pit , or from any other gravel-pit yet opened in the neighbourhood of Abbeville .
As to the anatomical characters of this jaw , I should not wish , without a more careful comparative examination of the specimen than I had the opportunity of making , to give any decided opinion ; but my impression is that they differ very decidedly from those of the same bone in any race at present inhabiting Western Europe .
I was struck with the thickness of the bone , the great breadth of the ascending ramus , but especially with the extraordinary breadth and depth of the groove between the ramus and alveolar border , in which I could almost lay my little finger .
The jaw would appear to be that of a person advanced in life ; and the tooth originally found , which very probably belonged to the other half of the same jaw , seemed to me to have been " endommagee " by caries during life rather than by subsequent violence .
9 , < Fig. 1 .
M. Boucher de Perthes had the kindness to give me the accompanying sketch of the specimen ; and I can testify to the accuracy of its representation of the general form of the bone .
On Tuesday morning I repaired , in company with M. Boucher de Perthes , to the gravel-pit of Moulin-Quignon ; in which he showed me , as nearly as he could , the situation in which this most interesting relic had been found .
Unfortunately there had occurred , a few days previously to my visit , a slip of the overlying strata , by the debris of which the exact spot was covered ; but a part of the same deposit was visible at a horizontal distance of a yard or two , so that I could indubitably verify its position and its general characters .
This deposit , distinguished from every other by the extreme depth of its ferruginous tint ( which corresponds exactly to that of the bone ) , lies at the very bottom of the pit , in immediate contact with the subjacent chalk , as shown in the accompanying representation of the section ( also kindly given to me by M. Boucher de Perthes ) , to the general accuracy of which I can bear the most explicit testimony .
I myself took away from this deposit some specimens of the small rounded flints which it contains , and which will serve to show you this peculiar tint .
Fig. 2.-Section of the Strata in the Gravel-pit of Moulin-Quignon , near Abbeville .
--------_ t. in .
1 .
Vegetable mould ... ... ... ... ... I0 2 .
Undisturbed subsoil , consist~q3~~~ ing of grey sand with broken flints ... ... ... ... ... ... ... ... ... ... 2 3 / ----^- < ~ 5/ ~ . ?
./ 3 .
Yellowish argillaceous sand , with large flints but little - ... ... ... .::- : ... ... .:__- : =l rolled , resting on a layer of -:- ... ... ... ... .--.------::-grey sand ... ... ... ... ... ... ... ... 50 ------4 .
Yellow ferruginous sand , containing smaller and more rolled flints , and divided by a second layer of less yellow sand ... ... ... ... ... ... ... ... ... ... 57 5 .
Argillaceous sand of a deep brown or almost black hue , sticking to the hand and staining it , containing small I~- ; -~-~=----=L----_ _ _flints more rolled than those -_ ___ of the upper strata.-N.B .
The white spaces left in this layer mark the position of the jaw and of the flint hatchet found in contiguity with it .
18 15 6 ... ... .
6 .
Chalk .
These facts must be admitted , I think , to exclude any possibilitY of doubt as to the truly fossil character of this bone .
Its peculiar condition could not have been produced by any artificial means at present known , and most assuredly indicates that it must have been long buried in the deposit from which its metallic impregnation has been derived * .
That it could not have found its way into that deposit in any other mode than by original imbedding , may be fairly concluded from the entire absence of the least indication of disturbance in the superjacent strata , which are most regularly superposed ( as seen in the accompanying section ) to a depth of more than 15 feet .
This complete regularity of superposition in the strata of the gravel-pits of Moulin-Quignon has , I understand , been already verified by numerous experienced geologists , whose testimony upon such a point is of far higher value than mine ; but it is so obvious that I cannot imagine the least doubt to remain in the mind of any intelligent observer who may visit the locality and examine its condition for himself , of the jaw having been imbedded in the lowest stratum before the deposition of the superincumbent layers .
I have further to point out , that as the gravel-bed of MoulinQuignon is about 100 feet above the present level of the river , it corresponds in position with the upper gravel of St. Acheul , not with the lower gravel of Menchecourt .
If , therefore , we accept the conclusions of Mr. Prestwich as to the relative ages of these gravels , this human jaw was buried in the very oldest portion of the earliest of these fluviatile deposits , and therefore dates back to the very remotest period at which we have at present any evidence of the existence of Man .
Believe me , dear Mr. President , Yours faithfully , WILLIAM B. CARPENTER .
|
112301 | 3701662 | On the Diurnal Inequalities of Terrestrial Magnetism, as Deduced from Observations Made at the Royal Observatory, Greenwich, from 1841 to 1857. [Abstract] | 529 | 532 | 1,862 | 12 | Proceedings of the Royal Society of London | George Biddell Airy | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 4 | 54 | 1,416 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112301 | null | http://www.jstor.org/stable/112301 | null | 108,798 | Meteorology | 65.691354 | Tables | 11.728666 | Meteorology | [
45.34917068481445,
10.447806358337402
] | I. " On the Diurnal Inequalities of Terrestrial Magnetism , as deduced from observations made at the Royal Observatory , Greenwich , from 1841 to 1857 .
" By GEORGE BIDDELL AIRY , F.R.S. , Astronomer Royal .
Received April 8 , 1863 .
( Abstract .
) The author describes this paper as one of the class which gives the epitomized results of long series of voluminous observations and laborious calculations , of which the fundamental details have been 1863 .
] 529 printed in works specially devoted to these subjects .
It exhibits in curves the diurnal inequalities of terrestrial magnetism , as obtained by the use of instruments essentially the same , through the whole period of seventeen years , during the last ten years of which the magnetic indications have been automatically recorded by photographic self-registration , on a system which has been continued to the present time , and is still to be continued .
From the last months of 1840 to the end of 1847 , the observations were made by eye , every two hours .
From the beginning of 1848 , for the declination and horizontal force magnetometers , and from the beginning of 1849 , for the vertical force magnetometer , the magnetic indications are recorded by Mr. Brooke 's photographic apparatus .
In preparing the reductions of the magnetic records from 1848 to 1857 ( which are printed in the " Results of Magnetical and Meteorological Observations for 1859 , " bound in the volume of 'Greenwich Observations , ' 1859 , and also issued separately ) , the days of unusual magnetic disturbance had been separated from the rest , and the reductions applied to the mass so diminished .
For unity of plan , it appeared expedient to follow the same course for the reductions from 1841 to 1847 .
In consequence of this , the numbers which are used here differ in some cases by small quantities from those printed in the ' Greenwich Magnetical Observations from 1841 to 1847 .
' The numbers in the reductions from 1848 to 1857 are adopted without change .
The author remarks that , taking the number of omitted days as a rough measure of the amount of magnetic disturbance , there is no appearance of decennial cycle in their recurrence , and no distinct relation to the magnitude of diurnal changes .
The author then proceeds to the description of the curves .
The first four sheets contain the curves in which the horizontal abscissa represents the declination at each hour as compared with the mean for the twenty-four hours and the vertical ordinate represents the horizontal force at each hour as compared with the mean for the twenty-four hours .
On the different sheets the days are differently grouped , thus:-On sheet I. all the observations at each nominal hour throughout the year are combined ; this sheet contains the separate curves for 1841 , 1842 , 1843 , 1844 , 1845 , 1846 , 1847 .
On sheet II .
similar curves are formed for 1848 , 1849 , 1850 , 1851 , 530 1852 , 1853 , 1854 , 1855 , 1856 , 1857 .
On sheet III .
all the observations at each nominal hour through all the months January from 1841 to 1847 are combined to form the January curve ; all those through the months February to form the February curve , and so on .
On sheet IV .
similar month-curves are formed from the period 1848 to 1857 .
It is remarked that the origin of coordinates necessarily represents the mean declination and mean horizontal force in each month .
The author then points out that the means for each month are themselves subject to an annual inequality , which can be ascertained with little difficulty .
The values of these inequalities are exhibited , for declination and horizontal force , separately for the period 18411847 and for the period 1848-1857 ; those in the first period far exceed in magnitude those in the second ( as holds also with regard to all the diurnal inequalities ) .
If we wished to exhibit the hourly state of magnetism , as referred to the mean state given by the supposition of uniform secular change of normal magnetism , we ought to apply these quantities with sign changed , to the origin of coordinates in each curve , in order to form a new origin of coordinates .
For the year-curves , the numbers destroy each other , and no new origin of coordinates is produced ; for the month-curves , however , they shift the origin materially .
The author does not perceive that any facility for theoretical reference or other advantage is gained by this step .
On examining the year-curves , it is seen that from 1841 to 1848 their magnitude very slowly increases , with a small change of form , but from 1848 to 1857 their magnitude very rapidly diminishes , with a great change of form .
Some great cosmical change seems to have come upon the earth , particularly affecting terrestrial magnetism .
On comparing these year-curves with the month-curves , especially with those for the period 1848-1857 , it appears that the change of the year-curves from 1848 to 1857 nearly resembles that of the month-curves from summer to winter ; and the author points out as a possible step to a physical explanation of the change from 1848 to 1857 , that the magnetic action of the sun upon the earth 's southern hemisphere may have remained nearly unaltered , while that on the northern hemisphere may have undergone a great diminution .
The author then alludes to the curves representing the hourly 1863 .
] 531 state of vertical force , as referred to the mean on each day .
The force is here represented by a simple ordinate .
The grouping is made by years and by months in the same manner as for the curves already mentioned .
The month-curves of the two periods ( 18411847 and 1848-1857 ) differ , in the magnitude and change of magnitude of the ordinates , and in the place and change of place of node .
The year-curves of the two periods have some very remarkable differences .
From 1847 to 1849 the magnitude of the ordinates increases sensibly ; from 1849 to 1850 still more ; it then remains nearly stationary .
In 1846 the descending node is at 11h nearly ; in 1847 it is at 9h nearly ; in 1849 at 7h nearly ; in 1850 at 5h ; in 1851 at 4h ; and there it continues with little alteration .
It is important to observe that , though the instrument was changed in 1848 , the change in the place of the node did not then occur suddenly ; it had begun with the old instrument , and continued to advance gradually for several years with the new instrument .
The author states that he had verified the correctness of the node in the first period from other observations , but he had not succeeded in finding observations corresponding in date with those of the latter period .
The paper is followed by eight sheets of curves , as follows : I. Diurnal Curves of combination of Declination and Horizontal Force .
( 1 ) Mean of all the days in each year ( separately ) , 1841-1847 .
( 2 ) Mean of all the days in each year ( separately ) , 1848-1857 .
( 3 ) Mean of all the days in the aggregate of the same nominal months ( separately ) through the period 1841-1847 .
( 4 ) Mean of all the days in the aggregate of the same nominal months ( separately ) through the period 1848-1857 .
II .
Diurnal Curves of Vertical Force .
( 5 ) Mean of all the days in each year ( separately ) , 1841-1847 .
( 6 ) Mean of all the days in each year ( separately ) , 1849-1857 .
( 7 ) Mean of all the days in the aggregate of the same nominal months ( separately ) through the period 1841-1847 .
( 8 ) Mean of all the days in the aggregate of the same nominal months ( separately ) through the period 1849-1857 .
53
|
112302 | 3701662 | On the Direct Transformation of Iodide of Allyle into Iodide of Propyle | 533 | 534 | 1,862 | 12 | Proceedings of the Royal Society of London | Maxwell Simpson | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0113 | null | proceedings | 1,860 | 1,850 | 1,800 | 2 | 41 | 595 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112302 | 10.1098/rspl.1862.0113 | http://www.jstor.org/stable/112302 | null | null | Chemistry 2 | 88.517708 | Thermodynamics | 10.445095 | Chemistry | [
-34.0219841003418,
-65.06671905517578
] | II .
" On the direct Transformation of Iodide of Allyle into Iodide of Propyle .
" By MAXWELL SIMRPSON , M.B. , F.R.S. Received April 7 , 1863 .
Iodide of allyle , as is well known , combines directly with two equivalents of metallic mercury , a well-defined crystalline compound being formed .
Would it be possible to make the same body combine with two equivalents of hydrogen , and thus to open a direct passage from the allylic to the propylic series of compounds ?
Indirectly this transformation has been already effected by M. Berthelot through the intervention of propylene gas .
In order to determine the above point , I submitted iodide of allyle to the action of hydriodic acid gas .
On passing this gas into the iodide , the latter became strongly heated and black from the liberation of a large quantity of iodine .
As soon as the gas was observed to pass unabsorbed through the liquid , the latter was allowed to cool , and filtered through asbestos .
It was then decolorized by agitation with a dilute solution of caustic potash , dried over chloride of calcium , and distilled .
Almost the entire quantity passed over between 90 ?
and 95 ?
Cent. The portion distilling between 92 ?
and 94 ?
Cent. I collected apart and analysed .
The numbers obtained correspond with the composition of iodide of propyle , as will be seen from the following table : Theory .
Per cent. Experiment .
C ... .
36 21-18 21 29 ... ... .
7 4'11 4-16 I ... ... . .
127 74-71 170 100-00 The specific gravity of the iodide is 1 73 at zero .
In order to satisfy myself that the body I had in my hands was really an ether of propylic alcohol , I endeavoured to prepare that alcohol from it .
This I succeeded in doing in the following manner:-About 60 grammes of the iodide were added to an equivalent of oxalate of silver contained in a flask surrounded by water .
The mixture became strongly heated from the violence of the reaction , and the decomposition was soon complete .
It was then digested with ether .
On submitting the ethereal solution to distillation , I observed that , as soon as the ether had passed over , the thermometer rose rapidly to 186 ?
, and that the entire liquid , previously dissolved in the ether , distilled over between that temperature and 197 ?
Cent. This was no doubt oxalate of propyle .
On heating this body in a retort with solid caustic potash , I obtained a volatile distillate .
This I then dried over chloride of calcium , and in order to secure its complete dehydration , treated it with a small piece of sodium .
On re-distilling , I found that the entire liquid passed over between 83 ?
and 88 ?
Cent. The portion distilling between 85 ?
and 88 ?
gave on analysis results corresponding with the formula of propylic alcohol , as will be seen on inspecting the following table : Theory .
Per cent. Experiment .
C6 ... ... . .
36 60'00 59'21 IH ... ... . .
8 13-33 13-47 O0 ... ... . .
16 26*67 60 100'00 By treating this body with iodine and phosphorus , I succeeded in regenerating iodide of propyle .
This is a very ready method of preparing propylic alcohol when a large quantity is not required .
|
112303 | 3701662 | On the Distillation of Mixtures: A Contribution to the Theory of Fractional Distillation | 534 | 535 | 1,862 | 12 | Proceedings of the Royal Society of London | J. A. Wanklyn | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0114 | null | proceedings | 1,860 | 1,850 | 1,800 | 2 | 22 | 542 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112303 | 10.1098/rspl.1862.0114 | http://www.jstor.org/stable/112303 | null | null | Chemistry 2 | 49.683945 | Thermodynamics | 30.876401 | Chemistry | [
-15.655731201171875,
-34.45127487182617
] | III .
" On the Distillation of Mixtures : a Contribution to the Theory of Fractional Distillation .
" By J. A. WANKLYN , Esq. Communicated by Dr. FRANKLAND .
Received April 17 , 1863 .
There are many points in the boiling of mixtures which are obscure .
The tension of the vapours at the temperature whereat the mixture boils , and the proportions in which the constituents of the mixture are present , are not the only factors which determine the relative rates at which the constituents distil .
There have , for instance , to be taken into account the adhesion of the liquids to one another , and the vapour-densities of these liquids .
On the present occasion I have to call attention to the influence of this latter element , which influence seems to have been lost sight of by most of those who have applied themselves to this subject .
Leaving out of account for a moment the influence of adhesion , and simplifying the influence of the proportion in which the ingredients are present by taking equal weights of two liquids of different boiling-points , we may set down the rates at which these ingredients will distil as determined by the tensions of the liquids and the densities of the vapours .
In the first instant of time the quantity of each ingredient which distils will be found by multiplying its tension at the boiling-point of the mixture by its vapour-density .
It thus appears that the liquid with the highest tension will not of necessity distil the quickest , for what the other liquids want in tension they may make up by the greater density of the vapours which they give off .
And so when we mix a more volatile with a less volatile liquid and proceed to distil the mixture , we shall now and then find that the less volatile liquid distils faster than the more volatile one .
I will here bring forward an experiment to illustrate this point .
Vapour-density .
Methyl-alcohol boils at 66 ?
C ... ... ... 1 107 Iodide of ethyl boils at 72 ?
C ... ... ... 5-397 I took 18 grammes of methyl-alcohol and 17 grammes of iodide of ethyl , mixed them , and distilled off rather more than one-third of the mixture .
The distillate consisted of 6'0 grammes methyl-alcohol , 8§ 7 grammes iodide of ethyl , 14'7 which shows that in this case the less volatile constituent had boiled the faster , the less volatile iodide of ethyl having a very much higher vapour-density than methyl-alcohol .
It will be obvious that when the vapour-densities and tensions are inversely proportional , the mixture must distil over unchanged .
This influence of vapour-density goes a great way to explain why homologous bodies are so difficult of separation by means of fractional distillation .
The more complex the formula the higher the boiling-point , but also the higher the vapour-density , and therefore the greater the value of the vapour .
Why oils , &c. distil so readily in steam is also explained ; for aqueous vapour is one of the lightest , while oily vapours are generally heavy .
|
112304 | 3701662 | On the Arrangement of the Muscular Fibres of the Ventricular Portion of the Vertebrate Heart; with Physiological Remarks | 536 | 536 | 1,862 | 12 | Proceedings of the Royal Society of London | James Pettigrew | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0115 | null | proceedings | 1,860 | 1,850 | 1,800 | 1 | 6 | 118 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112304 | 10.1098/rspl.1862.0115 | http://www.jstor.org/stable/112304 | null | null | Biography | 58.947055 | Neurology | 31.635268 | Biography | [
-55.8245849609375,
19.08155059814453
] | IV .
" On the Arrangement of the Muscular Fibres of the Ventricular Portion of the Vertebrate Heart ; with Physiological Remarks .
" By JAMES PETTIGREW , M.D. Communicated by Professor GOODSIR .
Received March 26 , 1863 .
This paper is a revised version of a previous one , having the same title , which was communicated to the Society on the 22nd of November , 1859 , and formed the substance of the Croonian Lecture delivered by the author on the 19th of April , 1860 .
The author has now inclucded the results of his researches on the structure of the ventricular portion of the heart in fishes , reptiles , and birds .
|
112305 | 3701662 | On Spectrum Analysis; with a Description of a Large Spectroscope Having Nine Prisms, and Achromatic Telescopes of Two-Feet Focal Power. [Abstract] | 536 | 538 | 1,862 | 12 | Proceedings of the Royal Society of London | John P. Gassiot | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 15 | 678 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112305 | null | http://www.jstor.org/stable/112305 | null | null | Optics | 38.647385 | Biography | 19.165508 | Optics | [
22.17095947265625,
-29.976533889770508
] | I. " On Spectrum Analysis ; with a Description of a large Spectroscope having nine Prisms , andAchromatic Telescopes of two-feet focal power .
" By JOIIN P. GAssIOr , F.R.S. Received April 21 , 1863 .
( Abstract .
) The author , after briefly alluding to the discoveries of Fox Talbot , Wheatstone , Foucault , Kirchhoff , and Bunsen , and the importance of spectrum analysis , states that among the numerous spectroscopes which were exhibited in the International Exhibition of 1862 , there was one which had been specially constructed by Messrs. Spencer , Browning , and Co. , philosophical instrument makers in London , which at the time excited considerable attention .
This spectroscope had two prisms , with a magnifying power of 40 , its definition being remarkably clear .
The skill evinced by Mr. Browning in the construction of this instrument induced the author to have one made in which still better effects might be produced , by multiplying the number of prisms and increasing the magnifying power , with the necessary precaution to avoid as much as possible loss of light .
After a few preliminary trials , it was finally arranged to use nine prisms , which is the number that can be applied with this instrument , although the arrangements are such as to allow the whole or any less number to be used with the utmost facility .
Verniers and micrometer screws are attached to the knife-edges of the slit through which the light to be observed is admitted to the collimator and to the telescope , also to the large circle of the instrument ; these enable the observer to note the exact position of the lines observed in the spectrum from whatever source it is obtained , and thus enable him to repeat and verify previous results with the utmost exactitude .
When two small prisms , one refracting and the other reflecting , are fixed outside the knife-edge slit , spectra obtained from three separate sources can be simultaneously examined ; and an illuminated micrometer scale enables the observer to note the precise relative position of the lines in the three spectra without reference to or reading off from the verniers .
By this arrangement a most interesting spectacle may be obtained , showing in the uppermost portion of the field of view the spectrum of thallium , strontium , or lithium , ignited in the flame of a Bunsen 's gas-burner ; in the centre of the field the spectrum of the same substance in the oxyhydrogen blowpipe , and at the bottom one in the voltaic arc ; each successive spectrum there exhibits an increased number of lines .
With this spectroscope the author has ascertained that the green line of thallium , so celebrated for its integrity , and hitherto believed .
to coincide with one of the lines in the spectrum of baryta , does not so coincide ; for by employing the nine prisms with a power of 80 on the telescope , the thallium line is clearly seen to occupy a dark space in the baryta spectrum , close by the side of the bright line with which it was supposed to coincide .
A range of prisms is adapted to the telescope , the highest of which , when used in conjunction with the amplifying lens , gives a power of 110 with good definition .
The author states that the results already obtained by this instrument have been so satisfactory as to leave him no cause to regret the time that has been devoted to , or the expense that has been incurred in the construction of this truly beautiful apparatus .
A full description of the instrument is introduced , with several diagrams showing the construction and adaptation of the different parts of the apparatus , and two drawings , one showing the general appearance of the instrument when prepared for observation , and the other representing it as seen when viewed from above .
|
112306 | 3701662 | The Bakerian Lecture: On the Direct Correlation of Mechanical and Chemical Forces | 538 | 550 | 1,862 | 12 | Proceedings of the Royal Society of London | Henry Clifton Sorby | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0117 | null | proceedings | 1,860 | 1,850 | 1,800 | 13 | 124 | 5,352 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112306 | 10.1098/rspl.1862.0117 | http://www.jstor.org/stable/112306 | null | null | Chemistry 2 | 29.691487 | Thermodynamics | 29.329896 | Chemistry | [
-3.468702554702759,
-9.25036907196045
] | II .
THE BAKERIAN LECTURE.- " On the Direct Correlation of Mechanical and Chemical Forces .
" By HENRY CLIFTON SORBY , F.R.S. Received April 29 , 1863 .
Perhaps it may be thought somewhat strange that a geologist should undertake such a subject as the correlation of forces ; but the very fact of my being a geologist has led to the investigations of which I now purpose to give a short preliminary account .
In studying general chemical and physical geology , and especially in examining the microscopical structure of rocks , I have for a number of years been greatly perplexed with a class of facts which pointed both to a mechanical and to a chemical origin .
At first I attributed them either to a mechanical or a chemical action , or to the two combined ; but in most cases no satisfactory explanation could be given .
At length , however , facts turned up which altogether precluded any supposition not involving direct correlation ; for they most clearly indicated that mechanical force had been resolved into chemical action in the same way as , under other circumstances , it may be resolved into heat , electricity , or any other modification of force , as so ably described by Grove in his work ' On the Correlation of Physical Forces .
' The effect of pressure on the solubility of salts has already been made the subject of speculation and experiment * , and a considerable number of facts have been described , showing that pressure will more or less influence such chemical actions as are accompanied by an evolution of gas , so that it may cause a compound to be permanent which otherwise would be'decomposed* ; but the results were for the most part so indefinite and unconnected , or of such a character , that Mr. Grove does not allude to the direct production of chemical action from mechanical force .
That this is , however , extremely probable will be evident to all who have considered the manner in which the various physical forces are correlated ; for if mechanical force can be produced by chemical action , why should not the converse be true ?
In this paper I shall endeavour to show that such is really the fact , and that in some cases the mechanical equivalent of the chemical force may be determined .
In order to obtain the necessary great pressure , I have made use of a modification of the method employed by Bunsen ; but instead of filling the tubes at the ordinary temperature of the atmosphere and then gently heating them for several hours , I in the first instance filled them at a temperature 10 ?
or 20 ?
C. lower , so that when finally sealed up they contained considerably more liquid than they could hold without pressure at the ordinary temperature of the atmosphere at the time being ; and thus , by its tendency to expand , this liquid and anything enclosed in the tube were subjected to a very great pressure .
By keeping the tubes in various parts of the house , according as the weather varied , I have been able to maintain for several weeks or even months a pressure of , for instance , about 100 atmospheres , as measured by means of a capillary-tube pressure-gauge enclosed within the larger tube .
Since in all cases I had a second tube which from first to last was treated precisely like the other , pressure excepted , I have been able to determine the effect produced by the pressure with very considerable accuracy-at all events so as to leave no doubt whatever about the general facts .
At the same time I wish it to be understood that the results described below must be looked upon only as approximations to the truth .
I will first call attention to the well-known influence of pressure on the fusing-point of various substances , since it is a connecting link between well-established facts and those I am about to describe .
Bunsen* and IHopkins t have shown that substances which expand when fused have their point of fusion raised by mechanical pressure ; that is to say , since mechanical force must be overcome in melting , the tendency to melt must be increased by heat before that opposition can be overcome ; and the pressure required to keep them solid at any temperature above their natural point of fusion may be looked upon as the mechanical representative of the force with which they tend to fuse at that temperature .
Professor VW .
Thomson has shown that , on the contrary , water , which expands in freezing , has its point of fusion lowered by pressure ; that is to say , since mechanical force must be overcome in crystallizing , crystallization will not take place under increased pressure unless the force of crystalline polarity be increased by reducing the temperature .
Thus , calculating from his experiments and from the known latent heat of ice , and assuming that no heat is gained or lost by contact with external objects , if we had 1 part of ice and 100 of water at 0 ?
C. , and then applied a pressure of 103 atmospheres , the ice would , as it were , dissolve in the water , the whole would become liquid , and the temperature be reduced to -'792 ?
C. ; or , in other terms , at that temperature the tendency to crystallize is exactly counterbalanced by that pressure .
Now I find that similar principles hold true with respect to the solubility of salts in water .
If , when they dissolve , the total bulk increases , pressure reduces their solubility ; whereas if the bulk decreases , pressure makes them more soluble ; in other words , solution or crystallization is impeded by pressure according as mechanical force must be overcome in dissolving or in crystallizing .
Various authors have written on the volume with which salts enter into solution ?
; but since the subject before us requires a different class of facts to be taken into account , I shall base my conclusions on my own experiments .
The volume with which salts exist when in solution , assuming that of the water to remain unchanged , varies greatly in the case of different salts , and also according to the amount in solution and the temperature .
Thus , taking sal-ammoniac as an example , when there are 3 per cent. in solution the volume is as if it expanded 3'40 per cent. on dissolving ; whereas when 25'55 per cent. are in solution , the expansion is 11'36 per cent. ; and when nearly concentrated at about 13 ?
C. , an additional quantity expands on dissolving 15 78 per cent. In by far the greater number of cases , however , there is a contraction on dissolving , and the amount gradually diminishes for each additional quantity entering into solution , so that the mean result is very different from what occurs when the solution is dilute or nearly saturated .
It is this contraction or expansion when a small additional quantity is dissolved in a nearly concentrated solution that must be taken into account in the following calculations .
In determining the influence of pressure on the solution of salts , I found it requisite to adopt somewhat different methods according to the peculiarities of the salts .
In some cases I sealed up in a saturated solution portions of the salt in clean , solid crystals , and determined the effect due to pressure from their loss in weight ; whereas in other cases I sealed up solutions containilg more salt than could be dissolved at the temperature at which the experirients were made , and determined the effect of pressure from the difference in the weight of the crystals deposited ; being of course careful to make allowance for any difference in the amount of solution in the tube with pressure and in that without , and to avoid any error that might be produced by a different temperature .
In all cases I have had a tube with pressure and another without , treated from first to last in precisely the same manner , and kept at exactly the same temperature , so that pressure was the only difference ; and usually the effect was so well marked that there was no doubt about the result .
In the case of chloride of sodium , solution goes on so slowly , and the .
mechanical equivalent of the force of crystallization is so great , that if pressure had been applied for only a few hours one might have concluded , with Bunsen , that pressure has no influence on solubility ; but , by maintaining it for a week or more , there was no difficulty whatever in perceiving that a solution which was quite saturated without pressure , dissolved more under a pressure of about 100 atmospheres .
The solubility of a salt in water appears to me to result from a kind of affinity which decreases in force as the amount of salt in solution increases .
This affinity is opposed by the crystalline polarity of the salt ; and when the two forces are equal , the solution is exactly saturated .
As is well known , a change in temperature alters this equilibrium ; and , according to my experiments , mechanical pressure relatively increases one or other of these opposing forces , according to the mechanical relations of the salt in dissolving .
At all events in the case of chloride of sodium the extra quantity dissolved under pressure varies directly with it for such pressures as glass tubes will resist , in the same manner as , according to Thomson 's experiments , the fusing-point of ice is reduced .
Thus I found that for a pressure of 491 atmospheres the extra solubility was 176 per cent. , and for 121 atmospheres '431 , which are almost exactly in the same ratio .
Hence , if S be the amount soluble without pressure , under a pressure of p atmospheres the solubility at the same temperature would be S +ps , where the values of S and s are independent , and vary for different temperatures and different salts .
Future experiments may perhaps show that this conclusion should be modified ; but yet it will be well to adopt it provisionally , in order to compare together the mechanical relations of different salts which otherwise would not be so intelligible .
According to Michel and Krafft* and to Schifft , sal-ammoniac is the only salt known for certain to occupy more space in solution than when crystallized .
Hence under pressure mechanical force must be overcome in dissolving , and experiment shows that , on this account , the relative force of crystalline polarity is increased and the solubility decreased .
This is the reverse of what results from an elevation of the temperature , so that the effect cannot be due to heat generated by the pressure , but must be the direct consequent of pressure .
Calculating from an experiment where the pressure was 164 atmospheres , which gave a decreased solubility of 1'045 per cent. of the whole salt in solution , a pressure of 100 atmospheres would cause '637 per cent. less to be dissolved than is soluble at 20 ?
C. without pressure , and the pressure requisite to reduce the solubility to the extent of 1 per cent. would be 157 atmospheres .
Expressing this fact in other words , we may say that a pressure of 157 atmospheres is the mechanical force with which the salt tends to dissolve in a solution containing 1 per cent. less than can dissolve at the same temperature without pressure , because the two forces exactly counterbalance one another .
In a still more dilute solution the force would of course be still greater , in accordance with the fact of a greater pressure being necessary to prevent the salt from being dissolved .
Supposing then that we had a solution a trifle more dilute than that just named , and in such indefinitely large quantity that a cubic inch of the salt could dissolve in it and yet produce no sensible change in its strength , so that from first to last it might be considered to dissolve under a pressure of 157 atmospheres , and also supposing that it was rigidly enclosed on all sides but one , so that the whole expansion must take place in one direction over an area of one square inch , since on dissolving there is an increase in bulk from 100 to 115'78 , the solution of this cubic inch would , as it were , raise 2355 lbs. through the space of 1578 inch .
This is mechanically the same as 371k lbs. raised 1 foot , or , the specific gravity of the salt being 1*53 , the same as 171 times the weight of the salt itself raised 1 metre .
Since it involves no arbitrary unit but the metre , I shall adopt the last expression as the measure of the total amount of mechanical work done by the solution of salts which expand in dissolving , and which may conversely be looked upon as the measure of the mechanical force rendered latent and , as it were , expended in the act of crystallization when crystals are deposited .
The value of this mechanical equivalent of course varies with the strength of the solution , as already remarked .
In the case of salts which occupy less space when dissolved than when solid , pressure , like the increased temperature , causes them to be more soluble ; mechanical force is lost when they dissolve , and is , as it were , expended in giving rise to solution .
When water thus containing more of a salt than could otherwise be dissolved at the same temperature is just saturated under any given pressure , the amount of pressure represents the force of crystalline polarity tending to cause the salt to be deposited in a crystalline form , but which is exactly counterbalanced by that pressure .
I will not give the details for each salt , but subjoin a Table of the results at which I have arrived for such as illustrate particular points of interest , the calculations being all made 1863 .
] 543 in accordance with the principles already described .
I also give them in the case of water , calculated from Thomson 's experiments , assuming that , when ice melts and mixes with water , it may be looked upon as dissolving in it ; and , as will be seen , the mechanical force thus deduced is of the same general order of magnitude as that generated by the crystallization of salts .
I. II .
IV .
V. 1 .
Chloride of Sodium ... .
1357 97 '407 -419 157 2 .
Sulphate of Copper ... .
4-83 60 1 910 3-183 7 3 .
Ferridcyanide of Potassium ... ... ... ... . .
2-51 86 -288.335 42 4 .
Sulphate of Potash ... .
3121 63 1 840 2-914 42 5 .
Ferrocyanide of Potassium ... ... ... ... . .
8'90 66 1-640 2-485 20 6 .
Water ... ... ... ... . .
893 ... .
991 106 Nos. 2 and 5 are calculated as hydrated crystals .
Column I. gives the expansion of each salt in crystallizing from a nearly saturated solution in water , the volume in a crystalline state being taken at 100 .
Column II .
gives the actual pressure in atmospheres in the experiment .
Column I11 .
gives the increased solubility due to the pressure given in column II .
, the total amount of salt dissolved without pressure being taken at 100 .
Column IV .
gives the increase in solubility that would be produced by a pressure of 100 atmospheres , as calculated in accordance with the principles already described , the same unit being taken as in column III .
Column V. gives the value of the mechanical work that could be done , or , so to speak , the amount of mechanical force set free when the various substances crystallized from a solution containing 1 per cent. more than would be dissolved without pressure , as measured by the number of times its own weight which any unit of the various salts could raise to the height of 1 metre in the act of crystallization .
Conversely , it is the amount of mechanical force which becomes latent in the act of solution ; and in the case of a still more supersaturated solution it would be greater , and vice versed , in accordance with the fact of the increased solubility varying with the pressure .
544 On comparing together the various salts , it will be seen that their properties vary very considerably .
Thus , under the same pressure , the extra quantity of sulphate of copper dissolved in nearly ten times that of ferridcyanide of potassium .
The mechanical equivalents also vary even more , being ( for chloride of sodium ) about 22times as great as for sulphate of copper .
On the contrary , the mechanical equivalents of ferridcyanide of potassium and sulphate of potash are the same ; but , under equal pressures , the extra quantity of the latter dissolved in nearly nine times as great , owing to the difference in the amount of expansion in crystallizing .
This latter is , however , nearly the same for water and ferrocyanide of potassium , whilst , under the same pressure , the extra quantity of that salt dissolved is 21times that of ice , in consequence of the much greater mechanical equivalent of the ice .
It appears to me that we may provisionally conclude that the increased solubility due to pressure varies directly with the change of volume , and inversely with the mechanical equivalent of the force of crystalline polarity , so that , if S be the total amount of salt which dissolves without pressure , c be some function of the change in volume in dissolving , and m some function of the mechanical equivalent of the force of crystalline polarity , the solubility , at the same temperature , under a pressure of p atmospheres would be S+ o-c .
If the salt be one that expands on dissolvin ing , c of course is negative , and therefore under pressure the solubility becomes S-_p-'c ; that is to say , it is diminished , as proved by experiments with sal.ammoniac .
If no change in volume took place , we may , I think , also conclude that pressure would not in any way increase or decrease the solubility of a salt .
Moreover , since , when a solution is just saturated , the force with which the salt tends to crystallize is equal to that with which it tends to dissolve , their mechanical equivalents must be equal and opposite .
Hence we may perhaps conclude that , other circumstances being the same , the mechanical equivalent of a salt like chloride of sodium , which so readily attracts moisture , would be greater than that of one like sulphate of copper , which so readily loses even its water of crystallization ; and thus also the relative influence of equal amounts of 1863 .
] 545 pressure would be very different , as is confirmed by experiment in the case of these and some other salts .
The facts I have described , therefore , show that there is a direct correlation between mechanical force and the forces of crystallization and solution .
According to some chemists , the latter is an instance of real combination ; but , whatever views be entertained respecting its nature , we cannot , I think , deny that the force represents some modification of chemical affinity , or is at all events most closely allied to it .
In comparison with some kinds of affinity , it may indeed be , and probably is , weak ; but yet , as I have shown , it sometimes has a very considerable mechanical equivalent , even when nearly counterbalanced by an opposite force ; and since such pressures as glass tubes will resist have no very great influence on what we may perhaps consider a weak affinity , we cannot expect that any pressure at our command would have much influence on strong affinities .
I have , however , succeeded in obtaining some results which apparently show that pressure influences undoubtedly chemical changes taking place slowly , and therefore probably due to weak , or nearly counterbalanced , affinities .
The method adopted in this part of the inquiry was to seal up some solid substance in a solution which gives rise to a slow double decomposition , taking great care to have in the tube with pressure , and in that without , pieces cut so as to be of the same size and form , and a solution of the same character , so that , with the exception of pressure , all the conditions were the same .
Possibly I may be so fortunate as to discover some case where the affinity is so weak that pressure may determine whether it go forward or not , of which fact the structure of metamorphic rocks furnishes examples ; but hitherto I have only been able to prove that pressure modifies the rate at which chemical action takes place .
This branch of the inquiry is , however , beset with many difficulties , for the change in volume produced by double decomposition is small , and its determination involves several complicated questions .
The volume of the solids is easily determined ; but that of the salts in solution is not the same when other salts are present as when they are dissolved in pure water , and varies much according to the strength of the solution and the nature of the salts ; and many points are still so obscure , that I shall only give two cases by way of example .
546 When a portion of Witherite is enclosed in a tube with a strong solution of protochloride of iron , there is a slow decomposition into chloride of barium , which is dissolved , and carbonate of iron , which remains firmly attached to the Witherite , and would ultimately give rise to an excellent pseudomorph .
The best conclusion at which I have been able to arrive is , that there is in this change an increase in volume equal to about 10'7 per cent. of the Witherite altered , so that , under pressure , mechanical force must be overcome .
In an experiment where everything went on in a very satisfactory manner , the pressure was maintained for three months at from 80 to 100 atmospheres , and for one month was under 80 atmospheres , so that , on an average , it was about 80 atmospheres ; and I found that the amount of chemical change was 21*7 per cent. less than when , all other circumstances having been the same , there had been no pressure ; thus clearly showing that pressure had , as it were , diminished the force of chemical affinity .
If then one cubic inch had been altered under this pressure , it would have overcome a mechanical force equal to that required to raise 1200 lbs. through the space of *107 inch , which is equivalent to raising twenty-one times its own weight to the height of 1 metre ; and under the same circumstances 1'278 cubic inch would have been altered when no such mechanical force had to be overcome .
Supposing then that in both cases the total energy at work was the same , but in one was altogether expended in producing a chemical result , and in the other in producing partly a chemical and partly a mechanical effect , we may say that the force which gives rise to the purely chemical change , taking place at a particular rate , is equal to that which gives rise to this chemical effect , taking place at *783 of that rate , and to a mechanical effect equal to the force required to raise in the same space of time 34'87 times the weight of the Witherite altered to the height of 1 metre .
Supposing also that the power of chemical force varies as the rate at which it gives rise to a chemical change , in the same manner as the power of a mechanical force varies as the velocity of motion imparted by it , we may perhaps conclude that this mechanical force is equal to -217 of the chemical force , and that the whole energy of the chemical action under the conditions of the experiment was equal to the mechanical power required to raise in the same period of time 160 times the weight of the Witherite altered to 1863 .
] 547 the height of 1 metre .
If these principles are correct , a pressure of more than 370 atmospheres would have entirely counterbalanced the force of chemical affinity , since to produce any chemical change it would then have had to overcome a greater force than it possessed .
This is so great a pressure that I fear it will be difficult to prove the deduction by experiment ; and until some such case can be found , capable of being verified , these calculations must be considered as little more than suggestions , which future investigations may confirm or disprove .
When calcite is sealed up in a mixed and rather strong solution of chloride of sodium and sulphate of copper , slow double decomposition gives rise to malachite , sulphate of lime , and carbonic acid ; and though this case is extremely complicated , and it is very difficult to determine what would be the change in volume , yet , so far as I am able to make out , until the solution becomes saturated with sulphate of lime , there is a decrease in volume equal to about 8 per cent. of that of the calcite altered , so that , under pressure , mechanical force is the very reverse of being opposed to the chemical change .
Three experiments , all indicating the same fact , and in which , on an average , the pressure was about 90 atmospheres for two weeks , show that , as a mean of the whole , the amount of chemical change was 17 per cent. more with the pressure than without ; thus proving that pressure had , as it were , increased the force of chemical affinity .
Calculating according to the principles described above , we may conclude that a pressure of 530 atmospheres would have caused the action to take place at double the rate , and that therefore the chemical action is equivalent to the expenditure of that amount of mechanical force , being thus generated by it .
Arguing then in a manner similar to that already described , but modified to suit the different conditions , if there be a contraction equal to 8 per cent. of the bulk of the calcite , there must be a loss of mechanical force capable of raising 28 times the weight of the calcite altered to the height of 1 metre , in the time required for the chemical change ; which amount of mechanical energy , as it were , becomes latent , and is transformed into chemical action , and would again exhibit itself as a mechanical force if , by any means , the chemical affinities could be inverted and everything restored to its original state .
In a like manner , other experiments indicate that in some cases 548 pressure causes a slower , and in others a quicker chemical action , whilst in others it has scarcely any influence whatever ; and though , for reasons already explained , I say it with some hesitation , yet , bearing in mind what is already known respecting the action of pressure on hydrate of chlorine , hydrated hydrosulphuric acid , and other substances described by the various authors referred to in the notes , I think the facts I have described make it very probable that further research will show that pressure weakens or strengthens chemical affinity according as it acts against or in favour of the change in volume ; as if chemical action were directly convertible into mechanical force , or mechanical force into chemical action , in definite equivalents , according to well-defined general laws , without its being necessary that they should be connected by means of heat or electricity .
On the present occasion I shall not attempt to consider the various geological and mineralogical facts which appear to me to admit of the application of the principles I have described , for many of them are peculiarities in structure of which neither myself nor any one else has ever given a description , and would therefore demand a preliminary notice .
However , I may say that it appears to me that a number of facts connected with metamorphic rocks and the phenomena of slaty cleavage , which , to me at all events , have hitherto been inexplicable , are readily explained if mechanical force be directly correlated to chemical action , and if in some cases the direction in which crystals are formed be more or less related to pressure , in some such way as there is a connexion between their structure and magnetic force , as shown by the experiments of Plucker , Faraday , Tyndall , and many other observers .
We may also , I think , explain the origin of the impressions on the limestone pebbles in the " Nagelflue " in Switzerland , about which so much has been written in Germany and France , without a satisfactory reason having been discovered ; and the same explanation accounts for the mutual penetration of the fragments of which some limestones are formed , apd for the banded structure of some which possess slaty cleavage .
The curious teeth-like projections with which one bed of limestone sometimes enters into another , also to a certain extent indicate a chemical action depending on mechanical force ; and probably the same may be said of some of the peculiarities of slickensides and mineral veins .
It is also possible that a pressure of several hundred atmospheres may facilitate some of the chemical changes involved in the transformation of water and carbonic acid into the organic compounds met with in animals and plants of low organization found at great depths in the ocean , and thus to a certain extent compensate for diminished light .
I , however , most willingly admit that very much remains to be learnt before we can say to what extent the principles I have described are applicable ; and yet , at the same time , cannot but think that henceforth they must be taken into account in many departments of chemical and physical geology , and will readily explain a number of facts which otherwise would be very obscure .
|
112307 | 3701662 | On the Physiological Properties of Nitrobenzole and Aniline | 550 | 559 | 1,862 | 12 | Proceedings of the Royal Society of London | Henry Letheby | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0118 | null | proceedings | 1,860 | 1,850 | 1,800 | 10 | 137 | 4,188 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112307 | 10.1098/rspl.1862.0118 | http://www.jstor.org/stable/112307 | null | null | Biology 2 | 37.297596 | Chemistry 2 | 25.187511 | Biology | [
-76.62803649902344,
-18.98539924621582
] | I. " On the Physiological Properties of Nitrobenzole and Aniline .
" By HENRY LETHEBY , M.B. , F.L.S. , &c. , Professor of Chemistry , and late Professor of Toxicology in the Medical College of the London Hospital .
Communicated by Dr. SHARPEY , Sec. R.S. Received April 23 , 1863 .
It is on record that Thrasyas , the father of Botany , was so skilled in the preparation of drugs , that he knew how to compound a poison which would remain for days in the living body without manifesting its action , and would at last kill by a lingering illness .
Theophrastus speaks of this poison , and says its force could be so modified as to occasion death in two , three , or six months , or even at the end of a year or two years .
The writings of Plutarch , Tacitus , Quintilian , and Livy are full of instances of what seem to be this kind of slow and occult poisoning .
In fact , until recently there has been a common belief among the unlearned that a skilful poisoner could so apportion the dose and combinations of certain subtle agents that he could destroy the life of his victim with certainty , and at the same time measure his allotted moments with the nicest precision , and defy the utmost skill of the physician and the chemist .
Even so late as the 16th century this belief was shared by the learned of the medical profession ; for we are told , in Sprat 's ' History of the Royal Society , ' that among other questions which were drawn up by the earlier Fellows to be submitted to the Chinese and Indians was , " ' Whether the Indians can so prepare that stupefying herb , Datura , that they make it lie several days , months , years , according as they will have it , in a man 's body without doing him any hurt , and at the end kill him without missing half an hour 's time ?
" Modern toxicologists have long since discarded these notions , and have set them down to the vague fears and exaggerated fancies of the ancients , rather than to the sober contemplation of facts .
But the account which I am about to give of the physiological properties of nitrobenzole will show that there is one substance , at least , which realizes to a great extent the extraordinary opinions of the ancients .
This compound may be given today , and yet , if the dose be not too large , it shall not manifest its action until tomorrow , or the day after , and shall then destroy life by a lingering illness , which shall not only defy the skill of the physician , but shall also baffle the researches of the medical jurist .
These facts are so remarkable , that they would be hardly credited if they were not susceptible of the proof of demonstration .
They are likewise the more interesting and important from the circumstance that nitrobenzole is now a common article of commerce , and is accessible to everyone .
In every manufactory where nitrobenzole and aniline are prepared on a large scale , the peculiar narcotic effects of these poisons are often observed .
The vapours escaping into the atmosphere are breathed by the workmen , and cause distressing headache and a heavy , sleepy sensation .
For the most part these effects are not serious , but are quickly relieved by fresh air and a mild stimulant , as a glass of brandy and water .
Now and then , however , the workmen , from carelessness in their habits , expose themselves to the action of comparatively large quantities of these poisons , and then the effects are most dangerous .
Two fatal cases of poisoning by nitrobenzole have been referred to me by the coroner for investigation during the last two years , and in both instances they were the results of careless manipulation .
In one case a man , forty-three years of age , spilt a quantity of the liquid over the front of his clothes , and he went about for several hours in an atmosphere saturated with the poison .
In the other a boy , aged seventeen years , received a little of the liquid into his mouth while sucking at a siphon .
The effects were nearly the same in both cases , notwithstanding that in one the poison was inhaled , and in the other it was swallowed .
For some time there was no feeling of discomfort beyond that of drowsiness ; gradually , however , the face became flushed , the expression stupid , and the gait unsteady the sufferers had the appearance of persons who had been drinking .
Little by little this stupor increased , until it passed into profound coma , and in this condition they died .
The progress of each case was much the same as that of slow intoxication , excepting that the mind was perfectly clear until the coming on of the fatal coma .
This was sudden , like a fit of apoplexy ; and from that moment there was no return of consciousness or of bodily powerthe sufferer lay as if in a deep sleep , and died without a struggle .
The duration of each case was nearly the same ; about four hours elapsed frcm the time of taking or inhaling the poison to the setting in of the coma , and the coma lasted for about five hours .
After death there were no appearances of convulsion , but rather of narcotism and apoplexy .
The face was flushed ; the lips were livid ; the superficial vessels of the body , especially about the throat and arms , were gorged with blood ; the dependent parts were turgid ; the blood was everywhere black and fluid ; the lungs were somewhat congested ; the cavities of the heart were full ; the liver was of a purple colour , and the gall-bladder distended with bile ; the brain and its membranes were turgid , and in the case of the man there was much bloody serosity in the ventricles .
Analysis discovered the existence of nitrobenzole in the brain and stomach , and also of aniline .
These effects were so remarkable , that I determined to examine them still further by experiments on domestic animals .
Dogs and cats were submitted to the action of from thirty to sixty drops of nitrobenzole which had been well washed with dilute sulphuric acid and water to free it from every trace of aniline .
The poison was generally administered by pouring it into the mouths of the animals , but sometimes it was given by means of an oesophagus-tube .
When the nitrobenzole had come into contact with the mouth , it always caused discomfort , as if from unpleasant taste , and there was profuse salivation .
Its local action on the stomach , however , was never very great , for there was rarely any vomiting until the setting in of nervou symptoms , and this seemed to be due to sympathy rather than to any local irritation of the stomach .
Two classes of effects were clearly observed : there was either the rapid coma which characterized the operation of the poison on the human subject , or there was a slow setting in of paralysis and coma , after a long period of inaction .
'When the effects were speedily fatal , the animal was soon seized with giddiness and an inability to walk .
The weakness of the limbs first appeared in the hind extremities , and was manifested by a difficulty in standing ; but very soon it extended to the fore legs , and then to the head and neck .
There was complete loss of voluntary power .
The animal lay upon its side , with its head drawn a little back , and with its limbs in constant motion , as if in the act of walking or running .
The muscles of the back were occasionally fixed in spasm , and every now and then the animal would have a sort of epileptic fit .
It would look distressed , would howl as if in pain , and would struggle violently .
After this it would seem exhausted , and would lie powerless .
The pupils were widely dilated , the action of the heart was tumultuous and irregular , and the breathing was somewhat difficult .
For some time , however , the animal retained its consciousness , for it would look up , and wag its tail when spoken to ; but suddenly , and often at the close of a fit , it would become comatose the eye would remain open , but the conjunctiva would be insensible to touch , and the movements of the limbs would nearly cease ; the breathing would be slow and somewhat stertorous , and the animal would appear as if s it were in a deep sleep .
This condition would last until it diedthe time of death varying from twenty-five minutes to twelve hours after the administration of the poison .
When the action of the poison was slower , there was often no visible effect for hours or days .
At first there was always a little discomfort from the taste of the poison , but this soon subsided , and then for a day or more the animal appeared to be in perfect health .
It would go about as usual , would be quite lively in its movements , would eat its food heartily , and in fact would seem to be in no way affected by the poison .
Suddenly , however , it would look distressed , it would have an attack of vomiting , and it would tumble over in an epileptic fit .
When this had subsided , it was generally found that the animal was weak , or even quite paralysed in its hind extremities ; and after two or three of such attacks , the loss of voluntary power would extend to the fore limbs .
The animal would lie upon its side perfectly helpless ; and then the progress of the case was much the same as that already described , except that it was considerably slower .
Consciousness , for example , would be retained for days after the animal was paralysed , and , although it was quite unable to stand , it would take food and drink when they were put into its mouth .
The condition in which it lay was most distressing : the look was anxious and full of fear ; the limbs were in constant motion ; and every now and then there would be a violent struggle , as if the animal was in a fit , or was making fruitless efforts to rise .
This would last for days , and then there would be either a gradual restoration of voluntary power with complete recovery , or death from exhaustion .
The time that elapsed from the administration of the poison to the coming on of the first symptoms , namely the epileptic fit , varied from nineteen hours to seventy-two-in most cases it was about two days ; and the time of death was from four to nine days .
The post-mortem appearances were nearly the same in all cases , whether the death was quick or slow .
The vessels of the brain and its membranes were extremely turgid ; the cavities of the heart were full of blood ; the lungs were but slightly congested ; the liver was of a deep purple tint , and the gall-bladder distended with bile ; the stomach was natural , without sign of local irritation ; and the blood all over the body was black and uncoagulated .
Whenever the progress of the case had been quick , and death had taken place within twenty-four hours , the odour of the nitrobenzole was clearly perceptible in the stomach , the brain , and the lungs ; and there was always unmistakeable evidence of the existence of aniline in the organs of the body .
In the slower cases the odour of the poison had often entirely disappeared ; but generally there were distinct traces of aniline in the brain and urine , and sometimes in the stomach and liver ; occasionally , however , no poison was found .
It has appeared to .
me that the facts which are here elucidated are very remarkable ; for they not only indicate a rare circumstance in toxicology , namely , that a poison may be retained in the system for many days without showing its effects , but also that the poison may be changed into an entirely different substance .
The importance of these facts cannot be overrated ; they are alike interesting to the chemist , the physiologist , and the medical jurist ; for , without dwelling on a very possible occurrence-namely , the criminal administration of this poison , with the knowledge that the effects would be delayed , that the symptoms would correspond to those of natural disease , that the progress of the case would be lingering , and that there would be either no discovery of poison in the body , or the discovery of a thing different from that administered-it will be manifest that the study of these facts by the medical jurist is of public importance .
To the physiologist they are also interesting , insomuch as they indicate a reducing power in the animal body by the conversion of nitrobenzole into aniline .
I have endeavoured to ascertain whether this is due to a living or a dead process .
In the first place , I find that dead and decomposing organic matter will effect the change alluded to ; for when nitrobenzole is placed in the dead stomach , or is kept in contact with putrid flesh for several hours , there is a partial reduction of it into aniline .
This may be the source of the poison found in the dead body ; but , on the other hand , there is a great similarity in the physiological effects of nitrobenzole and those of aniline .
When aniline is given to dogs and cats in doses of from twenty to sixty drops , it causes rapid loss of voluntary power .
The animal staggers in its gait , looks perplexed , and falls upon its side powerless .
Its head is drawn back , the pupils are widely dilated , there are slight twitchings or pasms of the muscles , the breathing is difficult , the action of the heart is tumultuous , and the animal quickly passes into a state of coma .
From this it never recovers , but remains upon its side as if in a deep sleep , and so dies in from half an hour to thirty-two hours .
The post-mortem appearances are much the same as the last : the brain and its membranes are turgid , the cavities of the heart are nearly full of blood , the lungs are but slightly congested , and the blood all over the body is black and uncoagulated .
In every case the poison was easily discovered in the brain , the stomach , and the liver .
While however , there seems to be a probable conversion of nitrobenzole into aniline in the living animal body by a process of reduction , there is also undoubtedly a change of an opposite character going on upon the surface of the body , whereby the salts of aniline are oxidized and converted into mauve or magenta purple .
Some remarkable facts illustrative of this have been brought under my own notice , and have been the subject of clinical observation .
In the month of June 1861 , a boy aged 16 was brought into the London Hospital in a semi-comatose condition .
He had been scrubbing out the inside of an aniline vat , and while so doing he breathed an atmosphere charged with the vapour of the alkali , and became insensible .
He did not suffer pain or discomfort , but was suddenly seized with giddiness and insensibility .
When he was brought to the hospital he looked like a person in the last stage of intoxication : the face and surface of the body were cold , the pulse was slow and almost imperceptible , the action of the heart was feeble , and the breathing was heavy and laborious .
After rallying a little , he complained of pain in his head and giddiness .
It was then noticed that the face had a purple hue , and that the lips and lining membrane of the mouth and the nails had the same purple tint .
The next day , although the narcotic effects of the poison had passed away , he was still remarkably blue , like a patient in the last stage of cholera .
In the early part of last year , sulphate of aniline was given in rather large doses to patients in the London Hospital affected with chorea .
The doses ranged from a quarter of a grain to seven grains .
They were frequently administered , so that large quantities of the salt were taken in a very short time .
In one case as much as 406 grains were given in the course of a few days .
No very remarkable effects followed beyond this-that after a few doses had been taken , and the system had become , as it were , saturated with the salt , the face became of a leaden blue colour , the lips and gums looked as if the patients had been eating black currants , and the nails also acquired a purple hue .
The colour faded a little before the time came for the administration of another dose , but soon after taking it it appeared again ; and this was the subject of constant observation .
Dr. Fraser and Dr. Davies have recorded the results of their experience in five cases * , from which it would seem that , although the free alkali is a powerful poison , the sulphate of it has but little action upon the animal body .
The general conclusions which appear to me to be warranted by these investigations are:1st .
That nitrobenzole and aniline in its free state are powerful narcotic poisons .
2nd .
That they exert but little action , as local irritants , on the stomach and bowels .
3rd .
That although the effects may be quick , and the fatal termination of them rapid , yet nitrobenzole may remain in the system for a long time without manifesting its action .
4th , That the salts of aniline are not nearly so poisonous as the free alkali .
5th .
That in rapid cases of fatal poisoning , both the poisons are readily discovered in the dead body .
6th .
That in slow cases the poisons may be entirely changed or eliminated , and therefore not recognizable .
7th .
That both of the poisons appear to be changed in the body by processes of oxidation and reduction , nitrobenzole being changed into aniline , and aniline and its salts into mauve cr magenta .
In an appendix t are given notes of the two cases of fatal poisoning by nitrobenzole referred to in the paper , and a detailed account of twelve experiments on animals with nitrobenzole , and three with aniline ; also the process employed for the recognition of aniline and nitrobenzole in the dead body , as follows:1st .
The matters to be analysed were bruised in a mortar with a little water , and very slightly acidulated with.dilute sulphuric acid , 2nd .
They were then submitted to distillation in a glass retort the distilled products being saved in three or four separate portions by changing the receiver at different stages of the process .
In this way the presence of nitrobenzole was discovered .
3rd .
The residue in the retort , when reduced to a pulpy mass by the distillation , was treated with strong spirit of wine and filtered .
4th .
The filtered alcoholic solution which contained the aniline was treated with a slight excess of subacetate of lead , and again filtered .
In this way gum , dextrine , &c. were removed .
5th .
The filtered solution was treated with a slight excess of a saturated solution of sulphate of soda in water .
In this manner the excess of lead was precipitated as a sulphate .
6th .
The clear solution was then made very alkaline with caustic potash , and distilled to dryness from an oil-bath .
The aniline , together with ammonia from the animal matters , was found in the clear , colourless , distilled spirit .
7th .
This was neutralized , or rather made acid , with a slight excess of dilute sulphuric acid , and evaporated nearly to dryness in a white porcelain dish .
If necessary , the spirit was saved by distillation .
8th .
The residue was of a pinkish colour if aniline was present , and occasionally there were little streaks of blue around the edges of the white porcelain dish .
If the quantity of the saline residue was not more than a grain or so , it was at once tested by dissolving it in a few drops , or even in a single drop , of dilute sulphuric acid ( 1 to 1 ) .
A small portion of it was then placed upon a strip of bright platinum ; and the platinum having been conneeted with the positive pole of a single cell of a Grove 's battery , the liquid was touched with the negative pole : in a few secon ds , if aniline was present , the liquid would acquire a bronze , a blue , or a pink colour ; the kind of colour being dependent on the am ount of aniline present-bronze being the result of much aniline , and pink of a very little .
In this way at least the -iooth part of a grain of aniline was easily recognized .
To another portion of the acid liquid placed upon a white porcelain plate , a little peroxide of lead or red prussiate of potash was added , and a blue or purple reaction followed .
This test is not so delicate as the last , for it fails when the amount of aniline is less than the T-:ith of a grain .
Other tests may be resorted to if necessary , as when the quantity 558 of aniline is large .
Thus peroxide of manganese or bichromate of potash may be used in the same way as the red prussiate of potash in the last experiment ; but these tests will not answer with less than the -^)th of a grain of aniline .
Lastly , a drop of a solution of chloride of lime may be added to the acid liquid , and if the quantity of aniline exceeds the To-oth part of a grain it will cause a purple reaction .
9th .
If the quantity of saline residue from the last operation is large , and there is reason to believe that much ammonia is present , this alkali must be got rid of , for it greatly interferes with the success of the colour-experiments .
The residue , therefore , is made moist with water , and rubbed down with about twice its bulk of neutral carbonate of soda .
It is then exposed to the air for a short time until the odour of ammonia has passed away .
It is then treated with strong alcohol , filtered , acidulated with dilute sulphuric acid , and again evaporated .
The aniline is now fit for the colour-experiments .
There are no fallacies to these experiments ; for although , as I have elsewhere shown , strychnia will give nearly the same colourreactions , yet in the first place this alkali is not volatile like aniline , and will not therefore distil over as the latter does ; and in the next place , while the best effects , in respect of colour , are developed with dilute acid and aniline , strychnia requires the concentrated acid .
These differences are sufficient to prevent any embarrassment as regards the two alkaloids .
|
112308 | 3701662 | On the Immunity Enjoyed by the Stomach from Being Digested by Its Own Secretion during Life. [Abstract] | 559 | 561 | 1,862 | 12 | Proceedings of the Royal Society of London | Frederick W. Pavy | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 25 | 787 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112308 | null | http://www.jstor.org/stable/112308 | null | null | Biology 2 | 50.456415 | Physiology | 37.999965 | Biology | [
-51.13958740234375,
4.363325119018555
] | II .
" On the Immunity enjoyed by the Stomach from being digested by its own Secretion during Life .
" By FREDERICK W. PAVY , M.D. Communicated by Dr. SHARPEY , Sec. R.S. Received April 29 , 1863 .
( Abstract .
) The author stated that the opposition which his view on the above subject received the evening of its announcement , in his former communication read January 8 , 1863 , had induced him to perform a series of additional experiments .
As from these experiments some important confirmatory evidence was supplied , he deemed it desirable to present a further communication to the Society on the subject .
He had again denuded the stomach of a patch of mucous mem1863 .
] 559 bran , and in one experiment had allowed the animal to live for ten days .
It had fed in an ordinary manner every day , and when killed , reparation was found in an advanced stage towards completion , the walls opposite the denuded part having been considerably thickened by new matter that had been thrown out .
Upon much further extended observation the author found that the standard he had taken from the rabbit , as regarded the postmortem action of the contents of the stomach upon the organ itself , was not just in its application to the dog .
Actual experiment on the dog had shown that upon the animal being killed at a period of full digestion , and its temperature being afterwards maintained about the degree belonging to life , the effect at the end of five and six hours only amounted to more or less digestion of the mucous membrane .
In the rabbit , under similar circumstances , the effect had gone on to perforation , on account , apparently , of the stronger acidity of the gastric contents .
In reality , then , the effect of arresting the circulation through the stomach during life , about coincided in both rabbit and dog with what occurred , other circumstances being equal , after death .
As a counterpart to the experiments originally mentioned , where dilute non-corrosive acids had been introduced into the stomach of the dog , and the flow of blood through the organ afterwards arrested , an operation that was followed by comparatively rapid perforation , the author had used the same acids , in the same quantities , and similarly diluted , but the circulation was allowed to remain free , and now the stomach resisted digestive attack .
Ligatures had of course been applied to secure the retention of the acid liquid introduced .
A mode of experimenting suggested by Dr. Sharpey had been undertaken .
After an incision through the anterior wall of the stomach , a portion of the posterior wall had been drawn forward , and a ligature placed tightly around it , so as thus to arrest the circulation through a limited portion of the organ 's parietes .
It was found that this constricted mass underwent digestion like a morsel of food .
An experiment had been performed bearing on the explanation that had been given to account for the attack upon the living frog 's legs and rabbit 's ear by digestion whilst the stomach remained protected .
Three drachms of muriatic acid , diluted to three ounces with water , were introduced into the stomach of a dog , and the end of the oesophagus and the pylorus ligatured , without including the vessels , so that the circulation through the organ was left free .
In one hour and forty minutes death took place , and on the parts being examined immediately , perforation , with extensive digestion of the interior of the stomach throughout , was found .
The author considered that the question of result was clearly shown to resolve itself into one dependent on degree of power possessed by the acid contents of the stomach on the one hand , as against the alkaline circulation on the other .
With a certain amount of acid only in the stomach , the circulation can afford the required protection ; whilst with a larger amount the influence of the acid prevails , and digestive solution of the organ is the result .
Allow , now , the contents of the stomach to remain the same , and vary the degree of vascularity in the parts submitted to the digestive influence .
We have simply here a converse arrangement of the circumstances ; and the position is represented by the situation of the stomach as compared with that of the frog 's legs and rabbit 's ear .
|
112309 | 3701662 | On a Question of Compound Arrangement | 561 | 563 | 1,862 | 12 | Proceedings of the Royal Society of London | J. J. Sylvester | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0120 | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 26 | 789 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112309 | 10.1098/rspl.1862.0120 | http://www.jstor.org/stable/112309 | null | null | Formulae | 50.1403 | Tables | 24.186587 | Mathematics | [
76.6303939819336,
-27.385684967041016
] | III .
" On a Question of Compound Arrangement .
" By J. J. SYLVESTER , M.A. , F.R.S. , Professor of Mathematics in the Royal Military Academy , Woolwich .
Received April 27 , 1863 .
My successful but as yet unpublished researches into the Theory of Double Determinants have involved the consideration of the following curious case of arrangements .
There are given m+ n1 counters of n distinct colours just capable of being packed into mn urns .
The question refers to the distribution of the counters among the urns , subject to the condition that it shall not be possible to form a closed circuit of double colours between any number of the urns chosen arbitrarily , ex. gr. we must allow no distribution of counters in which one urn contains blue and yellow , a second yellow and red , a third red and green , and a fourth green and blue , because here blue , yellow , red , and green would form a closed circuit .
This condition , it is evident , excludes the same combination of colours from existing in any two of the urns , and also the repetition of any one colour in the same urn .
Any distribution of counters obeying this condition may be called an excyclic distribution .
I annex two propositions , one qualitative , the other quantitative , referring to such distributions .
Qualitative Theorem .
In any excyclic distribution between m urns of m +n-1 counters of n different colours , any set of counters selected at will must befewer in number than the number of distinct colours which they contain added to the number of urnsfrom which they are drawn .
Before going on to enunciate the second proposition I must premise one or two simple definitions .
The capacity of an urn means the number of counters it will contain , the frequency of a colour the number of counters of that colour , so that the sum of all the capacities and the sum of all the frequencies must be each equal to the number of the counters .
Again , by the diminished capacity of any urn or diminished frequency of any colour , I mean such capacity or frequency respectively diminished by unity .
Finally , by thepolynomial function of any set of numbers a , b , ... I , I mean the coefficient of xa .
yb ... z. in the expansion of ( x+y+ ... )a+b+ ... +l .
I can now enunciate the following Quantitative Theorem .
The number of modes of excyclic distribution between m urns of m+n1 counters of n different colours is equal to the product of the polynomial function of the diminished frequencies of all the several colours multiplied by the polynomial function of the diminished capacities of all the several urns .
Observation .
A double determinant means the resultant of a system of ( m +n 1 ) homogeneous equations each containing mn terms , and linear in respect to each of two systems of m and n variables taken separately , but of the second order in respect to the variables of these two systems taken rn(m + n--i ) collectively .
Any such resultant is of the degree -r(m1 ) ( --1 ) 7r(m1.)7r(n-1\ in respect of the given coefficients , and may be represented by an ordinary determinant of the ( m + n-)th order , every one of whose terms corresponds to a particular system of capacities of the in urns and of repetitions of the n colours in the question above treated .
The total number of such systems or terms will be 7r(m+n-2 ) )2 7r(m1)7r(nl ) ' Every term in this determinant will itself be a sum of simple determinants of the ( mnl)th order , corresponding ( each to each ) with the totality of the excylcic distributions of ( mn+n--1 ) counters in respect of the particular systems of m capacities and n frequencies appertaining to that term ; so that the number of simple determinants whose sum constitutes a term in the grand total determinant is always the product of two polynomial coefficients .
In the particular case , where one of the systems contains only two variables , one of these polynomial coefficients becomes unity , and the other sinks down to a binomial coefficient .
The only instance of a double determinant which is believed to have been considered up to the present moment is that given by Mr. Cayley in the 'Cambridge and Dublin Mathematical Journal , ' vol. ix .
1854 , for the case of m= 2 , n= 2 .
|
112310 | 3701662 | On a Theorem Relating to Polar Umbrae | 563 | 565 | 1,862 | 12 | Proceedings of the Royal Society of London | J. J. Sylvester | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0121 | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 19 | 716 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112310 | 10.1098/rspl.1862.0121 | http://www.jstor.org/stable/112310 | null | null | Formulae | 83.60185 | Neurology | 7.487492 | Mathematics | [
74.31988525390625,
-32.40166473388672
] | IV .
" On a Theorem relating to Polar Umbrae .
" By J. J. SYLVESTER , M.A. , F.R.S. Received April 27 , 1863 .
By polar umbree I mean such as obey in the strictest manner the polar law of sign , so that not only any two appositions or products of such umbrae derivable from one another by an interchange of two of their elements are to be considered each as the negative of the other , but also any such apposition or product becomes zero if the same element is found in it more than once .
Thus Sir W. Hamilton 's i , j , k are not polar umbrae , because although ijk= -jik kij , &c. , ii , j , kk , instead of being nulls , are in the Calculus of Quaternions taken as unities* .
Let us now define any set arranged either in line or column of such umbral quantities to be multiplied by a corresponding set of actual quantities when each term of the one set is multiplied by the corresponding one of the other , and the sum taken of the products so obtained as in the ordinary case of the multiplication of the lines or columns of two determinants inter se .
Thus , ex. yr .
( a , b , cix , y , z ) , as also ( bsI/ is to mean the same product , viz. ax+ by +cz .
Again , imagine a rectangular ( square or oblong ) matrix of polar umbre , and that each line thereof is multiplied by the same line of actual quantities , the product of the products so obtained I call a Factorial of the Matrix .
I also call the product similarly obtained when the columns of the matrix are substituted for the lines , a Factorial of the same , but distinguish between the two by giving to one the name of a Transverse , the second of a Longitudinal Factorial of the matrix .
We are now in a position to enunciate the following remarkable theorem : The product of any longitudinal by any transverse factorial of the same polar umbral matrix is identically zero .
Ex. yr .
Let of be a matrix of polar umbrae , but x , y , z and also 4 , n actual quantities .
Then ( ax + b , cz ) ( dx + ey +fz ) is a transverse factorial , ( a +d/ ) ( b +en ) ( c +fT ) a longitudinal factorial of the above matrix , and by the theorem their product should be zero .
This is easily verified .
The two factorials expanded are respectively adx2 + bey2 + cfz + ( ae+ bd)xy + ( bf+ ce)yz+ ( af+ dc)zx , abcS3 + ( abf+ aec + dbc ) , ri + ( dec+ dbf+ aef)W2 + defr3 ; in their product the coefficient of x2T3 ==aboad=O , zxy3 =abcae + abebd= O , t242 " = abfad+ aecad+ dbcad= 0 , wyT2 = abfae + abfbd+ aecae + aecbd+ dbcae + dbcdb = aecbddbeae= aeebdaecbd= 0 , and so for all the other terms .
This is the fundamental theorem by aid of which I obtain the resultant of a lineo-linear system of equations in its most perfect form .
It is easy to obtain two different solutions , each of them unsymmetrical in respect of the data of the question ; the conversion and fusion of each of these into one and the same determinant , symmetrical in all its relations to the data , is effected instantaneously by a process derived from the above theorem .
In that particular application of it , the umbre involved each represent columns of actual quantities in number equal to the number of places in the width and length of the umbral matrix to which they belong , so that each coefficient in the product of a lateral by a longitudinal factorial represents an ordinary determinant made up of these columns , from which it is evident that the polar law of sign and nullity necessary for the truth of the theorem are satisfied in the case supposed .
|
112311 | 3701662 | Notes, Principally on Thermo-Electric Currents of the Ritterian Species. [Abstract] | 565 | 566 | 1,862 | 12 | Proceedings of the Royal Society of London | C. K. Akin | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 2 | 25 | 533 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112311 | null | http://www.jstor.org/stable/112311 | null | null | Electricity | 43.447547 | Fluid Dynamics | 23.37741 | Electricity | [
-6.7678399085998535,
-71.79753112792969
] | V. " Notes , principally on Thermo-electric Currents of the Ritterian Species .
" By C. K. AKIN , Esq. Communicated by Professor STOKES , Sec. R.S. Received March 26 , 1863 .
( Abstract .
) The electromotive force of a thermo-electric couple is a function of the nature of the metals of which it is composed , and of the temperatures of the junctions .
It is expressed in this paper by [ Ex y]T where x and y are names of metals , and T and t are temperatures .
In this notation Becquerel 's two laws become a , b]t , =[a , 6-[a , b ] ; ... .
( I. ) and ( a , c)T= [ a , ]T+ [ , c]T ... ... ( II .
) From ( I. ) we learn that the electromotive force of a couple may be expressed as the difference of two quantities which are functions of the temperature and of the nature of the circuit , or [ , Y]O=[ , y]T--[l Y ] ... . .
( II .
) From ( II .
) we learn that any number of metals with their ends at the same temperature may be introduced without effect , or [ a , b]t+[b , c]t=[a , C]t ... . .
( IV .
) This equation will always be true if [ L Y ] t= [ t[y ] ... ... .
( V. ) whence we may write ( III .
) [ Iy t[X ?
]t[y]t[T + [ y3 T ; or , in other words , the electromotive force of a couple may be considered as the difference of the electromotive force of two metals , each of which is found by subtracting its tension at the higher temperature from that of the lower one .
Everything therefore depends on a knowledge of the value of what may be called the electric tension of each metal at the various temperatures .
This for every metal is a function of temperature , and may be called , in the language of the paper , a function of the nature ( or name ) of the metal and the temperature .
( The nature of the metal may be altered otherwise than chemically .
) If the temperature of the metal vary in any way throughout its length , then if it be homogeneous , the electromotive force will depend only on the temperatures of its extremities .
In a circuit of one metal , the author considers that at the junction of the ends there may be a real discontinuity of temperature while there is a continuity of electric current .
He regards the explanation of the effect by the stratum of air between the unequally heated ends to be unsatisfactory .
Mercury , as is known , will not produce thermo-curyents in this way .
The author considers that the texture , &c. , as well as the chemical nature of the substance , influences the value of the thermo-electric function .
He also shows the possibility of the thermo-electric inversions first discovered by Professor Cumming .
|
112312 | 3701662 | On the Nature of the Sun's Magnetic Action upon the Earth. [Abstract] | 567 | 567 | 1,862 | 12 | Proceedings of the Royal Society of London | Charles Chambers | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 1 | 9 | 337 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112312 | null | http://www.jstor.org/stable/112312 | null | 108,808 | Meteorology | 41.105569 | Fluid Dynamics | 29.396636 | Meteorology | [
56.70547866821289,
-9.360730171203613
] | I. " On the Nature of the Sun 's Magnetic Action upon the Earth .
" By CHARLES CHAMBERS , Esq. Communicated by the President .
Received April 30 , 1863 .
( Abstract .
) If the sun were a magnet of sufficient power to exert a sensible attraction upon a small magnet at the distance of the earth , it would have a real influence on the earth by inducing magnetism in its soft iron , and an apparent one due to the direct action of the sun upon the magnets used for measuring the earth 's variations of force .
As the earth rotates upon its axis , producing a varying relation , as to position , of the place of observation with respect to the sun , a diurnal variation will thus be produced in the forces which act upon the magnetometers , which variation is shown to follow the simple law x= A sin ( h + a ) , x being the deviation of the magnet from its normal position , h the hour-angle of the sun ( and for a single day ) , Aa constant coefficient , and aa constant angle .
A comparison of this result with the laws of the observed diurnal variations shows that direct and inducing action of the sun is not the sole cause of the variations .
An endeavour is then made to prove that if any part of the observed diurnal variations is due to this cause , it is small in comparison with that produced by other forces in operation .
This is done by separating from the observed variations the part of them which obeys the law x'=B sin ( h+ / ) , and comparing the variations in the values of B and p from month to month with those of A and a , when it is seen that the former obey a law which has but little similarity to the law of variation of the latter .
|
112313 | 3701662 | Numerical Elements of Indian Meteorology.--Series I. [Abstract] | 567 | 568 | 1,862 | 12 | Proceedings of the Royal Society of London | Hermann de Schlagintweit | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 2 | 35 | 468 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112313 | null | http://www.jstor.org/stable/112313 | null | null | Meteorology | 48.033867 | Biography | 22.817748 | Meteorology | [
34.40459442138672,
17.401979446411133
] | II .
" Numerical Elements of Indian Meteorology."-Series I. By Dr. HERMANN DE SCHLAGINTWEIT , Corr. Memb. of the Academies of Sciences of Munich , Madrid , Lisbon , &c. Communicated by the President .
Received May 4 , 1863 .
( Abstract .
) In this paper the author communicates Plates il which the iso2s thermal lines are represented between the latitudes of 5 ?
N. and 36 ?
W. , and longitudes of 78 ?
E. and 98 ?
E. of Greenwich .
1st , of the mean temperature of the year ; 2nd , of the cool season , viz. December , January , and February ; 3rd , of the hot season , viz. March , April , and May ; 4th , of the rainy season , viz. June , July , and August ; 5th , of the autumn , viz. September , October , and November .
The memoir which accompanies the Plates contains a statement of the data on which the isothermal lines are founded .
These are : 1 .
Meteorological researches made by the author and his brothers at various stations in India and the Indian Archipelago during the years 1854-1858 .
2 .
The original manuscripts in thirty-nine folio volumes of meteorological observations made by various observers under the authority of the Indian Government at 207 stations in British India .
In regard to the observations referred to under this head , the author considers that he possesses a special qualification for using them advantageously by having himself visited most of the stations , examined the instruments , and acquainted himself with the circumstances of their employment .
The 207 stations are divided into ten geographical groups , as follows1 .
Eastern India : 1 , Assam ; 2 , Kharsia Hills ... ... ... .
12 2 .
Bengal and Bahar , and Delta of the Ganges and Brahmaputra ... ... ... ... ... ... ... ... ... ... ... ... . .
36 3 .
Hindostan , the upper Gangetic plain ... ... ... ... ... .
27 4 .
Panjab , including the stations west of the Indus ... ... 24 5 .
Western India : Rajvara , Guzrat , Kach , Sindh ... ... . .
10 6 .
Central India : Berar , Orissa , MAlva , Bandelkhand ... .
15 7 .
1 , Southern India : hilly districts , Dekhan and Maissur ; 2 , Nilgiris ... ... ... ... ... ... ... ... ... .
29 8 .
Southern India , coasts : Konhan , Malabar , Karnatik. .
24 9 .
Ceylon 10 .
Indo-Chinese Peninsula , Archipelago , and China ... .
20 Each group has its appropriate processes of reduction , which are severally discussed .
|
112314 | 3701662 | On the Structure of the So-Called Apolar, Unipolar, and Bipolar Nerve-Cells of the Frog. [Abstract] | 569 | 574 | 1,862 | 12 | Proceedings of the Royal Society of London | Lionel Beale | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 6 | 90 | 2,285 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112314 | null | http://www.jstor.org/stable/112314 | null | null | Biology 3 | 62.850907 | Neurology | 28.456642 | Biology | [
-76.24242401123047,
11.308545112609863
] | III .
" On the Structure of the so-called Apolar , Unipolar , and Bipolar Nerve-cells of the Frog .
" By LIONEL BEALE , M.B. , F.R.S. , F.R.C.P. , Professor of Physiology and of General and Morbid Anatomy in King 's College , London , and Physician to King 's College Hospital .
Received May 7 , 1863 .
( Abstract .
) The author adverts to the opinion generally received with regard to the existence of apolar , unipolar , bipolar , and multipolar nervecells , and observes that if cells having such very different relations to the nerve-fibres they are supposed to influence , as apolar , unipolar , and multipolar cells , 4o actually exist , as many different kinds of action must be admitted .
For it is hardly likely that a nerve-cell unconnected with any fibre can affect the fibres at a distance from it in the same way as a cell acts upon fibres which are in structural continuity with it .
Neither is it probable that a cell with but one fibre proceeding from it can constitute an organ which acts upon the same principle as the cell from which two or more fibres proceed .
If no fibre , or but one fibre proceeds from certain cells , the formation of complete:nervous circuits , at least in these instances , is impossible ; and if it be admitted that circuits do not exist in every case , a strong argument is advanced against the existence of such complete circuits as a necessary or fundamental condition of a complete nervous apparatus .
But if it can be shown , on the other hand , as the author maintains is the case , that all the supposed apolar and unipolar cells have at least two fibres proceeding from them , the fact must be accepted in favour of the view that such complete circuits may exist , while the fact that the fibres connected with many cells have been seen to proceed in opposite directions some distance after leaving the cell , is a very strong argument in favour of such general inference , and at the same time an explanation of many arrangements which are observed constantly in connexion with nerve-fibres in various tissues .
Many observers have described apolar and unipolar cells in ganglia in different parts of the frog .
The author , on the other hand , has failed to discover any apolar or unipolar cells in this or in any other animal , and considers that the apparent absence of fibres , and the presence of one fibre only in connexion with a cell , result from the defective modes of preparation generally employed .
He maintains that every nerve-cell , central or peripheral , has at least two fibres proceeding from it* .
In many cases he has demonstrated that these fibres pursue opposite directions , and he considers that such an arrangement is general , and therefore necessary .
The author considers himself justified in drawing the following conclusions from observations he has made during the last three years .
1st .
That in all cases nerve-fibres are in bodily connexion with the cell or cells which influence them , and this from the earliest period of their formation .
2nd .
That there are no apolar cells , and no unipolar cells , in any part of any nervous system .
3rd .
That every nerve-cell , central or peripheral , has at least two fibres in connexion with it .
Though the present inquiry is limited to the structure of the particular cells connected with the ganglia in different parts of the frog , the author has studied the 'arrangement of nerve-cells and nervefirbes in nervous centres , as well as at their peripheral distribution , in many different animals .
1 .
General description of the ganglion-cells connected with the sympathetic and other nerves of the frog .
The general form of these cells is oval or spherical ; but the most perfectly formed ganglion-cell is more or less pearor balloon-shaped in its general outline , and by its narrow extremity is continuous with nerve-fibres which may be followed into trunks .
The figure represents a well-formed ganglion-cell from a ganglion close to one of the large lumbar nerves of the little green tree-frog ( Hyla arborea ) .
The substance of the cell consists of a more or less granular material , which by the slow action of acetic acid becomes decomposed , oil-globules being gradually set free .
Near the fundus or rounded end is seen the very large circular nucleus with its nucleolus .
In some of these cells , at about the central part or a little higher , are a number of oval nuclei , some of which are in connexion with fibres .
The matter of which the mass of the cell consists gradually diminishes in diameter , and contracts so as to form a fibre , in which a nucleus is often seen .
At the circumference of the cell , about its middle , the material seems gradually to assume the form of fibres , which contain numerous nuclei , and these pass around So-called " unipolar " nerve-cell , with , 1st , a straight , and 2nd , a spiral fibre emanating from it .
The fibres continuous with these are seen to pursue opposite directions .
Magnified 700 linear .
L LL ... .
l 1000th of an inch X 700 .
1000 ' the first fibre in a spiral manner .
Thus in the fully formed cell a fibre comes from the centre of the cell ( straightfibre ) , and one or more fibres ( spiral fibres ) proceed from its surface .
These points are represented in the figure* .
2 .
On the formation of ganglion-cells in the fully formed frog .
This subject is arranged under the three following heads , but as it would not be intelligible without figures , it will not be given in abstract .
The development of these cells and many other structures may be studied in the fully formed animal as well as in the embryo .
a. Ganglion-cells developed from a nucleated granular mass like that which forms the early condition of all tissues .
b. Ganglion-cells formed by the division or splitting up of a mass like a single ganglion-cell .
c. Ganglion-cells formed by changes occurring in what appears to be the nucleus of a nerve-fibre .
3 .
Further changes in the ganglion-cell after its formation .
Under this head the movement of the cell from the point where its growth commenced is described .
It is shown that the two fibres , which at first seem to come from opposite extremities of the cell , lie parallel to each other .
They increase in length , and subsequently one is seen to be twisted round the other , as shown in the figure .
Sometimes the fibres below the point where the spiral arrangement exists run parallel for a long distance , but at length pursue opposite directions .
The author considers that the formation of the ganglioncell commenced at the point where the fibres diverge , and that subsequently the cell moved away , the parallel fibres , which at length become straight and spiral , being gradually formed or drawn out as it were from the cell .
4 .
Of the spiralfibre of the fully formed ganglion-cell .
The spiral fibre or fibres can be shown to be continuous with the material of which the body of the cell is composed , as well as the straight fibre , but the former are connected with its surface , while the latter proceeds from the deeper and more central part of its substance .
There are many nuclei in connexion with the spiral fibre , and several nuclei of the same character imbedded in the substance of the mass of which the cell is composed .
These latter nuclei seem to be connected with an earlier condition of the matter which becomes , when more condensed , spiral fibre .
A great difference is observed with regard to the extent of the spiral fibre in cells of different ages .
In the youngest cells the fibres near the cell are both parallel to each other , but as the cell grows one is seen to be coiled round the other ; and the number of coils increases as the cell advances in age , while the matter of which the fundus of the cell is composed gradually becomes less-apparently in consequence of undergoing conversion into fibres .
Nuclei are found in the course of the straight fibre , as well as in connexion with the spiral fibre .
Nuclei have been demonstrated in connexion with the dark-bordered fibres near their origin and near their distribution in all tissues .
Next follows a discussion " on the essential nature of the changes occurring during the formation of all nerve-cells , and on the formation of spiral fibres , " but this is not adapted for an abstract .
The term " nucleus " is only employed in a general sense .
The author believes that the " nucleus , " nucleolus , " and centres within the latter ( " nucleoluli " ) merely represent centres of different ages .
He considers that the matter of the nucleus becomes gradually transformed into the formed matter around it , and generally , that these bodies are merely centres which arise in pre-existing centres .
He maintains that from the outer formed matter connected with the fibres new nerve-cells could not be produced , while he holds that from the nuclei , nucleoli , and contained centres , entirely new and complete cells could be evolved .
So he considers that the difference in the properties and powers of the formed matter on the one hand , and the nuclei and nucleoli on the other , depends upon these two kinds of matter having arrived at different stages of existence .
That which is formed cannot form new formed matter , nor appropriate nutrient material ; but the living germinal matter of the nucleus can be resolved into formed matter , and it can appropriate inanimate pabulum , and confer upon it the same wonderful ( vital ) powers which it possesses itself , and which were communicated to it from preexisting germinal matter .
7 .
Of the fibres in the nerve-trunks continuous with the straight and spiral fibres of the ganglion-cells .
The conclusions upon this important question are as follows:1st .
That in some instances very fine fibres , not more than the J-6- , th of an English inch in diameter , are alone continuous with both straight and spiral fibres of the ganglion-cell .
2nd .
That a dark-bordered fibre may be traced to the ganglioncell as the straightfibre , while the spiral fibres are continued on as very fine fibres .
3rd .
That the spiral fibres may be continued onwards as a darkbordered fibre which may even be wider , at least for some distance , than the fibre continued from the straight fibre .
4th .
That both straight and spiral fibres may be continuous with dark-bordered fibres .
It is therefore quite certain that the spiral fibre is not connective tissue , although the author considers it probable that many German observers may adopt this view until they have an opportunity of seeing the fibres themselves .
8 .
Of the ganglion-cells of the heart .
The author 's conclusions are quite opposed to those of Kolliker , who states that all the cells are unipolar , and that the fibre always passes in a peripheral direction , also that the transcurrent fibres of the vagus have no connexion with these cells .
The author , on the contrary , affirms that the cells have at least two fibres comingfrom them , that some of the fibres pass towards the heart , and others towards the brain .
He regards it as very probable that many at least of these ganglion-cells are connected with fibres of the vagus .
Kolliker has also stated ( 1860 ) that many apolar cells could be seen in the heart , ganglia , and in the bladder .
The author has been able to demonstrate fibres in connexion with so many cells which appeared devoid of fibres , that he considers himself justified in denying the existence of apolar and unipolar cells altogether .
Next follow some observations on " the ganglion-cells and nerves of arteries ; " " on the connexion of the ganglion-cells with each other ; " and the paper concludes with a description of the so-called " capsule " of the ganglion-cell , and a discussion on the nature and formation of the connective tissue and its corpuscles in the immediate neighbourhood of nerve-fibres .
The paper is illustrated with forty-seven drawings of the specimens , magnified from 700 to 1700 linear ; and the author states that many of the specimens will probably retain the appearances he has copied for several months .
All the preparations have been made in the same manner .
An outline of the process has been already given in the author 's previous communications , but the author is aware that it may be some time before the correctness of his conclusions is generally admitted , in consequence of the difficulty of preparing demonstrative specimens .
|
112315 | 3701662 | On the Belts of Jupiter, in a Note Addressed to the Secretary | 575 | 575 | 1,862 | 12 | Proceedings of the Royal Society of London | John Phillips | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0126 | null | proceedings | 1,860 | 1,850 | 1,800 | 1 | 16 | 391 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112315 | 10.1098/rspl.1862.0126 | http://www.jstor.org/stable/112315 | null | null | Optics | 44.622858 | Astronomy | 26.213762 | Optics | [
74.97938537597656,
20.631542205810547
] | IV .
" On the Belts of Jupiter , " in a Note addressed to the Secretary .
By JOHN PHILLIPS , M.A. , LL. D. , Professor of Geology , Oxford .
Received May 5 , 1863 .
Oxford , 4th May , 1863 .
DEAR SIR , -The favourable position of Jupiter for scrutiny of his physical features may perhaps have already brought to the Royal Society some notice of the aspect of his belts .
Whether that be so or not , I think you will readily excuse the desire I feel to lay before the Society a sketch from my equatorial , which shows the colours of several celestial objects more distinctly than I am accustomed to hear is the case with some other instruments of the achromatic class .
The sketch shows the usual equatorial bands* , or rather bands nearly in the usual latitudes north and south of the equator .
These , to the eyes of my friends and to mine , appear not dark grey , or greyish brown , or brown , but nearly of the colour of some ochraceous sands , or the yellower parts of what is called " red " deal .
Several friends to whom I have shown the planet have immediately exclaimed , " how red the bands are ; " " never saw them so red before .
" The bands far from the equator are not reddened , but of a grey tint a little warmed .
The space between the equatorial bands , sometimes described as yellow , appears rather bright white and silverymuch the brightest part of the surface .
The outer borders of the equatorial bands are not parallel , the inner borders much unequal ; in one part the two bands are connected across .
Not the faintest trace of such a tint as that conspicuous in these bands appears on any part of the moon ; but it is pretty nearly the tint of the supposed " land " of Mars .
In fact , it was suggested to my mind that these coloured extra-equatorial belts were land , seen between white clouds , of which the brightest band was on the equator .
JOHN PHILLIPS , M.A. , LL. D. , F.R.S. , Professor of Geology , Oxford .
|
112316 | 3701662 | Notes of Researches on the Polyammonias, No. XXIII.--Hydrazobenzol, a New Compound Isomeric with Benzidine | 576 | 578 | 1,862 | 12 | Proceedings of the Royal Society of London | A. W. Hofmann | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0127 | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 37 | 1,030 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112316 | 10.1098/rspl.1862.0127 | http://www.jstor.org/stable/112316 | null | null | Chemistry 2 | 97.871779 | Geography | 1.039915 | Chemistry | [
-46.137481689453125,
-61.2940559387207
] | V. " Notes of Researches on the Polyammonias , No. XXIII .
Hydrazobenzol , a new Compound isomeric with Benzidine .
" By A. W. HOFMANN , LL. D. , F.R.S. , &c. Received May 7 , 1863 .
The discovery , among the secondary products of the manufacture of aniline , ofxenylamine , the probable connexion of which with benzidine ( xenylene-diamine ) I have already had an opportunity of pointing out* , has induced me to submit the latter compound to some experiments .
In preparing benzidine by the process originally pointed out by Zinint , viz. by treatment of azobenzol with sulphide of ammonium , I was led to the observation of some phenomena which appear to have escaped the attention of those who have hitherto studied this substance .
It is generally supposed that the action of reducing agents upon azobenzol produces directly benzidine .
C12 Hlo 2+ I2- , = C1 H12 N2 .
Y Azobenzol .
Benzidine .
Such , however , is not the case .
The well-defined base designated by the latter name is only a secondary product ; the first compound which is generated in this process being a neutral or feebly basic body , differing in all its properties from benzidine , with which , however , it is isomeric , and into which it may be converted by simple treatment with strong mineral acids .
On passing a current of sulphuretted hydrogen into a solution of azobenzol in alcoholic ammonia , the yellowish-red liquid is rapidly decolorized , and yields on addition of water a crystalline precipitate of a peculiar camphor-like smell .
This substance contains a minute quantity of the sulphur which separates , the bulk of which , however , remains dissolved as polysulphide of ammonium ; it is easily purified by two or three crystallizations from very dilute alcohol .
Submitted to combustion , the compound thus obtained yields numbers which coincide with those furnished by the analysis of benzidine .
The properties in which the new substance , for which I propose the name hydrazobenzol , differs from benzidine are the following : Hydrazobenzol crystallizes from alcohol , and more especially from benzol ( in which it is somewhat less soluble ) , in well-developed white plates , benzidine being always deposited from these solvents in welldefined needles ; and whilst the latter is freely soluble in boiling water , from which it separates on cooling in the form of a crystalline mass of nacreous lustre , the former is so sparingly soluble in water that it is impossible to recrystallize it from that solvent .
The fusingpoint of hydrazobenzol is 131 ?
C. , that of benzidine being 1180 C. The basic properties of benzidine are well defined ; it dissolves even in the weakest acids , such as acetic acid , in which hydrazobenzol is nearly insoluble .
Stronger acids , such as hydrochloric and sulphuric acids , more especially on application of heat , dissolve hydrazobenzol ; but the solution thus obtained contains no longer the unchanged body ; the addition of alkali , fixed or volatile , produces a precipitate which now possesses all the properties of benzidine .
These characters are sufficient to individualize hydrazobenzol .
There is , however , another property which marks its difference from benzidine in even a more conspicuous manner .
Benzidine when submitted to a high temperature distils ; a certain portion is decomposed in this process , but the larger quantity is volatilized without decomposition .
On heating hydrazobenzol considerably above its fusingpoint , a powerful reaction ensues , the heat evolved being sufficient to carry over nearly the whole amount of substance in the form of a deep red oil , from which , on cooling , crystals of azobenzol are deposited .
On addition of an acid the oil yields a further quantity of this substance , and the acid solution is then found to contain abundance of aniline .
The reaction which occurs is simple enough .
2C12 12 N2 = C12 Hlo N2 + 2C6 H7 N. Hydrazobenzol .
Azobenzol .
Aniline .
I had hoped that among the products of the reaction paraniline ( C12 H1S 4N=2 C H7 N ) might be met with ; in this hope I have been disappointed .
The reproduction of azobenzol from hydrazobenzol may be accomplished in a variety of other ways .
Nitrous acid , chlorine , bromine , iodine , chromate and permanganate of potassium , and nitrate of silver produce this effect in a most easy manner ; in these processes the loosely adherent hydrogen is simply eliminated , no aniline being formed as a secondary product .
Even when moistened with alcohol and exposed to the action of the atmosphere , hydrazobenzol is gradually reconverted into azobenzol .
It deserves to be noticed that some of the chemists who have been engaged in the examination of benzidine must have occasionally worked with hydrazobenzol .
Mr. Noble* , who many years ago prepared benzidine in my laboratory , especially remarks that the substance obtained by him is reconverted into azobenzol by the action of nitrous acid .
I have satisfied myself that benzidine thus treated yields no trace of azobenzol .
From the experiments described , it is obvious that in the formation of benzidine from azobenzol two distinct phases have to be distinguished : in the first phase the molecule of azobenzol assimilates a molecule of hydrogen , but this hydrogen remains in a very feeble state of combination , being eliminated again by a great variety of agents .
It is only under the influence of acids that the hydrogen molecule becomes incorporated in the system , if I may use this expression , and fixed benzidine , a substance of great stability , is formed .
Whatever view may be taken regarding the nature of azobenzol , the constitution of which it must be admitted is utterly unknown , the intermediate substance has to be viewed as its hydrogen compound , and it is this consideration which induced me to propose the name hydrazobenzol .
|
112317 | 3701662 | Note on the Composition of Aniline-Blue | 578 | 579 | 1,862 | 12 | Proceedings of the Royal Society of London | A. W. Hofmann | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0128 | null | proceedings | 1,860 | 1,850 | 1,800 | 2 | 15 | 164 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112317 | 10.1098/rspl.1862.0128 | http://www.jstor.org/stable/112317 | null | null | Chemistry 2 | 65.176144 | Tables | 12.846516 | Chemistry | [
-47.46950912475586,
-57.94881820678711
] | VI .
" Note on the Composition of Aniline-Blue .
" By A. W. HOFMANN , LL. D. , F.R.S. , &c. Reeeived May 21 , 1863 .
The prosecution of my researches on the aniline colours has led me to a result of great simplicity , which I hasten to lay before the Royal Society .
Aniline-blue is triphenylic rosaniline .
Aniline-red , Rosaniline ... ... ..C20 CH 9 N3 , 12 0 .
Aniline-blue , Triphenylic Rosaniline. .
C20 116 N,3 H2 0 ( C6 H , )3The commercial article is a salt of the base , the hydrochlorate for example , the composition of which corresponds to the monatomic hydrochlorate of rosaniline .
* Chem. Soc. Quart .
Journ. vol. viii .
p. 292 .
Hydrochlorate of Rosaniline ... ... C2O H20 N3 C1 .
Hydrochlorate of Triphenylic Rosaniline .
20 H13 C 3 .
Details of these experiments I hope to lay before the Society at an early meeting .
|
112318 | 3701662 | On the Calculus of Symbols.--Third Memoir. [Abstract] | 579 | 579 | 1,862 | 12 | Proceedings of the Royal Society of London | W. H. L. Russell | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 1 | 13 | 267 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112318 | null | http://www.jstor.org/stable/112318 | null | null | Formulae | 93.220088 | Biography | 2.911765 | Mathematics | [
81.46772003173828,
-34.29035186767578
] | VII .
" On the Calculus of Symbols."-Third Memoir .
By W. H. L. RUSSELL , Esq. , A.B. Communicated by A. CAYLEY , F.R.S. Received May 15 , 1863 .
( Abstract .
) In my second Memoir " On the Calculus of Symbols , " I worked out the general case of multiplication according to one of the two systems of combination of non-commutative symbols previously given .
In the present paper I propose to investigate the general case of multiplication according to the other system .
I commence with the Binomial Theorem , to which the second system gives rise .
In my previous researches I obtained the general term of the binomial theorem when the symbols combine according to the first system by equating symbolical coefficients ; here , on the other hand , I consider the nature of the combinations which arise from the symbolical multiplication , and obtain the general term by summation .
I next proceed to the multiplication of binomial factors .
Here the general term is obtained by considering the alteration of weight undergone by certain symbols in the process of multiplication .
The multinomial theorem according to the second system is next considered and its general term calculated .
I conclude the memoir with some applications of the calculus of symbols to successive differentiation .
This paper completes the investigation of symbolical multiplication and division according to the two systems of combination , the general case of division having been worked out by Mr. Spottiswoode in a very beautiful memoir recently published in the Philosophical Transactions .
|
112319 | 3701662 | Anniversary Meeting | 580 | 580 | 1,862 | 12 | Proceedings of the Royal Society of London | null | fla | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 1 | 10 | 282 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112319 | null | http://www.jstor.org/stable/112319 | null | null | Biography | 97.073421 | Physiology | 2.108022 | Biography | [
55.406028747558594,
68.84172058105469
] | 580 [ June 11 , June 4 , 1863 .
The Annual Meeting for the Election of Fellows was held this day .
Major-General SABINE , President , in the Chair .
The Statutes relating to the Election of Fellows having been read , Mr. John Bishop and Mr. John Iogg were , with the consent of the Society , nominated Scrutators to assist the Secretaries in examining the lists .
The votes of the Fellows present having been collected , the following gentlemen were declared duly elected into the Society-Edward William Cooke , Esq. , A.R.A. William Crookes , Esq. James Fergusson , Esq. Frederick Field , Esq. Rev. Robert Harley .
John Russell Hind , Esq. Charles Watkins Merrifield , Esq. Professor Daniel Oliver .
Frederick William Pavy , M.D. William Pengelly , Esq. Henry Enfield Roscoe , B.A. Rev. George Salmon , D.D. Samuel James Augustus Salter , M.B. Rev. Arthur Penrhyn Stanley , D.D. Colonel Frederick M. Eardley Wilmot , R.A. June 11 , 1863 .
Dr. W. B. CARPENTER , Vice-President , in the Chair .
Charles Watkins Merrifield , Esq. ; Professor Daniel Oliver ; Frederick W. Pavy , M.D. ; Samuel James Augustus Salter , M.B. ; and Col. Frederick M. Eardley Wilmot , R.A. , were admitted into the Society .
The CROONIAN LECTURE was delivered by Professor JOSEPH LISTER , F.R.S. , " On the Coagulation of the Blood , " as follows : The subject on which I have the honour to address you this evening , is one which lies at the foundation both of Physiology and Pathology , and , on account of its great importance , has engaged the
|
112320 | 3701662 | The Croonian Lecture: On the Coagulation of the Blood | 580 | 611 | 1,862 | 12 | Proceedings of the Royal Society of London | Joseph Lister | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0130 | null | proceedings | 1,860 | 1,850 | 1,800 | 32 | 314 | 13,722 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112320 | 10.1098/rspl.1862.0130 | http://www.jstor.org/stable/112320 | null | null | Biology 2 | 29.723552 | Physiology | 24.438509 | Biology | [
-62.4174690246582,
12.051061630249023
] | " On the Coagulation of the Blood , " as follows : The subject on which I have the honour to address you this evening , is one which lies at the foundation both of Physiology and Pathology , and , on account of its great importance , has engaged the best energies of many very able men , among whom may be mentioned , for example , such distinguished Fellows of this Society as John Hunter and lewson ; so that it might well seem presumptuous in me to hope to communicate anything new regarding it , were it jot that the constant progress of Physiology and the allied sciences is ever opening up fresh paths for inquiry , and ever affording fresh facilities for pursuing them .
Indeed , my difficulty , on the present occasion , does not depend so much on the lack of materials as on the complicated relationis of the subject , which make me almost despair of being able , in the short time that can be devoted to a lecture , to give , in anything like an intelligible form , even an adequate selection of the facts at my disposal .
It may , in the first place , be worth while , more especially for the sake of any present who may not be physiologists , to mention very briefly some well-known general facts respecting the constitution of the blood .
The blood , if examined by the microscope within the vessels of a living animal , is seen to consist of a liquid and numerous small particles suspended in it .
The liquid is termed the " liquor sanguinis , " the particles the " blood-corpuscles .
" Of these corpuscles a few are colourless , and are named the " coloulrless " or " white corpuscles .
" The great majority are coloured and cause the red appearance of the blood , and hence are called the " red corpuscles .
" Soon after blood has been shed from the body , it passes from the fluid into the solid form .
This depends upon the development in the blood of a solid material termed " fibrin , " so called from its fibrous nature , consisting , as examined by the naked eye , of tenacious fibres , arid having the same character also under the microscope .
These fibres form a complicated network among the blood-corpuscles , and from their tenacity are the cause of the firmness of the clot .
Soon after the process of solidification or coagulation is complete , the fibrin exhibits a disposition to shrink , and squeezes out from among the corpuscles entangled in its meshes a strawcoloured fluid termed the serum , very rich in albumen , in fact very similar in chemical composition to the fibrin , which , in its turn , may be said to be idelntical chemically with the material of muscular fibre .
The question before uls , therefore , is , What is the cause of the development of this solid material , the fibrin ?
The subject may be looked at in two aspects , -first , as to the essential nature of the process of coagulation ; and secondly , as to the cause of its occurrence when the blood is removed from the body .
With regard to the first point , the essential niature of the process of coagulation , different views have been entertained .
John Hunter was of opinion that the coagulation of the blood , the solidification of the fibrin , was an act of life-analogous , in some respects , to the contractioni of muscular fibre .
This , on the other hand , was made very unlikely by the observation of his contemporary , Mr. lewson , that blood may be kept in the fluid state by the addition of various neutral salts , but retains the faculty of coagulating when water is added to the mixture .
Mr. Gulliver , on one occasion , kept blood fluid , by means of nitre , for upwards of a year , but found that it still coagulated on the addition of water .
It seems exceedingly improbable that any part of the human body should retain its vital properties after being thus pickled for more than a year .
But here I would wish to make an explanation of the use of this term " vital properties .
" When employing it , I do not wish to commit myself to any particular theory of the nature of life , or even to the belief that the actionls of living bodies are not all conducted in obedienice to physical and chemical laws .
But it appears that every component tissue of the human body has its own life , its own health , just as we ourselves have ; and as the actions of living men will ever retain their interest whatever views be entertained of the nature of life , so must the actions of the living tissues ever continue to be essential objects of study to the physiologist and pathologist .
When , therefore , I use the term " vital properties , " I mean simply properties peculiar to the tissues as components of the healthy living body .
Turning now to the other aspect of the subject of coagulation the cause of the occurrence of that process on the escape of the blood from the living body we find that here again various theories have been held , which may be divided into mechianical , chemical , and vital .
The mechanical theory was , that mere rest of the blood was sufficient to cause coagulation .
I say this was the theory ; but I believe it will be found to be still taught by many , that the cause of the coagulation of the blood in an artery which has been tied is its stagnation in the vicinity of the ligature .
As to the chemical theories they have been various .
Onie very natural view was , that exposure to the air was the essential cause of coagulation .
Mr. Hewson believed that this was , at all events , an importaint element in the causes of the phenomenon ; and many eminelt physiologists and pathologists have held the same view , except that , instead of the air as a whole , the oxygen of the air has been supposed to be the important element .
Sir Charles Scudamore considered that coagulation was greatly promoted by the escape of carbonic acid ; and more recently the evolution of ammonia has beeni regarded as the essential cause of the change .
According to the ammonia theory , due to Dr. Richardson of this city , the fluidity of the blood within the body depends on a certain amount of free ammonia holding the fibrin in solution , and the coagulation of the blood when withdrawn from the vessels is the result of the escape of the volatile alkali .
Then , as to vital theories .
These have been held by many physiologists , amo-ng whom may be mentioned Sir Astley Cooper and Mr. Thackrah , who , from experiments which they performed , were led to the inference that the living vessels exert an active influence upon the blood , by which coagualation is prevented ; and Mr. Thackrah wenit so far as to attribute this action of the vessels to nervous influence .
The view that the blood is kept fluid by the operation of its natural receptacles has been advocated more recently by Briicke of Vienna , whose essay will be found iu the 'British and Foreign Medical Review ' for 1857 .
Br'icke performed his experiments on turtles and frogs , in which animals the blood remains fluid in the heart for days after death ; and I feel bound to say that some of the facts which he has brought forward seem to me quite sufficient to show that the ammonia theory , whatever amounit of truth it may contain , cannot be the whole truth , and cannot explain the flutidity of the blood within the body .
For example , Brileke found that , having shed blood from the heart of a living turtle into a basin , and transferred , with a syringe , a portion of that blood into the empty heart of another turtle just killed , the blood thus transferred into the empty heart remained fluid for hours ; whereas that which was left in the basin coagulated in a few minutes .
Hle also found that blood continued fluid in the heart of a turltle long afteir the injection of air into the heart through a veini till the cavities of the organ contained a foamny mixture of blood and air .
Yet it by no means follows that the vital theory and the ammonia theory are necessarily altogether inconsistent .
It might be true for anything we could tell , a priori , that the coagulation of the blood , when shed from the body , might depend on the evolution of a certain amount of ammonia , previously holding the fibrin in solution , and yet it might , at the same time , be true that the cause of the ammonia remaining in the blood in the healthy vessels might be an action of the living vessels retaining it there .
It might be that an action of the living vessels might chain down the ammonia and prevent it from escaping , whereas , when shed from the body , it would be free to escape .
This notion was , I confess , at one time entertained by myself ; and one of my earliest experiments was performed with a view to the corroboration of the ammonia theory as applied to blood outside the body .
It seemed to me desirable that further evidence should be afforded of the effect of mere occlusion from air in maintaining the blood fluid .
If the ammonia theory were true , then if blood could be shed directly from a living vessel into an air-tight receptacle composed of ordinary matter it ought to remain fluid .
For this purpose , I made the following experiment:-I tied into the jugular vein , V , ( fig. 1 ) of Fig. 1 .
v a sheep a long vulcanized india-rubber tube , T , adapted by means of short pieces of glass tule at its extremities , both ends being connected with the vessel so that the current of blood might be permitted to flow through the tube , and then continue its natural course .
When it had been ascertained that the blood was circulating freely through the tube , which could be readily done by placing the finger on the cardiac aspect of the vein , which was then made to swell if the circulation was proceeding through the tube , pieces of string well-waxed were tied at intervals of about 2 inches round the tube , which was thus converted into a number of air-tight receptacles containing blood , which certainly had no opportunity for the escape of ammonia .
The tube was then removed , and I found , in accordance with the view which I was then disposed to entertain , that the blood , instead of coagulating completely in a few minutes as it would have done if shed into a cup , remained partially fluid in these receptacles after the lapse of three hours .
But I have since found that if the experiment be repeated in the same way as regards its earlier stages , and if , after a few of the strings have been tied on , the tube be cut across , the blood which is in the part of the tube in the vicinity of the air , just like that which is in the air-tight receptacles , remains fluid in part for two or three hours .
In short , that my precautions in ensuring that these receptacles should be air-tight were , in so far as they applied to that object , utterly unnecessary .
I mention this partly as an illustration of the deceptions to which one is liable in this inquiry , and partly because the experiment thus modified seems to tell as clearly against the ammonia theory as the original one seemed to tell in favour of it .
Those receptacles which had been formed by the application of ligatures before the tube was opened afforded certainly no opportunity for the escape of ammonia , and yet in them the blood coagulated as quickly as in those which had communication with the air-implying that facility for the evolution of ammonia does not in itself affect the process of coagulation at all .
How then , it may be said , is the persistent fluidity of the blood under these circumstances to be explained ?
That will become more obvious than I can make it at present in the sequel ; but in the mean time I may observe that there are probably two explanations : one is , the coolness of the tube , and the other , far more important , that the blood , in slipping through this cylindrical tube , had had little opportunity of being influenced by its walls .
The portion of the blood that came first in contact with the walls of the tube had coagulated ; and it is to be observed that I never found , in these experiments , the blood altogether fluid , even after a comparatively short time : there has always been a certain amouLnt of coagulation , and only a certain amount of fluidity .
A layer of blood having thus coagulated upon the internal surface of the tube , the fresh blood which continued to flow through it , was not brought into contact with the walls of the tube at all , but with their lining of coagulated blood .
It has been long known that if blood is stirred with a rod , the process of coagulation is promoted .
It seemed desirable to ascertaini distinctly whether the cause of this was the contact of the foreign solid , or the opportunity givenl for the escape of ammonia ; for it is quite true that , in the ordinary process of stirring blood , more or less air is mixed with it .
For the purpose of determining this I devised a somewhat complicated experiment , which , however , it may be worth while to mention .
I made an apparatus ( fig. 2 ) of two portions of glass tube , A and B , connected in a vertical position by means of vulcanized india-rubber , I , the lower portion of the glass tube being also connected by indiarubber , It , with a wooden handle , which handle , H , was provided with an upright piece of wire , from which spokes pro.ected in different directions , so -Fig .
2. .
--g 7A ~~~_VS S $M_4 ; c a ] 12 , that they would , when moved , act as a churn on any blood contained in the lower portion of tube .
When the lower piece of tube was fixed by means of a vice , V , the flexibility of the india-rubber permitted the churn to be rotated so as to expose the blood to its influence .
This having been arranged , I first poured in strong liquor ammonice , so as to get rid of any slight acidity which the constituents of the apparatus might be conceived to possess , and then , having poured out the ammonia , filled up the apparatus with water , and boiled the whole in a large glass test-tube till all bubbles of air , in any portion of it , were expelled .
Having then tied into a branch of the carotid artery , C , of a calf a bent tube of small diameter , as represented , and having permitted the blood to flow till it escaped at the orifice of the tube , I compressed the artery and passed the tube down through the water to the bottom of the apparatus , and then let the blood flow again , which had the effect of displacing all the water ; and when the blood appeared at the top of the apparatus , the tube was withdrawn , when two effectual clamps , Cl , Cl , were placed on the vulcanized india-rubber connecting A and B ; the india-rubber was then divided between the clamps , and we had the state of things represented at the right-hand side of the diagram .
The upper portion of the apparatus , the orifice of which was exposed to the air , was set aside and left undisturbed .
Having ascertained that the lower portion had been effectually sealed by the clamp , and thus prevented from any opportunity of escape of ammonia , I subjected it to the action of the churn for a certain number of minutes .
It so happened that the blood of that calf was very slow in coagulating .
I knew this from previous experiments on the animal , and therefore continued the action of the churn for a considerable time , viz. thirty-seven minutes .
I then found the wire enveloped in a mass of clot ; and examination of the fluid residue with a needle indicated that the fibrin had been all withdrawn from the blood on which the churn had acted .
I did not now examine the other portion of the apparatus , which had been set aside ; but at the end of an hour and a quarter , when more than double the time had elapsed , I investigated this , and found the blood in it , for the most part , still fluid and coagulable .
Thus the blood in the churn , which , from the time it left the artery , had nio opportunity of parting with its ammonia , coagulated much more rapidly than that in an open vessel .
The difference between the two was , that the lower portion of the blood had been freely exposed to the influence of the foreign solid , whereas the other had only been subjected to the action of the wall of the tube .
The same principle may be illustrated by an exceedingly simple experiment which I performed only this very day .
Receiving blood from the throat of a bullock into two similar wide-mouthed bottles , I immediately stirred one of them with a clean ivory rod for 10 seconds very gently , so as to avoid the introduction of any air , and then left both undisturbed .
At the end of a certain nuinber of minutes I found that , while the blood which had not been disturbed could be poured out as a fluid , with the exception of a thin layer of clot on the surface , and an incrustation on the interior of the vessel , the blood in the other vessel , which had been stirred for so brief a period , was already a solid mass .
I have only lately been aware of the great influence exerted upon the blood by exposure for a very short time to a foreign solid , and I feel that many of my own experiments , and many performed by others , have been vitiated for want of this knowledge .
Take , for example , the effect of a vacuum , which was observed by Sir Charles Scudamore to promote coagulation .
This has been considered by Dr. Richardson as aln illustration of his theory , the vacuum being supposed to ac.t by favouring the escape of ammonia .
I have lately inquired into this subject , and I feel no doubt whatever that the greater rapidity of coagulation in a vacuium depends simply on the greater disturbance of the fluid .
I made the following experiment : I filled three bottles , such as these , from the throat of a bullock , placed one of them under the small bell jar of an air-pump in good order and exhausted it , leaving the other two unldisturbed .
The blood happened to be slow in coagulating ; and at the end of about forty minutes , in the vessels where the blood bad been undisturbed , there was only a slight film of coagulum on the surface , whereas the blood under the vacuum was found on examination to have a very thick crust of clot upon it .
But during the process of exhaustion the blood had bubbled very much .
Indeed , any exhaustion of blood recently drawn which is su-fficient to cause the evolution of its gases induces great bubbling ; so that the pump cannot be used freely , for fear of the froth overflowing .
To this disturbance , involving the exposure of successive portions of blood in the bubbles to the sides of the vessel , I was inclined to attribute the more rapid coagulation ; but in order to prove the point , I stirred for a few seconds the blood in one of the vessels hitherto undisturbed .
After eight minutes I emptied the three vessels .
I found that that blood which had not been disturbed at all , either by the vacuum or by the rod , was still almost entirely fluid , only showing a thin crust upon the glass and on the surface exposed to the air .
The blood which had been subjected to the vacuum had a thick crust of clot on the surface , and the sides of the glass were also thickly encrusted , but it still contained a considerable quantity of fluid that could be poured out from its interior .
But that blood which had been stirred for only a few seconds was a solid mass throughout .
In other words , gentle stirring of the blood for a few seconds bad much greater effect in producing coagulation than the protracted and efficient exhaustion which was continued for upwards of 40 minutes , which was a considerable time after all evolution of gas , as indicated by bubbles , had ceased .
Other experiments precisely similar in their effect were performed .
I therefore feel no hesitation in stating that the effects of a vacuum , regarding which , indeed , the statements of different experimenters have hitherto beenl conflicting , afford no evidence in favour of the ammonia theory .
There is another point of very great interest in the history of the coagulation of the blood , which has been supposed to give support to the ammonia theory ; and that is , the effect of temperature .
It has been long known that blood coagulates more rapidly at a high than at a low temperature , and , indeed , a little above the freezing-point remains entirely fluid .
This seemed beautifully in harmony with the ammonia theory , as heat would naturally promote , and cold retard the evolution of the alkali , and a depression of temperature to near the freezing-point might be reasonably supposed to prevent its escape altogether .
Indeed Dr. Richardson mentions as a fact , that ammonia artificially mixed with blood ceases to be given off under such circumstances .
Though thinking it n)ot unlikely that this was the true explanlation of the influence of temperature on coagulation , I thought it worth while to subject the matter to experiment .
For that purpose I kept the blood of a horse fluid by means of a freezing-mixture , and afterwards by ice-cold water ; and when the corpuscles had subsided from the upper part of the blood , I cautiously added to the liquor sanguinis extremely dilute ice-cold acetic acid till it was of distinctly acid reaction , the liquor sanguinis being of a colour that permitted the delicate application of test-paper , which is impossible with red blood .
By this means any free ammonia which the fluid might have contained must have been neutralized ; yet so long as it was kept in the cold it continued fluiid , but when brought into a warm room , coagulated just as a specimen which had not been acidulated .
Thus , when there could be no free anmmonia in the liquor sanguinis at all , it was still affected as usual by temperature .
This experiment may not be satisfactory to all minds , though I confess it appears so to me ; and as this is a point of very great interest , I have sought in another way for evidence regarding it .
First , however , I will mention an experiment which will not at once appear to bear on the question of temperature .
I drew out a fine glass tube in such a way as to produce a fusiform receptacle continued longitudinally each way into a tube of almost capillary fineness for about two inches , which again expanded at the end , as represented in fig. 3 .
Having squeezed out a drop of blood from iny finger , I sucked up a portion into the tube till the receptacle A and its capillary extensions were filled .
I then broke off the expanded ends , and placed the little tube thus filled , B , in a bath of the strongest liquor ammonia- .
Here certainly the blood was in circumstances in which it could not lose ammonia , but where any change in its amount must be by wav of inierease , and yet I found , on openiig the receptacle by Fig. 3 .
A.= snapping it across after a scratch with a file , that instead of remaining longer fluid than in a watch-glass , the blood in it , being more in contact with the glass , was always more quickly coagulated , while coagulation was still more rapid in the capillary tube , where the blood was still more exposed to the influence of the foreign solid the greater proximity to the liquor ammonim having no influence upon it .
It may perhaps be argued that the drop of blood employed being , a small drop , and this small drop having been drawn up by suction into the tube , it might have parted with its ammonia before it got into the tube ; but then ( and now comes the bearing of the experiment on the effect of temperature ) I found , if I placed a similar tube filled in the same way in a vessel of snow , so as not to freeze it but to keep it icecold , the blood in it remained fluid as long as I chose to keep it there .
Now if all the ammonia had left the blood before it was introduced into the tube , cold ought , according to the ammonia theory , to have had no effect in retarding its coagulation ; for , according to that theory , cold operates by retaining the ammonia .
On the other hand , if we take the other alternative and suppose that any ammornia which the blood might have contained was still in these tubes , the former experiment proves clearly that the retention of ammonia has no effect in producing fluidity-no effect in preventing coagulation ; and if the retenition of ammonia has no effect in preventing coagulation , then cold certainly cannot prevent coagulation by retaining the ammonia , because , even if retained , it would not influence the result .
In whatever way we look at them , therefore , these simple experimenits prove conclusively that cold maintains the fluidity of the blood in some manner unconnected with any influence it may exert upon ammonia .
Then , again , I varied the experiment in this way .
I placed such little tubes of blood in baths of liquor ammonie at different temperatures .
By careful management , guarding against the volatilization of ammonia and consequent reduction of temperature , I succeeded in employing satisfactorily a bath of liquor ammoniae at 1000 F. , the blood being in the bath within a few seconds of its leaving the vessels of my finger , and I found that the high temperature , though uncder such circumstanices it could not possibly dissipate any ammonia from the blood , vet accelerated its coagulation in precisely the same way as when it was applied to blood in watch-glasses exposed to the air .
It is clear , then , that the promotion of the solidification of fibrin by heat is as independent of the evolution of ammonia as the coagulation of albumen under the same agency .
Indeed it seems probable that the two cases are analogous , except that a higher temperature is required in the one than in the other .
When fine tubes containing blood were placed in liquor ammoniae , the alkali acted only upon those parts which were close to the ends of the tubes ; a very small portioni was rendered brownL by it , and beyond that a little was kept permanently fluid , but the chief length of the blood in the tube was uinaffected .
Having thus ascertained that ammonia travels so slowly along tubes of this capillary fineness , I thought T might have an opportunity of giving the ammonia theory a fair test by tying such a tube as has been above described into the jugular vein of a rabbit and filling it directly from the vessel , and then ascertaining whether there was any evidence of retardation of coagulation in the blood thus imprisoned .
But I could discover no such evidence , although I soug , ht for it in confirmation of a view I then held .
To this , however , there is one special exception to be made , viz. in the case of asphyxia .
I found that if two suich tubes were filled from the same blood-vessel of a creature , one under normal circumstances , and the other after asphyxia had been induced , there was a most remarkable difference between the rates of coagulation of the blood in the two tubes , the asphyxial blood coagulating very much more slowly than the ordinary blood ; but when the asphyxial blood was shed into a watch-glass and air was blown through it , it coagulated rapidly , showing that in the state of asphyxia there must be some volatile element in the blood which has an effect in retarding coagulation .
Supposing at first that this volatile element must be ammonia , I hoped to be able by chemical means to find evidence of its accumulation in asphyxia , and thus add a fact of great interest to physiology .
Imitating experiments previously made by Dr. Richardson , I passed air successively through blood and through hydrochloric acid , and then estitnated the amount of ammonia acquired by the latter by means of oichloride of platinum .
In order to prevent the possibility of the loss of any ammonia , I directed blood from the carotid artery of a calf fairly into a Woulfe 's bottle by means of a vulcaniized india-rubber tube tied into the vessel , and then drew a certain volume of air through it by means of an aspirating jar , the experiment being performed first before , and then during asphyxia .
The same procedure was adopted with a second calf , the animal being in each case under chloroform , which does not interfere with the development during asphyxia of the peculiarity in the blood above alluded to ; but I could not find satisfactory evidence of accumulation of ammonia ; and without going further into the question at present , I may say that it seems much more probable that the effect is due to carbonic acid , which is known to have a retardinxg influence on coagulation , and which probably accumulates greatly in asphyxial blood .
But in justice to the author of the ammonia theory , and to myself , too , who at one time expressed a qualified belief in it , it is but fair to say that this theory is extremely plausible .
It has been well shown by Dr. Richardson that ammonia is a substance well fitted to keep the blood fluid if it be present in a sufficient quantity .
An experiment of my own illustrates very well the same point .
I drew out a tube about a quarter of an inch in calibre ( fig. 4 ) , so that while for two inches at one end it retained its original width , the rest ( some ten inches ) was pretty narrow , though far from having the capillary fineness of those before described .
Into the thick part I initroduced a drop of strong liquor ammonie , A , and then securely corked that end of the tube , C. The object of this was that there should be a strong ammoniacal atmosphere in the narrow part of the tube .
I then opened a branch of a vein , V , in the neck of a sheep , introduced the narrow end of the tube into the vessel , and pushing it in so that its Fig. 4 .
__ , V CA _______ ~~~~~~~ la C7 orifice should be in the currenit of the main trunik of the vein , tied it in securely .
I then remnoved the cork and made pressure on the vein at the cardiac side , causing the vessel to swell and blood to pass into the fine part of the tube ; and before the blood had reached the part of the glass moistened by the ammonia , I put in the cork again and withdrew the tube .
In a short time , on introducing a hook of fine wire into the extremity of the tube , I found the blood already coagulated ; but on filing off a small portion of the tube , I found the blood there fluid .
The portion of blood thus exposed soon coagulated , when , a second small piece of the tube being removed by the file , fluid blood was again disclosed , which again soon coagulated ; and this proceeding was repeated with the same results time after time , till , near the thick part of the tube , the ammoniia in the blood was so strong as to prevent coagulation altogether .
This experimenit illustrates how fitted the ammonia is to maintain the fluidity of blood , and also how apt it is , when present in the blood , to fie speedily off from it , leaving it unimpaired in its coagulating properties ; and it must be confessed that the end of the tube sealed with a small clot resembled most deceptively the extremity of a divided artery similarly closed .
But although the experiment seems in so far to favour the ammonia theory , it will tell differelntly when I mention the object with which it was performed .
It appeared to me that , if the cause of the fluidity of the blood was free ammonia , then , if I provided an ammloniacal atmosphere in the tube , and introdlced blood by pressure directly from the veini into this ammoniiacal atmosphere , this blood , lying between the stronig ammoniacal atmosphere on the one side and the ammonia naturally present in the blood withiin the vein on the other side , ought to remaini fluid ; and if it did remain fluid , this would tend to co.nfirm , the ammonia theory by making it appear that the volatile material was the same at both ends of the tube .
But , to my disappointment , I iinvariably found that if I ( Iiew away the tube after a few minutes only had elapsed , there was already a clot in its extremity ; in other words , the amnmoniia had diffused from the end of the tutbe inito the blood within the vein as iito a non-ammoniacal atmosphere .
This experiment alone , if duly considered , would , I think , suffice to show that the blood does not containi enouigh ammonia to aceouIlnt for its fluidity .
Otne more experiment , however , may be adduced .
with the same object .
I mounted a short but wide glass tube , open at both ends ( T , fig. 5 ) , ulpon the enid of a piece of strong wire , W , and connected with the latter a coil of fine silver wire , S , so that it hung freely in the tube .
I then opened the carotid artery of a horse , and through the wound instantly thrust in the apparatus so far that I was sure the tube lay in the common carotid , which in veterinary language means the enormous trunk common to both sides of the neck of the animal .
The tube beinio open at both ends , and slightly funnelshaped at that end which was directed towards the heart , had thus a full current of arterial blood streaming through it .
Having ascertained how long the arterial blood took to show the first appearance of coagulation in a watchglass , I very soon after removed the apparatus , and , on taking out the coil of silver wire , found that it was already crusted over with coagulunm .
Yet here assuredly there had been no opportunity for the escape of ammonia .
From this experiment it is obvious that there is a very great difference between ordinary solid matter and the living vessels in their relation to the blood .
But the same conclusion may be drawn much more simply from experiments which I had the opportunity of performing after making an observation which it seems strange should have been left for me to make , and which , I may say , was made by myself purely accidentally ; and this is , that the blood of mammalia , although it coagulates soon after death in the heart and the principal arterial and venous trunks , remains fluid for an indefinite period in the small vessels .
If , therefore , a ligature be tied round the foot of a living sheep a little below the joint which is divided by the butcher , the foot being removed and taken home with the blood retained in the veins by the ligatiure , we have a ready opportunity of investigating the suibject of coagulation , and of making observations as satisfactory as they are simple .
Here are two feet provided in the way I have alluded to .
A superficial vein in each Fig. S. w foot has been exposed .
The veins I see have contracted very much sinice I reflected the skin from them before our meeting ; and I may remark that such contraction , dependent on muscular action , may occur days after amputation , indicating the persistence of vital properties in the veins .
Now as I cut across this vein , blood flows out , fluid but coagulable .
Into the vein of this other foot has been introduced a piece of fine silver wire , and when I slit up the vein you will see the effect it has produced .
Exactly as far as the silver wire extends , so far is there a clot in this vessel .
Now this experiment , very simple as it is , is of itself sufficient to prove the vital theory in the sense that the living vessels differ entirely from ordinary solids in their relation to the blood .
It is perfectly clear that by introducing a clean piece of silver wire ( and platinum or glass or any other substance chemically inert would have had the same effect ) I do not add any chemical material or facilitate the escape of any , and yet coagulation occurs round about the foreign solid .
Again , if a blood-vessel be injured at any part , coagulation will occur at the seat of injury .
As a good illustration of this , and also as bearing upon the ammonia theory , I may mention the following experiment .
Having squeezed the blood out of a limited portion of one of the veins of a sheep 's foot , and prevented its return by appropriate means , I treated the empty portion with caustic ammonia , the neighbouring parts of the vein being , protected from the irritating vapour by lint steeped in olive oil .
After the smell of ammonia had passed off , I let the blood flow back again and left it undisturbed for a while , when I found on examination a cylindrieal clot in the part that had been treated with ammoniia , while in the adjacent parts of the same vessel the blood remained fluid .
I repeated this experiment several times and always with the same result .
Where the ammonia had aeted there was a clot .
The chemical agent used here was one which , so long as any of it remained , would keep the blood fluid ; yet its ultimate effect was to induce coagulation , the vital properties of the vein having been destroyed by it .
If a needle or a piece of silver wire is introduced for a short time into one of the veins of the sheep 's foot , it is found on withdrawal to be covered over with a very thin crust of fibrin , whereas the wall of the vessel itself is never found to have fibrili or coagulum adhering to it unless it has been injured .
Now this seems to imply that the ordinary solid is the active agent with reference to coag-ulation-that it is not that the blood is maintained fluid by any action of the living vessels , but that it is induced to coagulate by an attractive agency on the part of the foreign solid .
We see at any rate that the foreign solid has an attraction for fibrin which the wall of the vessel has not .
And yet I own I was at first inclined to think that the bloodvessels must in some way actively prevent coagulation .
There were two considerations that led to this view .
One was , that the blood remained fluid in the small vessels after death , but coagulated in the large .
Now why should that be ?
It seemed only susceptible of explanation from there being some connexion between the size of the vessel and the circumstance of coagulation .
It looked as if in the small veins the action of the wall of the vessel was able to control the blood and keep it fluid , but that the large mass in the principal trunks could not be so kept under control .
The other circumstance was , the rapid coagulation of a large quantity of blood shed into a basin .
Why should this occur unless there was some spontaneouis tendency in the blood to coagulate ?
It seemed scarcely credible that it was the result of contact with the surface of the basin .
Both these notions , however , have since been swept away .
In the first place , I have observed recently that it is by no means only in small vessels that the blood remains fluid after death .
If blood be retainied within the jugular vein of a horse or ox by the application of ligatures , either before or after the animal has been struck with the poleaxe , it will often continue fluid , but coagulable , in that vessel , which is upwards of an inch in diameter , for twenty-four or even forty-eight hours after it has been removed from the body .
I say often , but not always .
The jugular vein seems to be in that intermediate condition , between the heart and the small vessels , in which it is uncertain whether it will retain its vital properties for many hours , or will lose them in the course of one hour or so .
Unfortunately for my present purpose , it happens that in this juigular veini , removed from an ox six hours ago , coagulation has already commenced , as I can ascertain by squeezing the vessel between my fingers .
But now that I lay open the vessel , you observe that the chief mass of its contained blood is still fluid , and we shall at all events have an opportunity of seeing , that what is now fluid will in a short tinme be coagulated .
It is an interesting , VOoL .
X-II 2 u circumstance with reference to the question which we are now considering , that the coagulation always begins in contact with the vein , indicatinDg that it is not the wall of the vessel that keeps the blood fluid , but that , on the contrary , the wall of the vessel , when deprived of vital properties , makes the blood coagulate .
The observation of the persistent fluLidity of the blood in these large vessels furnished the opportunity of making a very satisfactory experiment , which I hoped to have exhibited before the Society ; but as there was some clot in the vein , I did not think fit to run the risk of failure .
The experiment is performed in the following way .
A piece of steel wire is wound spirally round one of the veins in its turgid condition , and with a needle and thread the coats of the vessel are stitched here and there to the wire , care being taken to avoid puncturing the lining membrane , and thus the vessel is converted into a rigid cup .
Two such cups being prepared , and the lining membrane of the vein being everted at the orifice of each so as to avoid contact of the blood with any injured tissue , I found that , after pouring blood to and fro through the air in a small stream from one venous receptacle into the other half a dozen times , and closing the orifice of the receptacle to prevent drying , the blood was still more or less completely fluid after the lapse of eight or ten hours .
On the other hand , if a fine sewing , -needle is pushed through the wall of an unopened vessel so that its end may lie in the blood , it is found on examination , after a certain time has elapsed , that the needle is surrounded with an encrusting clot .
It is scarcely necessary to point out how entirely the ammonia theory and the oxygen theory , as well as that of rest , fail to account for facts like these .
While the blood may remain fluid for forty-eight hiouirs in the jugular vein of a horse or an ox , it coagulates soon after death in the heart of very small animals , such as mice ; so that it is obvious that the continuance of fluidity in small vessels is not due to their small size .
It is a very curious question , What is the cause of the blood remaining so much longer fluid in some vessels than in others ?
I belies-e that we must accept it simply as anl ultimate fact , that just as the braini loses its vital properties earlier than the ganglia of the heart , so the heart and principal vascular trunks lose theirs sooller than the smaller vessels of the viscera , or than more superficial vessels , be they large or small .
We can see a final cause for this , so to speak .
So long as the heart is acting , circulation will be sure to go on in the heart and principal trunks ; whereas , on the contrary , the more superficial parts are l able to temporary causes of stagnationi , and occasionally to what amoiunts to practical severance form vascular and nervous connexion with the rest of the body ; and it is , so to speak , of great impoirtance that the blood should not coagulate so speedilv in the vessels of a limb thus circumstanced as it does in the heart after it has ceased to beat .
Were it not for this provision , the surgeon would be unable to apply a touirniquet without fear of coagoilation occurring in the vessels of the limb .
As any illustration of the importance of a knowledge of these facts , I may mention a case that once occurred in my own practice .
I was asked by a surgeon in a couytry district to amputate an arm which he despaired of The brachial artery had been wounded , as well as veins and nerves , and at last , being foiled with the hemorrhage , he wound a long bandage round the limb at the seat of the wound as tightly as he possibly could .
It had been in this condition with the bandage thus applied for fortyeight hours when I reached the patient ; and the limib had all the appearance of being dead .
It was perfectly cold , and any colour which it had was of a livid tint .
But having been lately engaged in some of the experiments which I have been describing , and havin-g thus become much impressed with the persistent vitality of the tissues and the concomitant fluidity of the blood , I determined to give the limb a chance by tying the brachial artery .
Before I left the patient 's house hie had already a pulse at the wrist , and I afterwards had the satisfactitn of hearing that the arm had proved a useful onie .
One of the two arguments in favour of activity Cen the part of the vessels as a cause of the fluidity of the blood having been completely disposed of , let us now consider the other , viz. the rapid coagulation of blood shed into a basin , appearing at first sight to imply a spontaneous tendency of the blood to coagulate , such as would have to be counteracted by the vessels .
This also has proved fallacious .
In the first place it appears that the coagulation , after all , does not go on in a basini so suddenly as one would at first sight suippose , but always commences in contact with the foieign solid .
Wheni blood has beenl shed into a glass jar , if , on the first appearance of a film at the surface , you introduce a mounted needle curved at the end be2 u tween the blood and the side of the glass and make a slight rotatory movement of the handle , you see through the glass the point of the needle detaching a layer of clot whatever part you may examine .
The process of coagulation having thus commenced in contact with the surface of the vessel into which the blood is shed , may under favourable circumstances be ascertained to travel inwards , like advancing crvstallization , towards the centre of the mass .
It appears , however , that this extension of the coagulating process would not take place had not the blood been prepared for the change by contact , during the process of shedding , with the injured orifice of the blood-vessel and with the surface of the receptacle .
I have only very recently become acquainted with the remarkable subtlety of the influence exerted upon blood by ordinary solids .
I was lorng since struck with the fact , that if I introduced the point of an ordinary sewing-needle through the wall of a vein in a sheep 's foot and left it for twelve hours undisturbed , the clot was still confined to a crust round the point of the needle , implying that coagulum has only a very limited power of extension .
I thought , therefore , that by proper management it might be possible to keep blood fluid in a vessel of ordinary solid matter lined with clot .
But various attempts made with this object failed entirely , till I lately adopted the following expedient .
Having opened the distal end of an ox 's jugular vein containing blood and held in the vertical position , taking care to avoid contact of any of the blood with the wounded edge of the vessel , I slipped steadily down into it a cylindrical tube of thin glass , somewhat smaller in diameter than the vein , open at both ends , and with the lower edge ground smooth in order that it might pass readily over the lining membrane , and so disturb the blood as little as possible by its introduction , and influence only the circumferential parts of its contents .
The tube was then kept pressed down vertically upon the bottom of the vein by a weight , in a room as free as possible from vibration , and I found on examining it at the end of twelve hours that the clot was a tubular one , consisting of a crust about one-eighth of an inch thick next the glass and the part exposed to the air , but containing in its interior fluid and rapidly coagulable blood .
In another such experiment , continued for twenty-fours , though the crust of clot was thicker , the central part still furnished coagulable blood .
But it may pernaps be argued by those who say that the bloodvessels are active in maintaining fluidity , that the small portion of the vein covering the end of the tube was acting upon the blood , which certainly was fluid where in contact with it , the clot being in the form of a tube open at the lower end .
To guard against such an objection I made the following experiment:-I extended a tube like that above described by means of thin sheet gutta percha , G(fig .
6a ) , contriving that the internal surface of the gutta percha should be perfectly continuous with that of the glass tube as represented in section in fig. 6 6 .
The lower part of the gutta-percha tissue was strengthened by a ring of soft flexible wire such as is used by veterinary surgeons for sutures , and the wire W was also extended upwards to the top of the glass so as to maintain the rigidity of the gutta-percha portion during its introduction into a vein , but at the same time , from its softness , permit the gutta-percha part to be bent at a right angle after it had been introduced , and so close the orifice of the glass tube with ordinary solid matter .
In fig. 6c the tube is represented pressed down by a weight in a vein V , with blood B in the glass portion , while the gutta-percha part closes it below .
At the same time I performed a comparative experiment , to which I would invite particular attention , although I am sorry at this late hour to occupy the attention of the Society so long .
I tied a thin piece of guttapercha tissue over the lower end of a similar glass tube , and simply Fig. 6 .
a 6 .
c.d Q ' poured blood into it from the jugular veini of an ox .
I wished to compare the condition of blood which had been simply poured into a tube , with blood which had been introduced without any disturbance of its central parts .
But in order to make the experiment a fair one , as it might be said that the blood poured from the vein had been more exposed to the air than that into which the tube was slipped , I proceeded in the following way -I obtained a long vein containling plenty of blood , and having first filled the second tube , with the guittapercha bottom ( fig. 6 d ) , by simply pouring blood into it from the vein , I cut off a portion of the veini which had been thus emptied , and having tied one end and everted the lining merTibrane of the other enid , and having also everted the lining membrane of the orifice of the remaindcer of the vessel which was full , I poured the blood from the full portion through the air into the em pty part .
In doing this I had difficulty in gettintg blood eniongh , and it passed through the air in slow drops , and that only when the vein was squeezed by my warm hand .
At last , having introduLced sufficient for the pwrpose , I slipped down the compound tube arid bent its gutta-perca portion , as represenited in fig. 6 c , and left both tubes for a while und , is , turbed , At the end of three hours aid a half I found that the blood which had been simply poured in was a mass of clot , and fluid squeezed from it yielded no threads of fibrini , coagulation being complete .
Eow long it had beenl so I do not know .
I did not exaniine the other blood until seven hours and three quarters bad expired .
aY1d them found that , just as in the cases where a simple glass tuibe was introduced , the clot was tubular , and the chief part of the blood was still fluid in its interior , the ornly differeniee being that in this ecase the clot formed a complete capsule , being continued over the guitta percha instead of being deficient below , as it was when the vein closed the end of the tube .
Now if we consider the two parts of this comparative experiment , we see that thie receptacles in which the blood was ultimately contained were precisely similar in the two cases , viz. glass tubes closed below with gutta perchla ; and that the blood which was simply poured into the tube was much less exposed to the air than the other , and aso was not subjected , like it , to elevation of temperature , a circumstance which promaotes coagulationi ; but yet this blood becamne completely coag , ulated ill a comparatively short time , whereas the other after a much long , er time was coagulated only in a layer in contact with the foreign solid .
But in the latter case the blood had been so introduiced as to avoid direct action of ordinary matter on any but the circumferential parts of it ; whereas in the former , though poured quickly , it had run down the side of the glass , auid as a consequence of this almost momentary contact with the foreign solid , the central parts , like the circumferential , underwent the process of coagulation .
i Jysterious as this subtle agency of ordinary solids must appear , its occurrence is thus matter of experimental demonstration , and by it the coagulation of blood shed into a basin is accounted for ; while it is also shown conclusively from this experiment that the blood , as it exists within the vessels , has no spontaneous tendenlcy to coagulate , and therefore that the notion of any action on the part of the bloodvessels to prevent coagulation is entirely out of the question .
The peculiarity of the living vessels consists not in any such action upon the blood , but in the circumstanice , remarkable indeed as it is , that their lining membrane , when in a state of health , is entirely negative in its relation to coagulation , and fails to cause that molecular disturbance or , if we may so speak , catalytic action which is produced upoul the blood by all ordinary matter .
I afterwards found that the simplest method of maintaining blood fluid in a vessel composed entirely of ordinary matter was to employ a glass tube similar to those above described , except that its upper end was closed by a cork perfortated by a narrow tube terminating in a piece of vulcanized inidia-rubber tubing that could be closed by a clamnp .
This tube was slipped down inito a vein till the blood , havinSg , filled it completely , showed itself at the orifice of the india-rubber tubing , to which the clamp was then applied .
The whole apparatus was now quickly inverted , and the vein was drawn off from over the mouth of the tube , which was then covered with gutta-percha tissue to prevent evaporation .
After the inverted tube had been kept unidisturbed in the vertical position for nineteen hours and three quarters , coagulable blood was obtained from the interior of the clot .
Ve have seen that a clot has but very slight tendency to induce coagulation in its vicinity unless the blood has been acted on by an ordiniary solid ; and it is probable that with perfectly healthy blood it would be unable to produce such an effect at all .
This appears to me to be very interesting physiologically , but especially so with reference to pathology .
I must not go now fully into the circumstances that lead me to it ; but I may express the opinion I have formed , that clot must be regarded as living tissue in its relation to the blood .
It is no doubt a very peculiar form of tissue , in this respect , that it is soft , easily lacerable , and easily impaired in its vital properties .
If disturbed , as in an aneurism , it will readily be brought into that condition which leads to the deposition of more clot ; but if undisturbed , it not only fails to induce further coagulation , but seems to undergo spontaneous organizationl .
I have seen a clot in the right side of the heart , and extending into the pulmonary artery and its bralnches , unconnected withi the lining membrane of auricle or ventricle or with the pulmonary artery except at one small spot where it had a slight adhesion , developed into perfect fibrous tissue by virtue , it would appear , of its own inherent properties .
Another observation which I once made , and which then completely puzzled me , now seems capable of explanation .
In laying open the blood-vessels of a dead body , I observed in maniy of the veins a delicate white lace-like tissue which evidently must have been formed from a clot .
This I now believe to have had the same relation to the coagulum as the flimsy cellular tissue of old adhesions has to lymph .
It may not be altogether superfluous to mention some other facts illustrative of the active influence of ordinary matter in promoting coagulationl , and the negative charac er of the lining membrane of the vessels .
I find that a needle introduced into one of the veins of the foot of a sheep for a much shorter time than is necessary to produce the first appearance of the actual deposit of fibrill upon it , leads after a while to coagulationi where the needle had lain-in other words , that a foreigni solid , by a short period of action on the blood , brings about a change that results in coagulation , though the blood still lies in the living vessels .
I have also ascertained that after blood has been made to coagulate in a particular vessel by introducing a needle into it , if the coaguliim as well as needle is removed , and more fluid blood is allowed to pass in , this blood remains fluid for an incdefinite period , showing that the nleedIle had not impaired the properties of the vessel by its presence ; so that the previous coagulation must be attributed not to any loss of power in the vein , but simply to the action of the foreign solid .
In seeking for an analogy to this remarkable effect of ordinary solids upon the blood , we are naturally led to the beautiful observations of Professor Graham , lately published in the Philosophical Transactions .
He has there shown what insignificant causes are often sufficient to induce a change from the fluid or soluble to the " cpectous , " or insoluble condition of " colloidal " forms of matter .
Indeed Mr. Graham has himself alluided to the coagulation of fibrin as being probably an example of such a transition .
There is , however , another remarkable circumstance that must be takeni into consideration , of which I myself have been only recently aware , and which may be new to several Fellows of the Society ; and that is , that in spite of the iinfluence of an ordinary solid the liquor sanguinis is not capable of coagulating per se .
It was observed many years ago by my colleague , Professor Andrew Buchanan , of Glasgow , that the fluid of a hydrocele , generally regarded as mrlere serum , coagulated firmly if a little coagulum of blood diffused in water was added to it-an effect which he was disposed to attribute to the agency of the white corpuscles* .
I repeated Dr. Andrew Buchanan 's observations last year , and satisfied myself first that the diffused clot did not act simiply by providing solid particles to serve as starting-points for the coagulating process .
I tried various different materials in a finely divided state , and found that nonie of them , except blood , produced the slightest effect .
But I found that if a mixture of serum and red corpuscles from a clot was added to some of this hydrocele-fluid , it was soon converted into a firm solid mass .
If a small quantity of the serum and corpuscles was diropped into the fluid and allowed to subside without stirring , coagulation rapidly took place in those parts where the red corpuiscles lay , while other parts of the fluid remained for a long tinme uncoagulated .
This seemed to indicate that the red corpuscles had a special virtue in inducing the chanige .
I confess , however , that till very lately I was inclined to suppose that in the hydrocele-fluid the fibrin must be in some peculiar spurious form .
We know that the buffy coat of the horse 's blood coagulates in a glass without addition of clot , and we know that lymph coagulates ; so that I did not doubt Proccedirmis of the Glasgow Philosophical Society , Fehruary 19 , 1845 .
that liquor sanguinis would always undergo the chantge when influenced by ordiniary matter .
But an observation which I made not many days ago , shows that this was a mistake .
I obtained the jugular vein of a horse , and having kept it for a while in a vertical position till I could see through its transparent coats that the red corpuscles had fallen from the upper part , I removed all bloody tissue from that part of the vein , and punctured it so as to let out the Flequor sarnguiinis iinto a glass .
Finding after eighteen minutes that the liquid had not begun to coagulate , I added a drop of serurn and corpuscles to a portion of it , and within seven minutes there was a clot wherever the corpuscles lay , whereas the rest of the fluid was still very imperfectly coaguilated after another half hour had elapsed .
That the liquor sanguinis to which no addition had been made coagulated at all , was sufficiently explained by microscopic investigation , which showed not only abundanit white corpuseles , but also several isolated red ones that had not subsided .
This observation was made three hours after the death of the horse , but I obtained essentially similar results on repeating the experiment in another horse an hour after death ; so that there can be no doubt whatever that the fibrin was in the same condition as it is in the blood-vessels of a living animal .
The observation appears also particularly satisfactory on this account , that the liquor sanguinis was not separated from the corpuscles by any process of transudation through the walls of the blood-vessels , which might be conceived to involve retention of some constituent of the liquid , which , though in solution , might be unable to pass through their pores , but simply by the subsidence of the corpuscles , which must have left all the materials of the liquor sanguinis behinld them .
Hence it is proved beyorid question that if the liquor sanguinis could be separated completely from the blood-corpuscles , it would resemble the fluid of hydrocele in being incapable of coagulation when shed into a cup .
Now this struck me as a very satisfactory and beautiful truth , inasmuch as it clears away all the old mystery of the distinction between inflammatory exudations and dropsical effusionis .
Dropsical efiusions , exhibiting little disposition to coagulate , have been supposed to consist almost excluisively of serum , and the exudation of the entire liquor saniguinis has been regarded as the special characteristic of inflammation ; and very unsatisfactory theories have been put forward by ingenious pathologists to account for this difference .
But it now appears that a dropsical effusion , like that of hydrocele , is undistinguishable from pure liquor sanguinis .
Various dropsical effusions have been lately investigated with reference to their coagulability on the addition of blood-corpuscles , by Dr. Schmidt of Dorpat , who finds that while they differ from one another in the amount of water they contain ( just as is the case with serum filtered artificially through animal membranes under different degrees of pressure ) , yet they are all but universally coagulable .
Schmidt has also carried the investigation further .
He has found that by chemical means be can extract from the red corpuscles a soluble material which , when added to these exudations , leads to coagulation .
In other words , he shows that the corpuscles do not act as living cells , but by virtue of a chemical material which they contain , which can be used in the state of solution , free from any solid particles whatever .
He found also that the aqueous humour made a dropsical effusion coagulaW , and that the same effect was proda:ced by a material extracted from the non-vascular part of the cornea .
1-lence he regards the blood-corpuscles as only resembling other forms of tissue in possessing this property .
These observations are e:xtremely interesting , if trustworthy ; and that they are so , I do not at all doubt ; but having only read Schmidt 's papers within the last day or two , I have not yet had opportunity of verifying , ' his statements* .
It remains to be ascertained what share the material derived from the corpuscles has in the composition of the fibrin .
Schmidt inclines to the opinion that the fibrin is probably composed , in about equal proportions , of a substance fuirriished by them and one present in the liquor sanguinis .
If this be true , the action of an ordinary solid in determining the union of the components of the fibrini may be compared to the operation of spongy platinum in promnoting the combination of oxygen and hydrogen .
It may be asked , How comes it that when the blood of a horse is shed into a cup , the buffy layer coagulates as rapidly , or nearly so , as the lower parts rich in corpuscles ?
This is indeed a question well worthy of careful study .
We know that the liquor sanguinis left by the subsidence of the red corpuscles within a healthy vein is incapable of coagulating when shed , except in a slow manner , which is accounted for by the corpuscles that remain behind in it .
Hence it appears that when the blood as a whole is shed into a glass , the agency of the ordinary solid leads the corpuscles to communiicate to the liquor sanguinis , before they subside , a material or at least an influence which confers upon it a disposition to coagulate , though it still remains fluid for some time after they have left it .
Just as we have seen that a very short time of action of the ordinary solid upon the blood as a whole is sufficient to give rise to coagulationi , so we now see that , provided an ordinary solid be in operation , the presence of the corpuscles for but a little while is enough to make the liquor sanguiniis spontaneously coagulable , though not immediately solidified .
We shall see , before concluding , an illustration of the importance of this fact to pathology .
It remains to be added , that serous membranes resemble the lining melnbrane of the blood-vessels in their relations to the blood , as is implied by John Hunter 's observation that blood , which had lain for several days in a hydrocele , coagulated when let out .
The same thing is well illustrated in a frog prepared like this which I now exhibit .
About four hours ago , a knife having been passed between the brain and cord to deprive the creature of voluntarv mnotion in the limbs and trunk , the peritoneal cavity was laid open in the middle line , and its edges being kept raised and drawn aside by pins , I seized the apex of the ventricle of the heart with forceps and removed it with scissors .
Inl a short time the whole of the animal 's blood was in the peritoneum , and it may be seen that it is still fluid in spite of this long-continued exposure .
When I first performed the experiment three years and a half ago , the weather being cool ( about 45 ?
Fahr. ) and a piece of damp lint being kept suspended above the frog to prevent evaporationi and access of dust , I found that the blood remained fluid in the peritoneal cavity for four days , except a thin film on the surface , and a crust of clot on the wounded part of the heart ; but a piece of clean glass placed in the blood in the peritoneum became speedily coated with coagulum .
Here , it will be observed , not merely the liquor sanguinis , but the corpuscles also were present in the serous cavity , yet no coagulation took place in contact with its walls .
I think it probable , though not yet proved , that all living tissues have these properties with reference to the blood .
We know that the interstices of the cellular tissue contain coagulable fluid , and I have seen anasarcous liquid coagulate after emission ; but this indeed may possibly have been merely liquor sanguinis , coagulating in consequence of slight admixture of blood-corpuiscles from the wounds made in obtaining it .
Looking now at the principal results which we have arrived at , it must , in the first place , be admitted that the ammonia theory is to be discarded as entirely fallacious .
The fact that this theory is exceedingly plausible , and has been supported by many ingenious arguments and experiments , is of course no reason why we should retain it if unsound .
On the contrary , the more specious it is the more necessary is it that it should be effectually cleared away ; for it mystifies the subject of coagulation most seriously ; and I may save , for my own part , that it has cost me an amount of experimental labour of which the illustrations brought forward this evening convey but little idea .
Still these have been , I trust , sufficient to show that the coagulation of the blood is in no degree connected with the evolution of ammonia , any more than with the influence of oxygen or of rest .
The real cause of the coagulation of the blood , when shed from the body , is the influence exerted upon it by ordinary matter , the contact of which for a very brief period effects a change in the blood , inducing a mutual reaction between its solid and fluid constituerts , in which the corpuscles impart to the liquor sanguinis a disposition to coagulate .
This reaction is probably simply chemical in its nature ; yet its product , the fibrin , when mixed with blood-corpuscles in the form of an undisturbed coagulum , resembles healthy living tissues in being incapable of that catalytic action upon the blood which is effected by all ordinary solids , and also by the tissues themselves when deprived of their vital properties .
These principles have , of course , very extensive applications to the study of disease ; but I must content myself with alluding very brieflv to inflammationi , the most important of all pathological conditions , If we inquire what is the great peculiarity of inflamed parts in relation to the blood as exam:rined by the naked eye , we see that it consists in a tenclency to induce coagulation in their vicinity-implying , according to the conielusions just stated , that the affected tissues have lost for the time being their vital properties , and coimport themselves like ordinary solids .
Ths , when an artery or vein is inflamed , coagulation occurs upon its interior , in spite of the current of blood , precisely as would take place if it hadl been artificially deprived of its vital properties .
On one occasion I simulated the characteristic adherent clot of Phlebitis by treating the jugular vein of a living sheep with caustic ammonia , and then allowing the circulation to go on through the vessel for a while , when , on slitting it up , I found its lining membralne studded with grains of pink fibrin which could be detached only by scraping firmly with the edge of a knife .
Agaill , comparing an inflammatory exudation into the pericar(lium or into the initerstices of the cellular tissue with dropsical effusions into the same situations , we are struck with the fact that , while the liquor sanguinis effused in dropsy remains fluid , the inflammatory product coagulates .
Now we know that in intense inflammation the capillaries are choked more or less with accumulated blood-corpuscles , which must cause great increase in the pressure of the blood upon their walls ; and froDI what we know of the effect of venous obstruction in causing dropsical effusion of liquor sanguinis through increased pressure , we are sure that we have in the iulflammatory state the physical conditions for a similar transudation of fluid through the walls of the capillaries .
And the inatural interpretation of the difference in the two cases as regards coagulationi seems to be , that whereas in dropsy the fluid is forced through the pores of healthy vessels , in iinflammation the capillary parietes hbave lost their healthy condition , and act like ordinary matter ; so that the liquor sanguinis , having been subjected , immediately before effusion , to the combined influence of the injured tissue and the blood-corpuscles , has acquired a disposition to coagulate , juis like the buffy coat of horses ' blood shed into a glass , or like the frog 's liquor sanguinis filtered by Miiller from its corpuscles , the injured vessels acting uponl the blood like the filter .
This view of the condition of intensely inflamed parts is exactly that to which I was led some years ago by a microscopic investigation , the results of which were detailed in a paper* that received the honour of a place in the Philosophical Transactions .
It was there shown , as I thinik I may veniture to say , that the tissues generally are capable of being reduced under the action of irrita ts to a state quite distinct from death , but in which they are nevertheless temporarilyr deprived of all vital power , and that inflammatory congestion is due to the blood-corpuscles acquiring adhesiveness sueh as they lIave outside the body , in consequence of the irritated tissues acting towards them like ordinary solids .
I cannot avoid expressing my satisfaction that this inquiry inito the coagullation of the blood has furnished indepeildent confirmation of my previous conclusions regarding the nature of inflammation .
|
112321 | 3701662 | On the Molecular Mobility of Gases. [Abstract] | 611 | 623 | 1,862 | 12 | Proceedings of the Royal Society of London | Thomas Graham | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 13 | 184 | 5,106 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112321 | null | http://www.jstor.org/stable/112321 | null | 108,802 | Thermodynamics | 49.789969 | Fluid Dynamics | 24.053668 | Thermodynamics | [
-19.78261375427246,
-47.27120590209961
] | I. " On the Molecular Mobility of Gases .
" By TIol-MAs GRAHAM , F.R.S. , Mastelr of the Mint .
Received May 7 , 1863 .
( Abstract ) .
The molecular mobility of gases is here considered in reference chiefly to the passage of gases , under pressure , through a thin porous plate or septum , and to the partial separation of mixed gases which can be effected , as will be shown , by such means .
The investigation * " On the Early Stages of Inflammation , " Phil. Trans. for 1858 .
1863 .
] 611 arose out of a renewed and somewhat protracted inquiry regarding the diffusion of gases ( depending upon the same molecular mobility ) , and has afforded certain new results which may prove to be of interest in a theoretical as well as in a practical point of view .
In the diffusiometer , as first constructed , a plain cylindrical glass tube , rather less than an inch in diameter and about ten inches in length , was simply closed at one end by a porous plate of plaster of paris , about one-third of an inch in thickness , and thus converted into a gas receiver* .
A superior material for the porous plate is now found in the artificially compressed graphite of Mr. Brockedon , of the quality used for making writing-pencils .
This material is sold in London in small cubic masses about 2 inches square .
A cube may easily be cut into slices of a millimetre or two in thickness by means of a saw of steel spring .
By rubbing the surface of the slice without wetting it upon a flat sand-stone , the thickness may be further reduced to about one-half of a millimetre .
A circular disk of this graphite , which is like a wafer in thickness but possesses considerable tenacity , is attached by resinous cement to one end of the glass tube above described , so as to close it and form a diffusiometer , The tube is filled with hydrogen gas over a mercurial trough , the porosity of the graphite plate being counteracted for the time by covering it tightly with a thin sheet of gutta percha .
On afterwards removing the latter , gaseous diffusion immediately takes place through the pores of the graphite .
The whole hydrogen will leave the tube in forty minutes or an hour , and is replaced by a much smaller proportion of atmospheric air ( about one fourth ) , as is to be expected from the law of the diffusion of gases .
During the process , the mercury will rise in the tube , if allowed , forming a column of several inches in height-a fact which illustrates strikingly the intensity of the force with which the interpenetration of different gases is effected .
The native or mineral graphite is of a lamellar structure , and appears to have little or no porosity .
It cannot be substituted for the artificial graphite as a diffusion-septum .
Unglazed earthenware comes next in value to graphite for this purpose .
The pores of artificial graphite appear to be really so minute , that a gas in mass cannot penetrate the plate at all .
It seems to be molecules only which can pass ; and these may be supposed to pass wholly unimpeded by friction , for the smallest pores that can be imagined to exist in the graphite must be tunnels in magnitude to the ultimate atoms of a gaseous body .
The sole motive agency appears to be that intestine movement of molecules which is now generally recognized as an essential property of the gaseous condition of matter .
According to the physical hypothesis now generally received ' , a gas is represented as consisting of solid and perfectly elastic spherical particles or atoms , which move in all directions , and are animated with different degrees of velocity in different gases .
Confined in a vessel , the moving particles are constantly impinging against its sides and occasionally against each other , and such collisions take place without any loss of motion , owing to the perfect elasticity of the particles .
Now if the containing vessel be porous , like a diffusiometer , then gas is projected through the open channels , by the atomic motion described , and escapes .
Simultaneously the external air or gas , whatever it may be , is carried inwards in the same manner , and takes the place of the gas which leaves the vessel .
To the same atomic or molecular movement is due the elastic force , with the power to resist compression , possessed by gases .
The molecular movement is accelerated by heat and retarded by cold , the tension of the gas being increased in the first instance and diminished in the second .
Even when the same gas is present both within and without the vessel , and is therefore in contact with both sides of the porous plate , the movement is sustained without abatement-molecules continuing to enter and leave in equal number , although nothing of the kind is indicated by change of volume or otherwise .
If the gases in communication be different but possess sensibly the same specific gravity and molecular velocity , as nitrogen and carbonic oxide do , an interchange of molecules also takes place without any change in volume .
With gases opposed of unequal density and molecular velocity , the amount of penetration ceases of course to be equal in both directions .
* D. Bernoulli , J. Herapath , Joule , KrInig , Clausius , Clerk Maxwell , and Cazin .
The merit of reviving this hypothesis and first applying it to the facts of gaseous diffusion , is fairly due to Mr. Herapath .
See 'Mathematical Physics , ' in two volumes , by John Herapath , Esq. ( 1847 ) .
These observations are preliminary to the consideration of the passage through a graphite plate , in one direction only , of gas under pressure , or under the influence of its own elastic force .
It is to be supposed that a vacuum is maintained on one side of the porous septum , and that air or some other gas , under a constant pressure , is in contact with the other side .
Now a gas may pass into a vacuum in three different modes , or in two modes besides that immediately before us .
1 .
The gas may enter the vacuum by passing through a minute aperture in a thin plate , such as a puncture in platinum foil made by a fine steel point .
The rate of passage of different gases is then regulated by their specific gravities , according to a pneumatic law which was deduced by Professor John Robison from Torricelli 's well-known theorem of the velocity of efflux of fluids .
A gas rushes into a vacuum with the velocity which a heavy body would acquire by falling from the height of an atmosphere composed of the gas in question , and supposed to be of uniform density throughout .
The height of the uniform atmosphere will be inversely as the specific gravity of the gas , the atmosphere of hydrogen , for instance , sixteen times higher than that of oxygen .
But as the velocity acquired by a heavy body in falling is not directly as the height , but as the square root of the height , the rate of flow of different gases into a vacuum will be inversely as the square root of their respective densities .
The velocity of oxygen being 1 , that of hydrogen will be 4 , the square root of 16 .
This law has been experimentally verified* .
The times of the effusion of gases , as I have spoken of it , are similar to those of the law of molecular diffusion ; but it is important to observe that the phenomena of effusion and diffusion are distinct and essentially different in their nature .
The effusion movement affects masses of gas , the diffusion movement affects molecules ; and a gas is usually carried by the former kind of impulse with avelocity many thousand times greater than by the latter .
The effusion velocity of air is the same as the velocity of sound .
2 .
If the aperture of efflux be in a plate of increased thickness , and so becomes a tube , the effusion-rates of gases are disturbed .
The rates of flow of different gases , however , assume again a constant ratio to each other when the capillary tube is considerably elongated , when the length exceeds , the diameter at least 4000 times .
These new proportions of efflux are the rates of the " Capillary Transpiration of Gases " * .
The rates were found to be the same in a capillary tube composed of copper as they are in a tube of glass , and appear to be independent of the material of the capillary .
A film of gas no doubt adheres to the inner surface of the tube , and the friction is really that of gas upon gas , and is consequently unaffected by the nature of the tube-substance .
The rates of transpiration are not governed by specific gravity , and are indeed singularly unlike the rates of effusion .
The transpiration-velocity of oxygen being 1 , that of chlorine is 1'5 , that of hydrogen 2'26 , of ether vapour at low temperatures the same or nearly the same number as hydrogen , of nitrogen and carbonic oxide half the velocity of hydrogen , of olefiant gas , ammonia , and cyanogen 2 ( double or nearly double that of oxygen ) , of carbonic acid 13 76 , and of the gas of marshes 1'815 .
In the same gas the transpirability of equal volumes increases with density , whether occasioned by cold or pressure .
The transpiration-ratios of gases appear to be in constant relation with no other known property of the same gases , and they form a class of phenomena remarkably isolated from all else at present known of gases .
There is one property of transpiration immediately bearing upon the penetration of the graphite plate by gases .
The capillary offers to the passage of gas a resistance analogous to that of friction , proportional to the surface , and consequently increasing as the tube or tubes are multiplied in number and diminished in diameter , with the area of discharge preserved constant .
The resistance to the passage of a liquid through a capillary was observed by Poiseuille to be nearly as the fourth power of the diameter of the tube .
In gases the resistance also rapidly increases ; but in what ratio , has not been observed .
The consequence , however , is certain , that as the diameter of the capillaries may be diminished beyond any assignable limit , so the flow may be retarded indefinitely , and caused at last to become too small to be sensible .
We may therefore have a mass of capillaries of which the passages form a large aggregate , but which are individually too small to permit a sensible flow of gas under pressure .
A porous solid mass may possess the same reduced penetrability as the congeries of capillary tubes .
Indeed the state of porosity described appears to be more or less closely approached by all loosely aggregated mineral masses , such as lime plaster , stucco , chalk , baked clay , non-crystalline earthy powders like hydrate of lime or magnesia compacted by pressure , and in the highest degree perhaps by artificial graphite .
3 .
A plate of artificial graphite , although it appears to be practically impenetrable to gas by either of the two modes of passage previously described , is readily penetrated by the agency of the molecular or diffusive movement of gases .
This appears on comparing the time required for the passage of equal volumes of different gases under a constant ptessure .
Of the following three gases , oxygen , hydrogen , and carbonic acid , the time required for the passage of an equal volume of each through a capillary glass tube , in similar circumstances as to pressure and temperature , was formerly observed to be as follows : Time of capillary transpiration .
Oxygen ... ... ... ... .
1 Carbonic acid ... ... ... 0'72 Hydrogen ... ... ... ... . .
044 Through a plate of graphite , of half a millimetre in thickness , the same gases were now observed to pass , under a constant pressure of a column of mercury of 100 millimetres in height , in times which are as follows : Time of molecular Square root of density passage .
( oxygen 1 ) .
Oxygen ... ... ... 1 ... .
1 Iydrogen ... ... ... .
0-2472 ... .
0-2502 Carbonic acid ... ... . .
11886 ... .
11760 It appears then that the times of passage through the graphite plate have no relation to the capillary transpiration-times of the same gases first quoted above .
The new times in question , however , show a close relation to the square roots of the densities of the respective gases , as is seen in the last Table ; and so far they agree with theoretical times of difusion usually ascribed to the same gases .
The experiments were varied by causing the gases to pass into a Torricellian vacuum , and consequently under the full pressure of the 616 atmosphere .
The times of penetration of equal volumes of gases were nowTimes .
V/ Density , Oxygen ... ... ... . .
1 ... .
1 Air.0 ... ... ... ... 9501 ... .
09507 Carbonic acid ... ... 1-1860 ... .
1P1760 Hydrogen ... ... ... 0-2505 ... .
0-2502 This penetration of the graphite plate by gases appears to be entirely due to their own proper molecular motion , quite unaided by transpiration .
It seems to offer the simplest possible exhibition of the molecular or diffusive movement .
This pure result is to be ascribed to the wonderfully fine porosity of the graphite .
The interstitial spaces , or channels , appear to be sufficiently small to extinguish transpiration , or the passage of masses , entirely .
The graphite becomes a molecular sieve , allowing molecules only to pass through .
With a plate of stucco , the penetration of gases under pressure is very rapid , and the volumes of air and hydrogen passing in equal times are as 1 to 2'891 , which is a number for hydrogen intermediate between its transpiration-volume 2'04 and diffusion-volume 3 8 , showing that the passage through stucco is a mixed result .
With a plate of biscuitware , 2-2 millimetres in thickness , the volume of hydrogen rose to 3'754 ( air= 1 ) , approaching closely to 3'8 , the molecular ratio .
The rate of passage of a gas through graphite appeared also to be closely proportional to the pressure .
Further , hydrogen was found to penetrate through a graphite plate into a vacuum , with sensibly the same absolute velocity as it diffused into air , establishing the important fact that the impelling force is the same in both movements .
The molecular mobility may therefore be spoken of as the diffusive movement of gases ; the passage of gas through a porous plate into vacuum , as diffusion in one direction or single diffusion ; and ordinary diffusion , or the passage of two gases in opposite directions , as double , compound , or reciprocal diffusion .
Atmolysis.-A partial separation of mixed gases and vapours of unequal diffusibility can be effected by allowing the mixture to permeate through a graphite plate into a vacuum , as was to be expected from the preceding views .
As this method of analysis has a practical character and admits of wide application , it may be convenient to 1863 .
] 617 distinguish it by a peculiar name .
The amount of the separation is in proportion to the pressure , and attains its maximum when the gases pass into a nearly perfect vacuum .
A variety of experiments were made on this subject , of which perhaps the most interesting were those upon the concentration of the oxygen in atmospheric air .
When a portion of air confined in a jar is allowed to penetrate into a vacuum through graphite or unglazed earthenware , the nitrogen should pass more rapidly than the oxygen in the proportion of 1'0668 to 1 , and the proportion of oxygen be proportionally increased in the air left behind in the jar .
The increase in the oxygen actually observed when the air in the jar was reduced from 1 volume To 0'5 volume , was 0'48 per cent. 0-25 , , , , 0'98 0-125 , 1-54 0-0625 , , , 2-02 Or , the oxygen increased from 21 to 23'02 per cent. in the last sixteenth part of air left behind in the jar .
The most remarkable effects of separation are produced by means of the tu6e atmolyser .
This is simply a narrow tube of unglazed earthenware , such as a tobacco-pipe stem two feet in length , which is placedwithin a shorter tube of glass and secured in its position by corks , so as to appear like a Liebig 's condenser .
The glass tube is placed in communication with an air-pump , and the annular space between the two tubes is maintained as nearly vacuous as possible .
Air or any other mixed gas is then allowed to flow in a stream along the clay tube , and collected as it issues .
The gas so atmolysed is of course reduced in volume , much gas penetrating through the pores of the clay tube into the air-pump vacuum ; and the slower the gas is collected the greater the proportional loss .
In the gas collected , the denser constituent of the mixture is thus concentrated in an arithmetical ratio , while the volume of the gas is reduced in a geometrical ratio .
In one experiment the proportion of oxygen in the air after traversing the atmolyser was increased to 24-5 per cent. , or 16'7 upon 100 oxygen originally present in the air .
With gases differing so much in density and diffusibility as oxygen and hydrogen , the separation is of course much more considerable .
The explosive mixture of two volumes of hydrogen and one volume of oxygen , gave oxygen containing only 93 per cent. of hydrogen , in which a taper burned without explosion ; and with equal volumes of oxygen and hydrogen , the proportion of the latter was easily reduced from 50 to 5 per cent. Interdifusion of Gases-double diffusion.-The diffusiometer was much improved in construction by Prof. Bunsen , from the application of a lever arrangement to raise and depress the tube in the mercurial trough .
But the mass of stucco forming the porous plate in his instrumeht was too voluminous , in my opinion , and , from being dried by heat , had probably detached itself from the walls of the glass tube .
The result obtained of 3 4for hydrogen , air being 1 , is , I understand , no longer insisted upon by that illustrious physicist .
It is indeed curious that my old experiments generally rather exceeded than fell short of the theoretical number for hydrogen , 9=7997 .
With stucco as the material , the cavities in the porous plate form about one-fourth of its bulk , and affect sensibly the ratio in question , according as they are or are not included in the capacity of the instrument .
Beginning the diffusion always with these cavities filled with hydrogen , the numbers now obtained with a stucco plate of 12 millims. in thickness , dried without heat , were 3 783 , 3'8 , and 3'739 when the volume of the cavities of stucco is added to the air and hydrogen , and 3'931 , 3'949 , and 3*883 when such addition is not made to these volumes .
The graphite plate , on the other hand , being thin , and the volume of its pores too minute to require to be taken into account , its action is not attended with the same uncertainty .
With a graphite plate of 2 millims. in thickness , the number for hydrogen into air was 3'876 , and of hydrogen into oxygen 4'124 , instead of 4 .
With a graphite plate of 1 millim. in thickness , hydrogen gave 3'993 to air I. With a graphite plate of 0'5 millim. in thickness , the proportional number for hydrogen to air rose to 3*984 , 4*068 , and 4'067 .
A similar departure from the theoretical number was observed when hydrogen was diffused into oxygen or carbonic acid , instead of air .
All these experiments were made over mercury and with dried gases .
It appears that the numbers are most in accordance with theory when the graphite plate is thick , and the diffusion slow in consequence .
If the diffusion be very rapid , as it is with the thin plates , something like a current is possibly formed in the channels of the graphite , 1863 .
] 619 taking the direction of the hydrogen and carrying back in mass a little air , or the slower gas , whatever it may be .
I cannot account otherwise for the slight predominance which the lighter and faster gas appears always to acquire in diffusing through the porous septum .
Speculative ideas respecting the constitution of matter .
It is conceivable that the various kinds of matter , now recognized as different elementary substances , may possess one and the same ultimate or atomic molecule existing in different conditions of movement .
The essential unity of matter is an hypothesis in harmony with the equal action of gravity upon all bodies .
We know the anxiety with which this point was investigated by Newton , and the care he took to ascertain that every kind of substance , " metals , stones , woods , grain , salts , animal substances , &c. , " are similarly accelerated in falling , and are therefore equally heavy .
In the condition of gas , matter is deprived of numerous and vary .
ing properties with which it appears invested when in the form of a liquid or solid .
The gas exhibits only a few grand and simple features .
These again may all be dependent upon atomic and molecular mobility .
Let us imagine one kind of substance only to exist , ponderable matter ; and further , that matter is divisible into ultimate atoms , uniform in size and weight .
We shall have one substance and a common atom .
With the atom at rest the uniformity of matter would be perfect .
But the atom possesses always more or less motion , due , it must be assumed , to a primordial impulse .
This motion gives rise to volume .
The more rapid the movement the greater the space occupied by the atom , somewhat as the orbit of a planet widens with the degree of projectile velocity .
Matter is thus made to differ only in being lighter or denser matter .
The specific motion of an atom being inalienable , light matter is no longer convertible into heavy matter .
In short , matter of different density forms different substances-different inconvertible elements as they have been considered .
What has already been said is not meant to apply to the gaseous volumes which we have occasion to measure and practically deal with , but to a lower order of molecules or atoms .
The combining atoms hitherto spoken of are therefore not the molecules of which the movement is sensibly affected by heat , with gaseous expansion as 620 [ June 18 , the result .
The gaseous molecule must itself be viewed as composed of a group or system of the preceding inferior atoms , following as a unit laws similar to those which regulate its constituent atoms .
We have indeed carried one step backward and applied to the lower order of atoms ideas suggested by the gaseous molecule , as views derived from the solar system are extended to the subordinate system of a planet and its satellites .
The advance of science may further require an indefinite repetition of such steps of molecular division .
The gaseous molecule is then a reproduction of the inferior atom on a higher scale .
The molecule or system is reached which is affected by heat , the diffusive molecule , of which the movement is the subject of observation and measurement .
The diffusive molecules are also to be supposed uniform in weight , but to vary in velocity of movement , in correspondence with their constituent atoms .
Accordingly the molecular volumes of different elementary substances have the same relation to each other as the subordinate atomic volumes of the same substances .
But further , these more and less mobile or light and heavy forms of matter have a singular relation connected with equality of volume .
Equal volumes of two of them can coalesce together , unite their movement , and form a new atomic group , retaining the whole , the half , or some simple proportion of the original movement and consequent volume .
This is chemical combination .
It is directly an affair of volume , and only indirectly connected with weight .
Combining weights are different , because the densities , atomic and molecular , are different .
The volume of combination is uniform , but the fluids measured vary in density .
This fixed combining measure the metron of simple substances-weighs 1 for hydrogen , 16 for oxygen , and so on with the other " elements .
" To the preceding statements respecting atomic and molecular mobility , it remains to be added that the hypothesis admits of another expression .
As in the theory of light we have the alternative hypotheses of emission and undulation , so in molecular mobility the motion may be assumed to reside either in separate atoms and molecules , or in a fluid medium caused to undulate .
A special rate of vibration or pulsation originally imparted to a portion of the fluid medium enlivens that portion of matter with an individual existence , and constitutes it a distinct substance or element .
621 With respect to the different states of gas , liquid , and solid , it may be observed that there is no real incompatibility with each other in these physical conditions .
They are often found together in the same substance .
The liquid and the solid conditions supervene upon the gaseous condition rather than supersede it .
Gay-Lussac made the remarkable observation that the vapours emitted by ice and water , both at 0 ?
C. , are of exactly equal tension .
The passage from the liquid to the solid state is not made apparent in the volatility of water .
The liquid and solid conditions do not appear as the extinction or suppression of the gaseous condition , but something superadded to that condition .
The three conditions ( or constitutions ) probably always coexist in every liquid or solid substance , but one predominates over the others .
In the general properties of matter we have , indeed , to include still further ( 1 ) the remarkable loss of elasticity in vapours under great pressure , which is distinguished by Mr. Faraday as the Caignard-Latour state , after the name of its discoverer , and is now undergoing an investigation by Dr. Andrews , which may be expected to throw much light upon its nature ; ( 2 ) the colloidal condition or constitution , which intervenes between the liquid and crystalline states , extending into both and affecting probably all kinds of solid and liquid matter in a greater or less degree .
The predominance of a certain physical state in a substance appears to be a distinction of a kind with those distinctions recognized in natural history as being produced by unequal development .
Liquefaction or solidification may therefore not involve the suppression of either the atomic or the molecular movement , but only the restriction of its range .
The hypothesis of atomic movement has been elsewhere assumed , irrespective of the gaseous condition , and is applied by Dr. Williamson to the elucidation of a remarkable class of chemical reactions which have their seat in a mixed liquid .
Lastly , molecular or diffusive mobility has an obvious bearing upon the communication of heat to gases by contact with liquid or solid surfaces .
The impact of the gaseous molecule , upon a surface possessing a different temperature , appears to be the condition for the transference of heat , or the heat movement , from one to the other .
The more rapid the molecular movement of the gas the more frequent the contact , with consequent communication of heat .
Hence , probably , the great cooling power of hydrogen gas as compared with air 62 or oxygen .
The gases named have the same specific heat for equal volumes ; but a hot object placed in hydrogen is really touched 3'8 times more frequently than it would be if placed in air , and 4 times more frequently than it would be if placed in an atmosphere of oxygen gas .
Dalton had already ascribed this peculiarity of hydrogen to the high " mobility " of that gas .
The same molecular property of hydrogen recommends the application of that gas in the air-engine , where the object is to alternately heat and cool a confined volume of gas with rapidity .
|
112322 | 3701662 | Results of the Magnetic Observations at the Kew Observatory, from 1858 to 1862 Inclusive. --No. I. [Abstract] | 623 | 625 | 1,862 | 12 | Proceedings of the Royal Society of London | Edward Sabine | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 20 | 899 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112322 | null | http://www.jstor.org/stable/112322 | null | null | Meteorology | 67.631387 | Tables | 21.657761 | Meteorology | [
48.74797821044922,
8.235809326171875
] | II .
" Results of the Magnetic Observations at the Kew Observatory , from 1858 to 1862 inclusive."-No .
I. By MajorGeneral EDWARD SABINE , P.R.S. Received May 2 ] , 1863 .
( Abstract .
) The first three sections of this paper are occupied by a discussion of the Laws of the Disturbances of the Magnetic Declination at Kew , derived from the photographic records of the Kew Observatory between January 1 , 1858 , and December 31 , 1862 .
In the first section a synoptical table is given , showing the direction and amount of the easterly and of the westerly deflections of the declination magnet at 24 equidistant epochs on each of 95 days of principal disturbance occurring in the years 1858 to 1862 inclusive .
The deflections are measured from the normals of the same month and hour , computed from the undisturbed positions at the same epochs on the 1825 days comprised in the five years since the commencement of the photographic records .
The phenomenal laws of the disturbances on the 95 days are then investigated , and are compared with the corresponding laws derived from a far larger number of observations in the same years , taken out by the well-known process employed by the author in the reduction of the observations of the colonial magnetic observatories .
The result is shown to be that , so far as the laws of the disturbances are concerned , the two processes furnish mutual confirmation the laws being approximately the same whether they are derived from the whole body of the hourly positions , or from that portion only which includes 95 days ( or on an average 19 days in each year ) which were specially affected by disturbance , -but that , for the purpose of eliminating the effects of the disturbances in the 623 s1863 .
] subsequent investigation of the secular , periodical , and other minor magnetic variations , the process of elimination introduced by the author and employed by him for several years past in the reduction of the colonial observations has the advantage of separating from the whole body of the observations a far greater portion of the disturbing influence than would be gained by the simple omission of the observations on the 95 days .
The laws of the disturbance-diurnal variation , thus found to be approximately the same whether obtained from the narrower or from the wider basis of investigation , are then stated , and are compared with the results of similar investigations recorded in the author 's previous publications the points of accordance or of difference being severally discussed in the third section .
The fourth section contains Tables of the " Diurnal Inequality , " and of the " Solar-diurnal Variation " at Kew , showing the mean values at each hour and in each month .
The " Diurnal Inequality " is explained as consisting of two principal constituents , viz. the " Disturbance-diurnal Variation , " and the " Solar-diurnal Variation .
" It is obtained for each month by taking the differences between the mean positions of the magnet at each of the 24 hours , in the month , and the mean position in the month itself ( viz. the mean of all the days and all the hours)-no omission whatsoever being made of disturbed observations .
The " Solar-diurnal Variation " is obtained by a similar process , after the separation and omission of all the observations which differed by a certain small and constant value from the normals of the same month and hour .
By this process the effects of the " Casual and Transitory changes " are in a very great degree eliminated , and a very close approximation is obtained to the systematic diurnal action of the sun upon the direction of the horizontal magnet , apart from the effects of disturbances .
The solar-diurnal variation thus obtained at Kew is compared with results similarly obtained at six other stations , viz. three stations in the interior of the two great northern continents , one equatorial station , and two stations in the middle latitudes of the southern hemisphere-thus generalizing upon a very extensive scale the action of the sun in producing the phenomena under notice .
The fifth section is occupied by a similar generalization of the facts which have placed in evidence the existence of a semiannual inequality 624 [ June 18 , in the solar-diurnal variation , having its epochs coincident , or very nearly so , with the sun 's passage of the equator , and dependent consequently on the earth 's position in its orbit .
The sun 's action in producing this semiannual inequality is shown to be characteristically different from that which is manifested in the solar-diurnal variation itself , pointing apparently to a difference in the mode of the sun 's action in the two cases .
The sixth section contains a tabular view of the " ' Lunar-diurnal Variation " at Kew , in each of the five years during which the photographic record has been maintained there ; this is followed by a comparison with similar results at other stations on the globe , and a statement of the principal points of agreement or of difference which are shown thereby .
|
112323 | 3701662 | Results of the Magnetic Observations at the Kew Observatory, from 1858 to 1862 Inclusive. --No. II. [Abstract] | 625 | 630 | 1,862 | 12 | Proceedings of the Royal Society of London | Edward Sabine | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 6 | 57 | 2,289 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112323 | null | http://www.jstor.org/stable/112323 | null | null | Meteorology | 86.067869 | Tables | 11.233512 | Meteorology | [
48.41633987426758,
8.409632682800293
] | III .
" Results of the Magnetic Observations at the Kew Observatory , from 1858 to 1862 inclusive."--No .
II .
By MajorGeneral EDWARD SABINE , P.R.S. Received June 18 , 1863 .
( Abstract .
) This paper is a continuation of the preceding one .
It consists of two sections , the seventh and eighth .
In the seventh section the author discusses the secular change and annual variation of the declination ; and in the eighth section , the annual variation or semiannual inequality of the inclination and of the horizontal and total magnetic force .
Seventh Section.-The positions of the horizontal magnet at 24 equidistant epochs in the day , tabulated from the photograms of the Kew declinometer , with the omission of the disturbed observations , as described in the former paper , are grouped in weekly means , forming 52 mean values , corresponding to the number of weeks in the year .
A Table is given of these weekly values , comprehending , in five columns , the five years from January 1858 to December 1862 inclusive , and from these a sixth column is formed , representing the mean declination in each of the 52 weeks of a mean or typical year , corresponding in this instance to the year 1860 .
The mean declination obtained from all the weekly results in the five years , and corresponding to its middle epoch July 1 , 1860 , is 21§ 39 ' 18"f1 ; and from a comparison of the mean declinations corresponding to July 1 in the 1863 .
] 625 columns which severally present the weekly values in the years from 1858 to 6182 inclusive , the mean value of the secular change corresponding to the period comprised in the Table is deduced .
A proportional part of the secular change is then applied with its appropriate sign to each of the weekly values in the mean or typical year .
These should all correspond with the mean declination of the whole Table ( viz. 21§ 39 ' 18 " -1 ) , or should exhibit only such small and unsystematic differences as might reasonably be ascribed to casual errors .
The final column of the Table contains these differences , in which it is at once seen that they divide themselves into two distinct categories , distinguished by the sign in the semiannual period from March 21 to Sept. 21 , and by the + sign from Sept. 21 to March 21 .
Hence the author infers the existence of a variation in the declination at Kew having an annual period , and consisting of a semiannual inequality with epochs coincident , or nearly so , with the sun 's passage of the equator the magnet being deflected towards the east when the sun is north , and towards the west when he is south of the equator .
The amount of the semiannual inequality , as shown by the Table , averages 28"'95 in the weeks from March 21 to Sept. 21 , and 29"'9 in those from September to March .
The whole amount of the annual variation at Kew is therefore 58"'85 .
The result thus obtained from the observations at Kew is compared with the result of an investigation of the corresponding phenomena at Hobarton in the southern hemisphere , obtained from hourly observatious of the declination during five years , commencing in October 1843 , and terminating in September 1848 .
The observations themselves are published in the 2nd and 3rd volumes of the Hobarton Observations , and are treated , for the purposes of this paper , precisely in the same way as those of the Kew Observatory , forming a table strictly analogous to the one , previously described , at Kew .
The final column of the Hobarton Table exhibits the differences , in each of the 52 weeks of the typical year , from the mean declination derived from the whole of the observations in the five years .
The + and signs in this column attest in as striking a manner as do those at Kew , the existence at Hobarton of a semiannual inequality of which the epochs coincide , or very nearly so , with the sun 's passage of the equator : the direction of the deflection is the same as at Kew , viz. , of the north end of the magnet 626 [ June 18 , 1863 .
] towards the east when the sun is north of the equator , and to the west when he is south of the equator .
The amount of the deflection in the first-named semiannual period is , on the average , 19"'1 in each week ; and in the opposite semiannual period 19 " ; making together an annual variation of 38 " ' 1 .
The author then refers to the result of a similar investigation of the phenomena at St. Helena in the equatorial zone , the particulars of which have been already published in the 2nd volume of the St. Helena Observations .
The result , derived from eight years of observation , of which five years were hourly , evidences at that station also the existence of a semiannual inequality with epochs coinciding , or nearly so , with the equinoxes the deflections being also in the same directions as those at Kew and Hobarton , viz. , to the east when the sun is north , and to the west when he is south , of the equator .
The amount of the annual variation thus produced is less at St. Helena than at either Kew or Iobarton the semiannual difference being about 7 ' ?
, and the annual variation 14 " .
The author remarks that the difference in the amount of deflection at the three stations may , in part at least , be occasioned by the difference in amount of the antagonistic force of the earth 's magnetism , tending to retain the magnet in its mean position in opposition to all disturbing causes .
The antagonistic force , viz. the horizontal component of the earth 's magnetic force , is approximately 5'6 ( in British units ) at St. Helena , 4*5 at Hobarton , and 3'8 at Kew .
In a note appended subsequently to the delivery of this paper , viz. on June 19 , 1863 , the author refers to a similar investigation of the phenomena at the Cape of Good Hope , published in 1851 , in the 1st volume of the magnetical observations at that station .
The volume contains the fortnightly means of the declination from July 1842 to July 1846 , corrected for secular change , and collected in Table III .
, page v , of that volume .
The differences of the declination in each fortnight , so corrected , from the mean declination of the whole period , are shown in its final column .
The mean of the thirteen fortnights ( in the four years ) between March 26 and Sept. 23 , is 0'4 more easterly , and of the thirteen fortnights between September 24 and March 25 , 0'4 more westerly than the mean value-showing an annual variation of 0'8 ( or 48 " ) , or a semiannual inequality averaging 24 " to the east in the thirteen fortnights from March 26 627 to Sept. 23 , and 24 " to the west in the thirteen fortnights from Sept. 24 to March 25 .
This is in accordance with the conclusions at all the other stations at which the phenomena have been subjected to a suitable investigation .
The antagonistic horizontal component of the earth 's magnetism is approximately 4'5 .
Eighth Section .
In the eighth section the author examines the evidence which the monthly determinations of the dip and of the horizontal component of the magnetic force at Kew afford of the existence of a semiannual inequality in the absolute values of the dip and of the total magnetic force .
The results of the monthly determinations from April 1857 to March 1863 are exhibited in two Tables , one appropriated to the dip , and the other to the horizontal force .
The whole series of the determinations of the horizontal force were made with the same unifilar magnetometer and the same collimator magnet throughout , and also by the same observer , Mr. Chambers , one of the assistants at the Kew Observatory .
In the monthly determinations of the dip from April 1857 to September 1860 , twelve different circles , and their twenty-four needles were occasionally employed , the mean of all the observations in each month being taken as the mean result in that month .
There were also several observers in this part of the series , chiefly four .
In the months from October 1860 to March 1863 , one circle with its two needles were the sole instruments , and Mr. Chambers the sole observer .
The probable error of a single monthly determination of the dip in the first part of the series , when several instruments and several observers were employed , is stated to be + 01"69 ; and in the second part of the series , obtained by a single circle and the same observer throughout , the probable error is + 0 ' 75 ; whence it is inferred that the greater number of partial results which contributed to produce the monthly mean in the earlier period more than counterbalanced the diversities which might have been occasioned by the peculiarities of the different observers and of the different instruments .
The probable error of a single monthly determination of the dip , after the application of the corrections for secular change and annual variation , is stated to be + 0'.71 , and of a single monthly determination of the horizontal force derived from the 72 monthly determinations + '0024 .
The results of the monthly determinations at Kew , as bearing 628 upon the question of annual variation , may be briefly stated as follows:-1st .
The dip is subject to an annual variation , which , on the average of the six years , amounts to 1'35 ; consisting of a semiannual inequality with epochs coinciding , or very nearly so , with the equinoxes ; the mean dip being on the average 0'"65 lower than its annual mean value in the six months from April to September , and 0'`7 higher than its annual mean value in the six months from October to March .
2nd .
That the horizontal force is subject to a semiannual inequality having the same epochs-being on the average *0013 higher than its annual mean in each of the six months from April to September , and '0013 lower than its annual mean in each of the months from October to March .
3rd .
That , combining the results of the dip and horizontal force , the total terrestrial magnetic force is expressed in British units by 10'3002 as its mean value in the months from April to September , and by 10'30347 in the months from October to March , -there being thus a difference of 00327 , by which the intensity of the magnetic force of the earth is greater in the months when the sun is south of the equator than in the months when he is north of the equator .
This conclusion is compared with the results obtained in a corresponding manner from the published observations of the Hobarton Observatory , viz. , with the monthly determinations of the horizontal force in the five years from January 1846 to December 1850 inclusive , and with those of the dip in the ten years from January 1841 to December 1850 inclusive .
From these data the conclusions are drawn , 1st , that at Hobarton the dip is subject to an annual variation amounting to 1'18 , consisting of a semiannual inequality with epochs coinciding or nearly so with the equinoxes the ( south ) dip being on the average 0'"59 less in the months from April to September , and 0'"59 greater in the months from October to March than the mean annual value ; and 2nd , that the horizontal force is subject to a similar semiannual inequality , being '0007 less than its mean value in the months from April to September , and '0005 greater in the months from October to March ; and combining these two results , that the total force at Hobarton is expressed in British units by 13-56882 in the months from October to March , and by 13'55195 in the months from April to September : the difference , ?
01687 , expresses the measure of the greater intensity of the earth 's magnetic force when the sun is south than when he is north of the equator .
The author concludes this section of his investigations by drawing the attention of the Royal Society to this concurrent evidence , from the observations of three observatories situated in parts of the globe so distant from each other , of a semiannual inequality having such strong features of resemblance in both hemispheres , and remarks that it seems difficult to assign such effects to any other than to a cosmical cause .
The " inequalities " may in themselves seem to be small ; but judged of scientifically , i. e. in the proportions they bear to their respective probable errors , they are large .
|
112324 | 3701662 | Experiments, Made at Watford, on the Vibrations Occasioned by Railway Trains Passing through a Tunnel. [Abstract] | 630 | 633 | 1,862 | 12 | Proceedings of the Royal Society of London | James South | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 4 | 35 | 1,280 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112324 | null | http://www.jstor.org/stable/112324 | null | 112,000 | Biography | 19.515325 | Astronomy | 16.324937 | Biography | [
36.12659454345703,
11.471528053283691
] | IV .
" Experiments , made at Watford , on the Vibrations occasioned by Railway Trains passing through a Tunnel .
" By Sir JAMES SOUTH , LL. D. , F.R.S. , Member of the Board of Visitors of the Royal Observatory , Greenwich .
Received June 17 , 1863 .
( Abstract .
) These experiments were made in consequence of an attempt in 1846 to run a line of railway through Greenwich Park , in what seemed to several competent judges a dangerous proximity to the Royal Observatory .
It was abandoned , but ( as Sir James South was informed ) only for a time ; and he thought it right to make some examination of the probable effects of such a vicinity , especially as to the power of a tunnel in deadening the vibrations .
The Watford tunnel was chosen as the observing station , being , on the high authority of the late Mr. Warburton , in ground very analogous to that on which the Royal Observatory stands ; and every facility for making observations was afforded by the late Earl of Essex , through whose park and preserves this tunnel passes .
As the chief inconvenience to be feared from the proposed railway was the disturbance of the observations by reflexion in mercury , it seemed best to take a series of these under circumstances as nearly as possible resembling those which might be expected at Greenwich .
An Observatory was therefore erected , in which a large and powerful [ June 18 , 630 transit-instrument was mounted , with all the attention to stability that could be given in a first-class Observatory ; and it had sufficient azimuthal motion to enable the observer to follow the Pole-star in its whole course ; so that night or day ( if clear ) , he could have the reflected image of the star in the mercurial vessel , ready to testify against the tremors caused by any train .
The distance of the vessel from the nearest part of the tunnel was 302 yards , that proposed for Greenwich belng 286 yards .
The length of the tunnel is 1812 yards ; its southern or London end is 643 yards from where the mercury was placed , its northern or Tring end 1281 yards ; and about 64 feet of chalk and gravel lie above the brickwork of its crown .
The author 's preparations were not complete till December 1846 , and then a continuance of cloudy weather interfered with observation till January the 11th , 1847 , when and on the following nights he obtained results so decisive that he felt it his duty to communicate them at once to the then First Lord of the Admiralty , the late Lord Auckland , who was so satisfied with them , that in a letter to Sir James , dated " Admiralty , Jan. 26 , 1847 , " he recorded the impression they had made on his mind in the following words:-- " They would be quite conclusive if the question of carrying a tunnel through Greenwich Park were again to be agitated .
" Sir James , however , continued the work to the end of March .
With the ordinary disturbance to which an Observatory is liable ( as wind , carriages , or persons moving near it ) , the reflected image of a star breaks up into a line of stars , perpendicular to the longest side of the mercury-vessel .
With increased agitation , another line of stars perpendicular to the first appears , making a cross .
With still more the cross becomes a series of parallel lines of stars ; still more makes the images oscillate ; and at last all becomes a confused mass of nebulous light .
The first of these ( the line ) is not injurious to onec lass of observations ; but the others are , and therefore the second ( the cross ) was taken as a measure of the beginning and end of injurious disturbance .
Signal shots were fired when a train passed the southern entrance of the tunnel , and a shaft 1162 yards from it .
Hence the train 's velocity was obtained , and thence its position at any given time .
Upwards of 230 observations are given in detail , and their most important results are shown in a Table , which contains the date , the 22 1863 .
] 631 distances at which the cross of stars begins and ceases to be visible , those at which the series of parallel lines is seen , the velocity in miles per hour , the weight of each engine , and also the length and weight of each train ( when it could be identified ) .
This Table proves that in all cases but one ( which in fact is scarcely an exception ) there is sufficient vibration to excite the cross at 670 yards , and that in 24 per cent. of the number it is seen beyond 1000 , its maximum being 1176 .
At the southern end such distances reach far beyond the tunnel , while at the north they fall within it .
From comparing them in the two cases , the author infers that the train 's agitation extends laterally as far when it is in the tunnel as when in the open cutting .
The amount of disturbance does not depend solely on the velocity and weight of the train , but also on other circumstances , of which prolonged action and length of train are the chief .
In one instance , with only a velocity of 11'4 miles , the cross was seen at 1110 yards-a proof that no regulation of the speed in passing an Observatory at a distance of 300 or 400 yards would be of any avail .
The system of parallel lines is only seen between lines making angles of 450 with the perpendicular to the rails , that is , at distances under 427 yards ; it scarcely ever is produced unless the cross be visible beyond 1000 yards .
These forms are also produced by the reports of cannon of twelve ounces calibre , at distances from 300 to 3000 yards ; in the last case there is but a faint trace of the cross .
In all , the appearance is momentary , not lasting in any case more than a second and a half .
They are not produced by the roar of a two-pound rocket fired 82 feet from the mercury , though very loud .
When the cannon were fired in the tunnel , where the perpendicular meets it , two sets of tremors were seen-one , he believes , propagated through the ground , the other through the air about a second later , the sound escaping probably through the shafts .
Attempts were made to substantiate or refute this hypothesis ; but the difficulties of rapidly shifting and unshifting the coverings prepared for the purpose were such as to compel him to relinquish them .
These observations were reduced in 184 7 ; but conceiving all danger to the Royal Observatory was past , the author did not think it necessary then to proceed with them .
As , however , no Observatory 63 can now be considered secure from railway injury , he wishes to make them public , in hopes that they may be useful , not only to practical astronomy , but to some other departments of science .
|
112325 | 3701662 | Preliminary Notice of an Examination of Rubia munjista, the East-Indian Madder, or Munjeet of Commerce | 633 | 639 | 1,862 | 12 | Proceedings of the Royal Society of London | John Stenhouse | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0136 | null | proceedings | 1,860 | 1,850 | 1,800 | 7 | 107 | 2,792 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112325 | 10.1098/rspl.1862.0136 | http://www.jstor.org/stable/112325 | null | null | Chemistry 2 | 85.329439 | Biography | 5.12873 | Chemistry | [
-48.235740661621094,
-49.78407669067383
] | V. " Preliminary Notice of an Examination of Hubia munjista , the East-Indian Madder , or Munjeet of Commerce .
" By JOHN STEN-IOUSE , LL. D. , F.R.S. Received June 18 , 1863 .
It is rather remarkable that while few vegetable substances have been so frequently and carefully examined by some of the most eminent chemists than the root of the Rubia tinctorum , or ordinary madder , the Rubia munjista , or munjeet , which is so extensivel ) cultivated in India and employed as a dye-stuff , has been , comparatively speaking , very much overlooked , never having been subjected , apparently , to anything but a very cursory examination .
Professor Rung , at the close of his very elaborate memoir upon madder , published in 1835 , details a few experiments which he made upon the tinctorial power of munjeet , the constituents of which he regarded as very similar to those of ordinary madder .
Professor Rung stated that munjeet contains twice as much available colouring matter as the best Avignon madder .
This result was so unexpected that the Prussian Society for the Encouragement of Manufactures , to whom Professor Runge 's memoir was originally addressed , referred the matter to three eminent German dyers , Messrs. Dannenberger , B6hm , and Nobiling .
These gentlemen reported , as the result of numerous carefully conducted experiments , that , so far from munjeet being richer in colouring matter than ordinary madder , it contained only half the quantity .
This conclusion has been abundantly confirmed by the experience of my friend Mr. John Thom , of Birkacre , near Chorley , one of the most skilful of the Lancashire printers .
From some incidental notices of munjeet in Persoz and similar writers , and a few experiments which I made some years ago , I was led to suspect that the colouring matters in -munjeet , though similar , are by no means identical with those of ordinary madder , and that probably the alizarine or purpurine of madder would be found to be replaced by some corresponding colouring principle .
This hypothesis I have found to be essentially correct ; for the colouring matter of munjeet , instead of consisting of a mixture of alizarine and purpurine , contains 1863 .
] 633 no alizarine at all , but purpurine and a beautiful orange colouring matter crystallizing in golden scales , to which I purpose giving the name of " munjistine .
" Munjistine exists in munjeet in considerable quantity , and can therefore be easily obtained .
The colouring matter of munjeet may be extracted in various ways ; that which I have found most suitable is as follows:-each pound of munjeet in fine powder is boiled for four or five hours with two pounds of sulphate of alumina and about sixteen of water .
The whole of the colouring matter is not extracted by a single treatment with sulphate of alumina ; the operation must be repeated therefore two or three times .
The red liquid thus obtained is strained through cloth filters while still very hot , and the clear liquor acidulated with hydrochloric acid .
It soon begins to deposit a bright red precipitate , the quantity of which increases on standing , which it should be allowed to do for about twelve hours .
This precipitate is collected on cloth filters and washed with cold water till the greater portion of the acid is removed .
It is then dried , reduced to fine powder , and digested in a suitable extracting apparatus with boiling bisulphide of carbon , which dissolves out the crystallizable colouring principles of the munjeet , and leaves a considerable quantity of dark-coloured resinous matter .
The excess of the bisulphide of carbon having been removed by distillation , the bright red extract , consisting chiefly of a mixture of munjistine and purpurine , is treated repeatedly with moderate quantities of boiling water and filtered .
The munjistine dissolves , forming a clear yellow liquid , while almost the whole of the purpurine remains on the filter .
When this solution is acidulated with hydrochloric or sulphuric acid , the munjistine precipitates in large yellow flocks .
These are collected on a filter and washed slightly with cold water .
The precipitate is then dried by pressure , and dissolved in boiling spirit of wine slightly acidulated with hydrochloric acid to remove any adhering alumina .
As the munjistine does not subside from cold alcoholic solutions , even when they are largely diluted with water , about three-fourths of the spirit are drawn off by distillation , when the munjistine is deposited in large yellow scales .
By two or three crystallizations out of spirit in the way just described the munjistine is rendered perfectly pure .
I have likewise succeeded in extracting munjistine directly from munjeet by boiling it with water , filtering the solution , which has a dark brownish-red colour , and then acidulating with hydrochloric [ June 18 , 634 acid .
The precipitate which falls is collected on a filter , washed , dried , and treated with boiling spirit of wine , which leaves a large quantity of pectine undissolved .
The munjistine which dissolves in the alcohol is obtained in a pure state by repeated crystallizations in the way already indicated .
The first process which I have described is , however , by far the best .
The colouring matter of munjeet can likewise be extracted with boiling solutions of alum ; but I find sulphate of alumina greatly preferable , as the alum , by its tendency to crystallize , very much impedes the filtration of the liquids .
I likewise attempted to employ Professor E. Kopp 's process with sulphurous acid , which gives such excellent results with ordinary madder , but I found it wholly inapplicable to munjeet .
Munjistine , prepared by the processes described , when crystallized out of alcohol , forms golden-yellow plates of great brilliancy .
It is but moderately soluble in cold , but dissolves pretty readily in boiling water , forming a bright yellow solution , from which it is deposited in flocks when the liquid cools .
Saturated solutions almost gelatinize .
It dissolves to some extent in cold , but more readily in boiling spirit of wine , and is not precipitated by the addition of water .
It dissolves in carbonate of soda with a bright red colour .
In ammonia it forms a red solution with a slight tinge of brown : caustic soda produces with it a rich crimson colour .
Both its aqueous and alcoholic solutions , when boiled with alumina , form beautiful flakes of a bright orange colour , almost the whole of the munjistine being withdrawn from solution .
These flakes are soluble in a large excess of caustic soda , with a fine crimson colour .
Munjistine dyes cloth mordanted with alumina a bright orange .
With iron mordant it yields a brownish-purple colour , and with Turkey-red mordant a pleasing deep orange .
These colours are moderately permanent , and bear the application of bran and soap tolerably well .
The munjistine sensibly modifies the colours produced by munjeet , giving the reds a shade of scarlet , as has been long observed .
Commercial nitric acid dissolves munjistine with a yellow colour , but does not appear to decompose it even on boiling .
Fuming nitric acid ( 1'5 ) dissolves munjistine in the cold , and on application of heat decomposes it , no oxalic acid being produced .
It readily dissolves in cold sulphuric acid with a bright orange colour ; and the solution may be heated nearly to boiling without blackening or 635 1863 .
] giving off sulphurous acid ; it is reprecipitated by water in yellow flocks apparently unaltered .
When bromine water is added to a strong aqueous solution of munjistine , a pale-coloured flocculent precipitate is immediately produced ; this , when collected on a filter , washed and dissolved in hot spirit , furnishes minute tufts of crystals , evidently a substitution product .
I may remark , in passing , that when alizarine is treated with bromine water in a similar way , it also forms a substitution product crystallizing in needles .
I am at present engaged in the examination of both these compounds .
When munjistine is strongly heated on platinum foil , it readily inflames and leaves no residue ; when it is carefully heated in a tube , it fuses , and crystallizes again on cooling .
It sublimes more readily than either purpurine or alizarine , forming golden scales which consist apparently of unaltered munjistine , as they give the characteristic rich crimson coloration with caustic alkalies .
Baryta water produces a yellow precipitate with munjistine .
Acetate of lead throws down a bright crimson precipitate , both in its aqueous and alcoholic solutions .
I expect , from this and the bromine substitution compound , very shortly to ascertain the atomic weight of this body ; in the mean time I submit the results of its ultimate analysis .
I. '314 grm. of munjistine yielded *732 grm. of carbonic acid and '106 grm. of water .
II .
*228 grm. munjistine yielded *535 grm. carbonic acid and ?
0765 grm. water. .
IH .
C per cent. 63'6 64-0 H , , 3-77 3-73 O , , 32-63 32-27 100-00 100'00 The munjistine operated upon in each case was prepared at different times ; moreover No. 1 was burnt with oxide of copper , No. 2 with chromate of lead .
Munjistine in some of its properties bears considerable resemblance to Runge 's madder-orange , the " rubiacine " of Dr. Schunck : it is , however , essentially different from rubiacine , both in several of its properties , such as its solubility in water and alcohol , &c. , and in the amount of its carbon-rubiacine , according to Dr. Schunck 's analysis , 636 containing 67'01 per cent. of that element , while munjistine contains only 64 .
The spectra afforded by solutions of the two substances , as may be seen from the following extract from a letter received from Professor Stokes , are decidedly different .
" The two substances are perfectly distinguished by the very different colour of their solution in carbonate of soda , when a small quantity only of substance is used .
The solution of munjistine is red inclining to pinkish orange , that of rubiacine a claret-red .
The tints are totally different , and indicate a different mode of absorption .
Both present a single minimum in the spectrum ; but while that of rubiacine extends from about D to F , that of munjistine extends from a good way beyond D to some way beyond F. The beginning and end of the band in each case is not very definite , and varies of course with the strength of the solution ; but by comparing the substances with different strengths of solution , there can be no doubt of the radical difference in the position of the band of absorption .
In this way it is easy to convince oneself that the difference of colour is not to be explained by the possible admixture of some small imn purity present in one or other specimen .
With caustic potash munjistine gives as nearly as possible the same colour as rubiacine , agreeing with the colour of rubiacine in carbonate of soda .
'There appears to be a slight difference in the spectrum of the munjistine and rubiacine solutions , but not enough to rely on ; so that the substances are not to be distinguished by their solutions in caustic alkalies .
" A second perfectly valid distinction is , however , afforded by the different colour of the fluorescent light of the ethereal solutions .
The solid substances themselves and their ethereal solutions are fluorescent to a considerable degree ; but the tint of the fluorescent light of the ethereal solution of rubiacine is orange-yellow , while that of the ethereal solution of munjistine is yellow inclining to green .
The examination in a pure spectrum shows that the difference is not due to the admixture of a small impurity , itself yielding a fluorescent solution ; but the tints may be readily contrasted by daylight , almost without apparatus , by the method I have described in a paper 'On the existence of a second crystallizable fluorescent substance in the bark of the horse-chestnut ' ( Quart .
Journal Chem. Soc. vol. ii .
p. 20 ) .
I consider either of the two points of difference I 1863 .
] 637 have mentioned sufficient by itself to establish the non-identity of munjistine and rubiacine " " .
The purpurine which I succeeded in extracting from munjeet and in purifying from munjistine in the way already described , formed beautiful dark crimson needles , having all the usual properties of that substance .
When examined by Professor Stokes , they gave the very characteristic spectra of purpurine .
*3285 grm. of purpurine gave '8005 grm. carbonic acid and ?
1050 grm. water .
Analysis .
Theory .
Found .
Debus ( mean ) .
C ... ... . .
6667 66-46 66-40 ... ... . .
3-70 3-55 3'86 ... ... . .
2963 29'99 29-74 100-00 100-00 100-00 From the results above detailed there can therefore be no doubt that the colouring matter of munjeet , as already stated , consists of purpurine and munjistine .
I cannot conclude this preliminary notice without acknowledging the essential services I have received from Professor Stokes , who kindly submitted the different products obtained by me to optical examination .
Though it is plain that a substance optically pure , that is , containing no impurities affecting the spectrum , may still be far from being chemically so , yet the spectroscope is extremely useful in indicating admixtures of kindred substances of very similar properties , having a great affinity for each other , and therefore not readily separable .
I feel certain therefore that if Professor Stokes would draw up a short treatise embodying his extensive and accurate observations on the spectra of the colouring matters and similar substances , he would confer a great boon on the cultivators of organic chemistry .
PosTscRIPT.-Received July 18 , 1863 .
Since the preceding paper was communicated to the Royal Society I have been enabled to examine the action of nitric acid on munjis* I may mention that the rubiacine which Professor Stokes examined was prepared by Dr. Schunck himself .
[ June 18 , 638 time much more fully .
When munjistine is digested with moderately strong nitric acid , as already stated , copious fumes are given off , the munjistine gradually dissolving and forming a colourless solution .
When this is evaporated to dryness on the water-bath , a white crystalline mass is obtained , consisting almost entirely of phthalic acid contaminated with a small quantity only of oxalic acid .
The oxalic acid may be easily removed by washing the mass with a little cold water and then pressing between folds of bibulous paper , or by neutralizing the mixture of the two acids with lime and then treating with boiling water , which dissolves the phthalate of lime .
The acid freed from oxalic acid by either of these methods presents all the usual reactions of phthalic acid .
One of the most convenient ways of purifying it consists in subliming it repeatedly in a Mohr 's apparatus , when the anhydrous acid is obtained in beautifully white iridescent four-sided prisms , frequently several inches in length . ?
3745 grin .
of the crystals of the anhydride , burnt with chromate of lead , gave *891 grm. carbonic acid and *095 grm. of water .
Theory .
Expt. Marignac .
Laurent .
C1 ... ..96 64-86 64-89 64-88 64-70 11 ... 4 2-70 2-81 2-71 2-38 06 ... .48 32-44 32-30 32-41 32-92 From this result it is evident that the acid chiefly produced by the action of nitric acid upon munjistine is phthalic acid , which , as is well known , may also be procured from alizarine and purpurine .
This reaction , therefore , indicates a very close relationship between these three substances , the only true colouring principles of madder with which we are at present acquainted .
|
112326 | 3701662 | Notes of Researches on the Poly-Ammonias.--No. XXIV. On Isomeric Diamines | 639 | 645 | 1,862 | 12 | Proceedings of the Royal Society of London | A. W. Hofmann | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0137 | null | proceedings | 1,860 | 1,850 | 1,800 | 7 | 89 | 1,959 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112326 | 10.1098/rspl.1862.0137 | http://www.jstor.org/stable/112326 | null | null | Chemistry 2 | 97.201256 | Astronomy | 2.04049 | Chemistry | [
-45.8376350402832,
-62.070526123046875
] | VI .
" Notes of Researches on the Poly-Ammonias.-No .
XXIV .
On Isomeric Diainines .
" ByA .
W. HOrMANN , LL. D. , F.R.S. Received May 26 , 1863 .
In a former paper* I have described phenylene-diamine , an aromatic diamine which is formed by the action of powerful reducing agents upon dinitrobenzol .
Phenylene-diamine , the last product of this reaction , is preceded by the formation of an intermediate compound , nitraniline , a substance discovered many years ago by Dr. Muspratt and myself , C6 116 C H4NO 64 NO2 C6 NHi2 NO,2 N , NH2 , .
Benzol .
Dinitrobenzol .
Nitraniline .
Phenylene-diamine .
Nitraniline , as might have been expected , was found to be readily convertible into phenylene-diamine .
By the researches of M. Arppet , chemists have become acquainted with a second nitraniline , which is obtained by the action of fuming nitric acid upon phenyl-pyrotartramide and subsequent treatment of the nitro-compound with potassa .
This substance , which , as I afterwards found , may be more readily prepared by a similar treatment of other less difficultly obtainable phenylamides , such as phenylacetamide or phenyl-succinamide , is isomeric with ordinary nitraniline , but differs from the latter compound both in its physical and chemical properties , so as to leave no doubt regarding the individuality of the two compounds , which have accordingly been distinguished as alpha-nitraniline and beta-nitraniline .
This singular isomerism , which has been traced also in other phenyl-derivatives , remains unexplainedl .
Whilst engaged with the examination of phenylenedic.time , the idea naturally suggested itself , to ascertain whether beta-nitraniline , when submitted to reducing agents , would yield a body isomeric but differing from the phenylene-diamine obtained from dinitrobenzol and alpha-nitraniline .
Beta-nitraniline is readily reduced by a mixture of iron and acetic * Chem. Soc. AMem .
vol. iii .
p. 112 .
t Chem. Soc. Journ. vol. viii .
p. 175 .
+ Among the various attempts I have made to decipher this isomerism , I may mention the treatment of the two nitranilines with the iodides of methyl and ethyl .
But these substances are not acted upon by the reagents in question , and I take this opportunity of correcting an error which has crept into my paper on the molecular constitution of the volatile organic bases ( Phil. Trans. 1850 , vol. i. p. 93 ) .
In this paper I state that the action of iodide of ethyl on nitraniline gives rise to the formation of hydriodate of ethyl-nitraniline .
This statement is based upon a single platinum determination .
The platinum-salt of nitraniline contains 28'66 per cent. of platinum , that of ethyl-nitraniline 26-53 per cent. Analysis had furnished me 26'23 per cent. I have since satisfied myself that the salt was the imperfectly purified platinum-salt of nitraniline .
640 [ June 18 , acid .
The basic compound which distils over has the same compo .
sition as phenylene-diamine , viz. C6 H8 N2 , and presents in its properties many analogies with this substance , but it is far from being identical with it .
The two diatomic bases obviously are related to each other in the same manner as the two nitranilines from which they are derived , and I propose therefore to distinguish them as alpha-phenylene-diamine and beta-phenylene-diamine .
Beta-phenylene-diamine differs from alpha-phenylene-diamine by its superior crystallizing power : whilst the latter for days and often for weeks remains liquid , the former immediately , when separated from one of its salts by an alkali , solidifies into a beautifully crystalline mass .
The fusing-point of alpha-phenylene-diamine is 63 ?
( corr .
) , that of betaphenylene-diamine is 140 ?
( corr .
) ; the former boils at 287 ?
( corr .
) , the latter at 267 ?
( corr .
) .
Beta-phenylene-diamine is remarkable for the facility with which it sublimes even at temperatures below its boiling-point .
The experiment succeeds particularly well in a current of hydrogen gas , when the base is obtained in splendid crystalline plates resembling pyrogallic acid .
The salts of beta-phenylene-diamine , although they are more soluble than the corresponding alpha-phenylene-diamine salts , are distinguished by the same superior crystallizing power .
They are all remarkable for the facility with which they yield beautiful and mostly well-formed crystals .
I have examined only two of these salts somewhat more minutely .
Hydrochlorate of Beta-phenylene-diamine.-This salt crystallizes in large prisms , which are at present in the hands of M. Quintino Sella .
Extremely soluble in water , difficultly soluble in hydrochloric acid , it contains C H8 N2 , 2I-C1 .
Hydrobromate of beta-phenylene-diamine resembles in every respect the hydrochlorate .
The crystals , which were found to have the formula C6 II8 N2 , 2 IBr , are apt to assume a reddish tint when left in contact with the air .
Platinum-salt.-Light-yellow plates extremely soluble in water and readily decomposed by heat .
Composition : C6 8 N2 , , 2 HC1 , 2 Pt C1 .
s1863 .
] 641 The sulphate and nitrate are easily crystallizable salts , somewhat less soluble in water than the hydrochlorate .
Beta-phenylene-diamine and its salts are remarkable for the facility with which they are converted into violetand blue-coloured compounds under the influence of oxidizing agents such as chlorine , bromine , chromic acid , ferric and platinic chloride , &c. Both alphaand beta-phenylenediamine are readily attacked by the iodides of the alcohol radicals ; and a means was thus afforded of ascertaining whether both substances exhibit the same degree of substitution .
Since only the last products of substitution presented any interest , I have submitted the two bases to methylation .
This experiment showed that both alphaand beta-phenylene-diamine are capable of absorbing six equivalents of methyl to produce ammonium compounds of perfect substitution , and that both bases must therefore be represented by the formula C6 Hl4 -I2 > N2 .
In the case of both bases , alternate treatment with iodide of methyl and oxide of silver or distillation with soda , thrice repeated , leads to the formation of a well-crystallized iodide of the formula C H~ NI =-(Co 11 ) N 0121222 =2 L(C I'i ) }N ] IJ2 Whether prepared from alphaor from beta-phenylene-diamine , this salt crystallizes in plates extremely soluble in water , less so in alcohol .
I have found no other difference except that the betaphenylene-compound is more soluble than the derivative of the alpha-base .
Whilst studying the methylated derivatives of the two bases , I have , of course , repeatedly obtained the lower , still volatile bases , which on this occasion were submitted to a few experiments .
The compound C 1H6 N2 ( C6 Hl ) } N , procured from beta-phenylene-diamine , when submitted to the action of iodide of methyl , was found to produce , in the first place , a rather difficultly soluble iodide , Cn0 Hin N2 I ( C I-I)4 N , CH3 I2 ( C I1)4J 2 ' 3 before it was converted into the final product C( H2 N I= ( C H4 ) N2 , 2CH I ( C61 4)l N2 I 2112,21 ( c 113)4 N,11 CL( 113 ) 6 ) The pentamethylated iodide , when treated with hydriodic acid instead of iodide of methyl , furnished the di-iodide of pentamethylphenylenediammonium , ( HI 114 ) ' C11 H20 N2 I2= [ ( C I , ) , H3 N2 12 The two phenylene-diamines are thus seen not only to be isomeric , but to have actually the same degree of substitution , as far as the latter may be rendered transparent by the action of iodide of methyl .
Under these circumstances I was pleased to observe some additional phenomena which removed every doubt regarding their individuality .
On mixing a solution of beta-phenylene-diamine in sulphuric acid with peroxide of manganese , the odour of kinone becomes at once perceptible , and on heating the mixture , kinone distils overthe residuary liquid containing the sulphates of manganese and ammonium , C , H,1 N+ 2H2 , S04 M+ Mn2 S0 , = 4 ( H4 N)2 SO , .
Beta-phenyKinone .
lene-diamine .
The reaction proceeds with such ease that a few milligrammes of the diamine , when submitted to this treatment in the test-tube , yield a distinct crystalline sublimate of kinone , readily recognizable by its many salient properties .
Alpha-phenylene-diamine , when similarly treated , evolves a faint odour of kinone , but does not yield crystals of this substance .
The elegant and easy formation of kinone in this reaction presents some interest , inasmuch as the process appears to be of general application , and will probably lead to the preparation of the higher homologues of kinone .
I have observed the formation of beta-phenylene-diamine in two additional reactions , which , in conclusion , I beg leave to mention .
In the hopes of obtaining the triamine of the phenyl-series ( C HT , ) " ' " C6 It N=H N , It3 1863 .
] 643 I submitted dinitrophenylamine , [ C6 H3 ( NO2)2 ] C6 H1N304O H SN , HJ to distillation with iron and acetic acid , but , instead of the compound which I endeavoured to procure , I invariably obtained beta-phenylenediamine and ammonia , CH 9N3 + H2 = C6 H , N , + HN .
Phenylic triaBeta-phenylenemine .
diamnine .
Again , dinitrazobenzol , C , H , N , O=C N(NO , , when submitted to the action of powerful reducing agents , yields likewise beta-phenylene-diamine CH12 1 N4 04 , +8H2=4H20+2C,6 HN2 .
Dinitrazobenzol .
Beta-phenylenediamine .
I-ere also beta-phenylene-diamine is the final product of the , reaction , the formation of which is preceded by that of another base , the diphenine of Messrs. Gerhardt and Laurent .
Diphenine , according to these chemists , is C12 H N , , a formula chiefly supported by the unequivocal presence of C12 in the molecule of azobenzol , C , 1 HI N2 , whence it derives .
The facility , however , with which diphenine under the influence of nascent hydrogen , by treatment with sulphuric acid and zinc , for instance , is converted into beta-phenylene-diamine renders it probable that the molecule of diphenine is C H116 N , when the two bases become related to each other as kinone and hydrokinone , Kinone ... ... C6 , 02 Diphenine ... ... ... .
N2 H-Iydrokinone. .
CG HI 02 Beta-phenylene-diamine C6 HI N2 .
I have hitherto vainly tried to transform kinone into diphenine or beta-phenylene-diamine ; but it deserves to be noticed that M. Woskresensky , by treating kinone with ammonia , has obtained a green * Woskresensky , Journ. Pract .
Chem. vol. xxxiv .
p. 251 .
644 [ June 18 , beautifully crystalline mass , kinonamide , C6 H5 NO , which stands midway between kinone and diphenine , C6 H4 02+H , N=C , H5 NO+H2 O. Kinone .
Kinonamide .
Another similar step of transformation would lead to diphenine , C6 H5 NO+H3 N=C6 I , N2+H2 O. Kinonamide .
Diphenine .
The preparation of azobenzol in large quantity , its transformation into dinitrazobenzol , and , lastly , the conversion by means of sulphide of potassium of the nitro-compound into diphenine , present so little difficulty , that treatment of diphenine with nascent hydrogen affords the easiest and simplest means of procuring beta-phenylene-diamine in appreciable quantity .
|
112327 | 3701662 | Contributions towards the History of the Colouring Matters Derived from Aniline | 645 | 647 | 1,862 | 12 | Proceedings of the Royal Society of London | A. W. Hofmann | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0138 | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 35 | 750 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112327 | 10.1098/rspl.1862.0138 | http://www.jstor.org/stable/112327 | null | null | Chemistry 2 | 82.712218 | Biography | 16.910893 | Chemistry | [
-46.211788177490234,
-58.42732238769531
] | VII .
" Contributions towards the History of the Colouring Matters derived from Aniline .
" By A. W. HOFMANN , LL. D. , F.R.S. Received June 2 , 1863 .
In a short paper recently submitted to the Royal Society , I pointed out the existence of two aromatic diamines , both represented by the formula ( C , H4 ) " C , HN = H2 N , and closely resembling each other , but differing in some of their fundamental characters to such an extent that I did not hesitate to assert their individuality , and to distinguish them as alpha-phenylene-diamine and beta-phenylene-diamine .
The existence of two closely allied bodies among the diatomic derivatives of the phenyl-series very naturally suggested the idea of searching for two similarly related monatomic bases of the same group , and accordingly I undertook during the last week a careful comparison of specimens of aniline prepared by different processes .
This comparative study is still incomplete , but I beg leave to record even now an observation which appears to merit the attention of chemists .
I have , in the first place , examined aniline obtained by distillation of isatin ( indigo ) with hydrate of potassium .
The base prepared in this manner boils at 182 ?
, and possesses the general characters attributed to aniline .
But neither by treatment with mercuric or stannic chloride nor with arsenic acid is this substance converted into aniline-red .
Aniline derived from benzol was next submitted to examination .
The benzol employed for the preparation of the base was partly obtained by the distillation of benzoic acid with lime , partly by the fractional distillation of coal-tar naphtha , and the ultimate solidification of the product , boiling between 80 ?
and 83 ? .
Both varieties of benzol were treated with fuming nitric acid , and the nitro-compound thus obtained converted into aniline by means of iron and acetic acid .
The base prepared from benzoic benzol boils at 182 ? .
Like indigo-derived aniline , it refuses to yield the red colour by treatment with the agents previously mentioned .
Aniline obtained from coal-tar benzol , as might have been expected , likewise boils at 182 ?
, and neither mercuric nor stannic chloride nor arsenic acid converts this substance into aniline-red .
When I communicated these observations to my friend Mr. E. C. Nicholson , I found that in this case , as in so many others , practice is far in advance of theory .
The facts which I have mentioned had been long known to this distinguished manufacturer , who in reply to my note transmitted to me a gallon of absolutely pure aniline boiling at 182 ?
, prepared from coal-tar benzol , and perfectly incapable of yielding aniline-red .
During the last few months I have had occasion to examine a great variety of commercial specimens of aniline , more especially samples which had been kindly supplied to me by Messrs. Simpson , Maule , and Nicholson , of London , and by Messrs. Renard Brothers and Franc , of Lyons .
All these specimens furnished , by the ordinary processes , very notable quantities of aniline-red , but they also invariably boiled at a higher temperature , exhibiting in fact boiling-points varying between 182 ?
and 220 ? .
It is thus obvious that commercial aniline contains a base different from normal aniline , the cooperation of which is indispensable for the production of aniline-red .
Is this base an isomeric variety of aniline , an aniline holding to the normal aniline a relation somewhat similar to that whicn obtains between alphaand beta-phenylene-diamine ?
It is well known * Phil. Mag. S. 4 .
vol. xiii .
p. 415 ( June 1857 ) .
that Mr. Church has separated from coal-tar naphtha a hydrocarbon isomeric with benzol , parabenzol , which boils at 97 ?
'5 .
This substance is readily converted into a nitro-compound , and ultimately into the corresponding base .
Is it the base thus formed which gives rise to the formation of aniline-red ?
Or is it not more probable that commercial aniline contains another base analogous or homologous with aniline which is involved in the generation of the red ?
These are questions equally interesting for theory and practice , and the solution of which will probably throw considerable light upon the still enigmatical genesis of rosaniline .
|
112328 | 3701662 | Contributions towards the History of the Colouring Matters Derived from Coal-Tar | 647 | 648 | 1,862 | 12 | Proceedings of the Royal Society of London | A. W. Hofmann | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0139 | null | proceedings | 1,860 | 1,850 | 1,800 | 2 | 20 | 517 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112328 | 10.1098/rspl.1862.0139 | http://www.jstor.org/stable/112328 | null | null | Chemistry 2 | 78.229167 | Biography | 11.865519 | Chemistry | [
-46.205078125,
-58.329673767089844
] | VIII .
" Contributions towards the History of the Colouring Matters derived from Coal-tar .
" By A. W. HOFMANN , LL. D. , F.R.S. Received June 9 , 1863 .
In a previous Note I have shown that the red colouring matter cannot be obtained from normal aniline by the action of the agents usually employed for the preparation of this colour on a large scale .
This observation naturally induced me to seek for the constituent in the commercial aniline which gives rise to the formation of aniline-red .
I have already remarked that the commercial product which is best suited for the manufacture of the red colour , boils at a temperature appreciably higher than the boiling-point of normal aniline .
The idea presented itself of submitting this substance to a fractional distillation , or else of effecting a methodical separation of the hydrocarbons which constitute the starting-point for the manufacture of the bases ; but , as is well known , these processes are difficult and tedious , and there is little chance of success unless the operation be performed on a very large scale .
In the hope of accelerating the inquiry , I examined the action of mercuric and stannic chlorides upon the homologues of aniline , of which I fortunately possessed some pure specimens .
The contiguous term toluidine was the first to fix my attention .
The presence of this base in commercial aniline could not be doubted , since the benzol employed in the manufacture of this substance almost invariably boils at temperatures between 80 ?
and 100 ?
, or even higher .
Indeed Mr. Nicholson having convinced himself that pure aniline is not 2z2 647 available for the preparation of rosaniline , was at one time disposed to consider toluidine the true source of the so-called aniline-red .
But toluidine the purity of which was established by combustion when submitted under the most varied circumstances to the action of the agents already mentioned , does not produce a trace of colouring matter .
The subject , which thus appeared to become more and more obscure , was elucidated by a happy experiment .
A mnixture of pure aniline and pure toluidine , when heated with mercuric chloride , stannic chloride , or with arsenic acid , instantaneously produced a magnificent red of most intense tinctorial power .
This experiment appears to show that the red belongs to both the phenic and toluic series .
I have not as yet pursued my researches further in the new field opelled by this experiment .
In conclusion I may be allowed to state that by transforming into oxalate commercial aniline , and especially a specimen of aniline which was furnished to me by Mr. Nicholson as particularly well adapted for the preparation of the red , I have been enabled to obtain considerable quantities of toluidine in a state of perfect purity .
Having thus at my disposal the necessary material , I hope soon to acquire further experimental data for the explanation of the formation of rosaniline .
|
112329 | 3701662 | On the Measurement of the Chemical Brightness of Various Portions of the Sun's Disc | 648 | 650 | 1,862 | 12 | Proceedings of the Royal Society of London | Henry Enfield Roscoe | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0140 | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 46 | 800 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112329 | 10.1098/rspl.1862.0140 | http://www.jstor.org/stable/112329 | null | null | Optics | 60.304621 | Astronomy | 32.260386 | Optics | [
10.09792709350586,
-23.209217071533203
] | IX .
" On the Measurement of the Chemical Brightness of various portions of the Sun 's Disc .
" By HENRY ENFIELD RoscoE , B.A. , F.R.S. Received June 12 , 1863 .
The author has applied the method of measurement of the chemical action of sunlight , which Professor Bunsen and he described in a memoir presented to the Royal Society in November last* , to the measurement of the chemical brightness of various portions of the solar disc ; and although the observations which have as yet been made are only preliminary , yet he thinks that the results obtained are of sufficient interest to warrant his bringing them before the Society .
Secchi has shownt that the calorific radiation of the centre of the sun 's disc is nearly double that from its borders , and that the equatorial regions are somewhat hotter than the polar , whilst observers have long noticed a great difference in luminosity between the centre and edge of the disc .
For the purpose of obtaining a measurement of the relative chemical brightness of various portions of the solar disc , the image of the sun , of about 4 inches in diameter , obtained by a3 -inch refractor* , was allowed to fall into a camera placed on the instrument , upon a sheet of standard photographic paper prepared according to the method described in the above-mentioned research .
The peculiar property of this standard paper is that it can always be prepared of one and the same degree of sensitiveness , and is perfectly homogeneous .
The exposure lasted for from 30 to 120 seconds , the sun 's motion being carefully followed by a tangent-screw .
After exposure , the shade of tint at several points on the picture was determined by comparison with a graduated photographic strip insolated in the pendulum-photometer , and the chemical intensities corresponding to these shades obtained by reference to the Table given in the memoir above cited .
The following numbers give the chemical brightness , thus obtained , at various points on the sun 's disc on May 9th , 1863 .
From these numbers it is seen that the intensity of ' the chemically active rays at the centre is from three to five times as great as that at the edge of the disc , the chemical rays thus showing a wider variation than the calorific rays exhibited as determined by Secchi .
This is doubtless owing to the relatively greater absorption effected by the solar atmosphere on the more refrangible chemical rays .
Chemical Brightness of Sun 's Disc on May 9 , 1863 .
1 .
At centre of 2 .
At 150 from edge of Sun 's 3 .
At edge of Sun 's Dis Sun 's Disc .
Disc .
N. Pole .
Equator .
S. Pole .
N. Pole .
Equator .
S. Pole .
No. 1 .
100'0 38-8 48-4 58-1 18-7 30'2 28-2 No. 2 .
100-0 52-8 ... ... 56-6 305 ... ... 410 Hence it is likewise seen that on May 9th the chemical brightness of the south polar regions was considerably greater than that of the north polar regions , whilst about the equator the brightness was between that of the poles .
Inr order to show that the sensitive paper , when exposed to ordinary sunlight , becomes homogeneously tinted , the author appends the readings , taken in the way described , from various portions of a piece of the standard paper used for the sun-pictures exposed for some seconds to direct sunlight .
Reading .
Deviation from mean .
Portion No. 1. .
101-4 ... .
+0-93 , , 2. .
1007 ... .
+0-23 3. .
98-5 ... .
-1-97 4 .
101-6 ... .
+113 , , 5 .
, 99.9 ... .
-0-57 , 6 .
100-7 ... .
+0-23 Mean. .
100-47 The sun-pictures obtained on the sensitive paper must possess only a slight tint , otherwise the differences in shade cannot be accurately observed ; they then exhibit a peculiar coarse mottled appearance , which is not due to imperfections in the paper or the lenses , nor to the action of the earth 's atmosphere .
Perhaps these irregular dark and light patches are owing to clouds in the solar atmosphere , and they may have an intimate connexion with the well-known phenomenon of the red prominences .
Mr. Baxendell and the author propose to carry out , according to this method , a regular series of observations of the variation of the relative amounts of brightness on the sun 's disc , and they hope before long to be able to present the Society with some further details .
|
112330 | 3701662 | On the Contractility of Healthy and Paralysed Muscles as Tested by Electricity | 650 | 651 | 1,862 | 12 | Proceedings of the Royal Society of London | Harry Lobb | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0141 | null | proceedings | 1,860 | 1,850 | 1,800 | 2 | 12 | 502 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112330 | 10.1098/rspl.1862.0141 | http://www.jstor.org/stable/112330 | null | null | Nervous System | 48.865982 | Electricity | 30.2932 | Nervous System | [
-62.380184173583984,
-11.252593040466309
] | X. " On the Contractility of Healthy and Paralysed Muscles as tested by Electricity .
" By HARRY LOBB , Esq. Communicated by JOHN SIMrON , Esq. Received April 30 , 1863 .
If a moist conductor from the positive pole of the finer wire of an electro-magnetic battery* be placed upon the skin covering the origin of a healthy muscle , and the moist conductor from the negative pole , upon its belly , and a current of moderate intensity be allowed to pass , the muscle will contract tonically as long as the current passes ; and if it be increased in intensity , cramp will eventually be induced .
The positive pole may be placed upon almost any part of the body to produce this effect ; only as it is removed further from the muscle to be acted on , the intensity of the current must be progressively increased .
A healthy muscle contracts with more vigour if the current be direct-that is to say , the positive pole towards the centre , the negative pole towards the periphery .
If a muscle paralysed from recent injury to the brain be acted upon in the same way , it will be found to contract more vigorously than a healthy one under the same intensity of current .
If an extensor muscle paralysed and wasted , the result of poisoning by lead , be treated in the same way , no contraction can be induced even with the highest power of the apparatus ; the unparalysed flexors will alone contract .
If a muscle paralysed and wasted from loss of nutrition , as in those local paralyses which are the sequelae of fever , the exanthemata , convulsions , irritation during teething , &c. , be acted on in the same way , no contraction can be induced ; if the current is increased in intensity , the healthy or antagonistic muscles contract .
In these two latter instances-after treatment by the continuous galvanic current , when circulation has been re-established , and the paralysed muscles are better nourished-if the current be reversed , the positive pole placed on the insertion of the muscle , and the negative pole on the belly , and if the current is not too strong , faint contraction takes place , gradually increasing until the muscle is sufficiently restored to contract under the direct stimulus .
A singular fact in connexion with these paralysed and wasted muscles is , that they will contract at the will of the patient , for some time , before they will do so to the stimulus of the current ; but the paralysed muscles are not safe from a relapse until they contract vigorously to the ordinary direct electrical stimulus .
At a certain stage of improvement , when the paralysed muscle will neither contract to the will nor to the electro-magnetic current , it will do so to the combinationD of the two .
1863.1 651
|
112331 | 3701662 | On the Influence of Temperature on the Electric Conducting-Power of Alloys. [Abstract] | 652 | 654 | 1,862 | 12 | Proceedings of the Royal Society of London | A. Matthiessen|C. Vogt | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 46 | 1,085 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112331 | null | http://www.jstor.org/stable/112331 | null | 108,867 | Tables | 34.503657 | Measurement | 30.024597 | Tables | [
-6.430154323577881,
-74.15072631835938
] | XI .
( " On the Influence of Temperature on the Electric Conducting-Power of Alloys .
" By A. MATTHIESSEN , F.R.S. , and C. VOGT , Ph. D. Received June 11 , 1863 .
( Abstract .
) The subject of this paper has been divided into four parts , viz.:I .
Experiments on the influence of temperature on the electric conducting-power of alloys composed of two metals .
II .
Experiments on the influence of temperature on the electric conducting-power of some alloys composed of three metals .
III .
On a method by which the conducting-power of a pure metal may be deduced from that of the impure one .
IV .
Miscellaneous and general remarks .
In the first part , after having given the numerical results , we proceed to explain the law which regulates this property .
It is as follows : The observed percentage decrement in the conducting-power of an alloy between 0 ?
and 1000 C. is to that calculated between 0 ?
and 100 ?
C. as the observed conducting-power at 100 ?
C. is to that calculated at 100 ?
C. Or in symbols , Po : Pc : : X 10 : X1X ' , where Po and Pc represent the observed and calculated percentage decrements in the conducting-power of the alloy between 0 ?
and 100 ?
C. ; and X100o and X'l00o its observed and calculated conductingpower at 100 ?
C. , Pc is equal in nearly all cases to 29'307 * , the exceptions being only in the instances of thallium and iron alloyst .
The above law holds good for most of the alloys belonging to the first and third groups , as well as for a part of those belonging to the second group T. Now , if the above proportion , Po : Pc : : X10o:X'..(1 ) P=:00X ... ... ( 1 ) be converted into terms of resistance , the following formula is obtained , 2= loopo-r0oo= 100 ?
-o * .
**** ( 2 ) where r100o0 ro 2100r ' and r'0O represent the observed and calculated resistances at 0 ?
and 100 ?
C. The formula , however , expresses the fact that the absolute dijference between 0 ?
and 100 ?
C. in the resistance of an alloy is equal to the absolute diff'erence between 00 and 100 ?
in the calculated resistance of the alloy .
Formula 2 may also be written r100§ 100 ?
= ?
0o ' which , if correct , leads to the expression r ' : o r0o ; that is , the absolute deference between the observed and calculated resistances of an alloy at any temperature equals the absolute difference between the observed and calculated resistances at 0 ?
C. ; or , in other words , r - ?
r= a constant ... ... .
( 3 ) After giving various examples to show the correctness of the above , we prove that from the expression rtr'= a constant ( 3 ) we may deduce the formula for the correction of resistance or conducting-power for temperature of an alloy as soon as we know its composition and its resistance at any temperature ; for , as r'10 r ' 0 , and r ' , may be calculated with the help of the formula given for the correction of conducting-power for temperature for most of the pure metals , if the constant rt-r't be determined , then r100 = rt2100 + constant , rt =r't constant , 0o =r00 + constant ; and from these terms the formula for the correction of resistance or conducting-power for temperature may be calculated , which in most cases will be found very near the truth .
In the second part we show by a few experiments that most alloys of three metals will probably be governed by the same law with respect to the influence of temperature on their conducting-power as alloys of two metals .
In the third part we deduce iP ' : : M mool.(4 ) P 100P 100te od ad cd ( where P and P ' represent the observed and calculated percentage decrements in the conducting-power of impure and pure metals between 0 ?
and 100 ?
C. , M1 and ' 10M their conducting-powers at 100 ?
C. ; P ' is for most metals 29-307 ) from Po : Pc : : X : X ' ... ( 1 ) 10 0o ... .1 For when we consider the last two terms of the proportion , and bear in mind that a trace of another metal has very little or no effect upon X'100o ( when it represents the conducting-power of an alloy consisting of one metal with only a trace of another metal ) , while it alters X10o to a very marked extent , it is evident that X'100o may be replaced by M1i00o We verify this by comparing the conducting-power of a pure metal directly determined , with the conducting-power of the same metal deduced from a determination of the conducting-power of its alloy with small quantities of other metals .
It is a curious fact , that the deduced values from experiments upon hard-drawn wires are in reality the conducting-powers of the annealed ire e of te pure metal .
After having thus verified the method , we have not hesitated to employ it in the determination of the conducting-power of certain metals which have not yet been experimented upon in a state of purity .
In the fourth part we point out , first , that the percentage decrement in the conducting-power of alloys between 0 ?
and 100 ?
is never greater than that of the pure metals composing them ; secondly , that the conducting-power of alloys decreases with an increase of temperature ( some bismuth alloys form an exception to this law ) ; thirdly , that in some cases the percentage composition of an alloy may be deduced from its conducting-power , with the aid of the percentage decrement in its conducting-power ; fourthly , the method which we have used for determining the class to which the metals belong in respect to the conducting-power of their alloys ; and fifthly , that the results which we have obtained and described in this memoir fully bear out the views put forward in a former one on the chemical nature of alloys .
|
112332 | 3701662 | On the Peroxides of the Radicals of the Organic Acids. [Abstract] | 655 | 658 | 1,862 | 12 | Proceedings of the Royal Society of London | B. C. Brodie | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 4 | 85 | 1,353 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112332 | null | http://www.jstor.org/stable/112332 | null | 108,803 | Chemistry 2 | 94.514304 | Tables | 4.093558 | Chemistry | [
-28.528947830200195,
-61.73280715942383
] | XII .
" On the Peroxides of the Radicals of the Organic Acids .
" By Sir B. C. BRODIE , Bart. , Professor of Chemistry in the University of Oxford .
Received June 18 , 1863 .
( Abstract .
) In a former notice published in the 'Proceedings of the Royal Society ' ( vol. ix .
p. 361 ) , an announcement was made of the discovery of a new group of organic combinations , the peroxides of the radicals of the organic acids-bodies which in the systems of the combinations of these radicals occupy the same relative position as is held by the peroxides of hydrogen , barium , or manganese in the systems of the combinations of those elements .
An account was given of the mode of preparation and properties of two members of this group , the peroxides of benzoyl and of acetyl , C,1 H1o 0 and C4 H6 04 .
The present paper contains an extension of this inquiry .
In it is given an account of several other peroxides of monatomic radicals , the peroxides of nitro-benzoyl , of cumenyl , of butyl , and of valeryl , and also an inquiry into the action of the peroxide of barium on the bibasic anhydrides .
The nitro-benzoic peroxide is formed by the action of fuming nitric acid on the peroxide of benzoyl .
It stands to peroxide of benzoyl in the same relation as anhydrous nitro-benzoic acid stands to anhydrous benzoic acid , and may be regarded as derived from that peroxide by the substitution in it of two atoms of peroxide of nitrogen for two of hydrogen .
The formula of the substance is C,4 Hg ( NO2)2 0 .
Calculated .
Found .
C14 ... ... . .
168 ... ... . .
50-60 ... ... . .
5060 I , ... ... . .
8 ... ... . .
2-41 ... ... . .
2-58 N ... ... . .
28 ... ... . .
8-43 ... ... . .
849 08 ... ... . .
128 ... ... . .
38-56 ... ... .
38-33 332 100-00 100-00 The peroxide of cumenyl is procured by a process strictly analogous to that by which the peroxide of benzoyl is formed ; it has the constitution C20 I22 04 .
The peroxides of butyl and valeryl are prepared by the action of hydrated peroxide of barium on the anhydrous acid .
It is only necessary to mix in a mortar equivalent quantities of the two sub1863.J 655 [ June 18 , stances .
The peroxide is separated by solution in ether from the water in which it is dissolved and suspended .
These substances are dense oily fluids , exploding slightly when heated , but not so readily decomposible as the peroxide of acetyl .
The analysis of the peroxide of butyl , dried by chloride of calcium , gave results corresponding with the formula C8 HE1 O0 .
Calculated .
Found .
C8 ... ... . .
96 ... ... . .
55-17 ... ... . .
55-11 1H , ... ... . .
14 ... ... .
8-05 ... ... . .
8-28 0 ... 64 ... ... . .
36-78 ... ... . .
3661 174 100-00 100-00 The analysis of the peroxide of valeryl gave results corresponding with the formula CIo HI1 04 .
Calculated .
Found .
C , , ... ... . .
120 ... ... . .
59-40 ... ... . .
59-39 H , , ... ... . .
18 ... ... . .
8-91 ... ... . .
9-17 0 ... ... . .
64 ... ... . .
31-69 ... ... . .
31-44 202 100-00 100-00 The mode of formation of these peroxides is given in the equation 2R , O0+Ba , 02=2Ba RO+R2 02 .
These substances are decomposed as well as formed by the action of the alkaline peroxide , according to the equation R2 02+ Ba202 =2 BaRO 1+0 , , giving a striking example of those consecutive actions referred to in a former paper as the cause of certain catalytic decompositions .
The action of the bibasic anhydrides on the alkaline peroxides is of special interest .
When anhydrous succinic acid , lactide , or anhydrous camphoric acid is mixed with an equivalent of hydrated peroxide of barium , a solution is obtained possessing the most powerful oxidizing properties , which bleaches indigo , evolves chlorine with hydrochloric acid , and oxidizes the protosalts of iron and manganese , but which does not discolour permanganic acid , or give with chromic acid the blue colour formed by peroxide of hydrogen .
When boiled , the solutions evolve oxygen , and afterwards contain a salt of the acid employed-in the case of succinic acid , giving a crystalline precipitate of succinate of 656 1863 .
] barium , and in the case of camphoric acid , giving with acetate of lead a precipitate of camphorate of lead .
These solutions are in a state of continual decomposition .
Only in one instance , that of camphoric acid , was it found possible to analyse the substance , and that only by indirect processes .
The oxygen contained in the organic peroxide was estimated in a measured portion of the solution by means of a standard solution of iodine ; the camphoric acid formed on boiling was determined by precipitation with acetate of lead in another measured portion ; and in a third portion the barium was estimated as sulphate .
The results of these determinations are given below , the camphoric acid being assumed as correct .
They lead to the conclusion that the solution contains the elements of one equivalent of anhydrous camphoric acid , one of oxygen , and one of baryta .
Atomic weight .
Calculated ratio .
Found .
C,0 1 03 ... ... . .
182 ... ... . .
25-12 ... ... . .
25-12 0 ... ... . .
16 ... ... 220 ... ... . .
207 Ba2O ... ... . .
153 ... ... . .
2112 ... ... . .
21-51 the reaction being C , , Hi , 0 , + Ba2 , 0-Co HE , , 0O Ba , .
That the substance formed is to be regarded as the baryta salt of the peroxide of camphoryl , and not as the camphorate of the peroxide of barium , is proved by the reactions of the solution , which does not give peroxide of hydrogen when decomposed by acids , or a precipitate of the hydrated peroxide of barium when heated with a solution of baryta .
The organic peroxides constitute a new and peculiar group of chemical substances characterized by reactions never hitherto found in any compound of carbon , and which materially extend our views of the possible properties of the so-called organic combinations , and of their analogies to inorganic substances .
They are the organic representatives of chlorine in the same sense as the oxides of the compound ammoniums are the representatives of potash , and in a yet closer sense than ether and alcohol resemble the oxide and its hydrate , or than ethyl or marsh-gas are analogous to hydrogen .
This analogy is of a profound character , not consisting merely in the analogy of symbolic form , but in the absolute identity of reactions .
657 The admitted analogies of the peroxide of chlorine have as it were their maximum in the organic peroxide .
Not only is chlorine represented in the peroxide , but hydrocloric acid is represented in the organic acid , and a series of parallel equations may readily be constructed , showing the identical character of the reactions of the two classes of substances .
Both bleach a solution of indigo , oxidize the protosalts of iron and manganese , decompose water under the influence of sunlight , and evolve oxygen with an alkaline peroxide , forming the salt of the corresponding acid .
|
112333 | 3701662 | Explorations in Spitzbergen, Undertaken by the Swedish Expedition in 1861, with the View of Ascertaining the Practicability of the Measurement of an Arc of the Meridian | 658 | 662 | 1,862 | 12 | Proceedings of the Royal Society of London | Otto Torell | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0144 | null | proceedings | 1,860 | 1,850 | 1,800 | 5 | 61 | 1,973 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112333 | 10.1098/rspl.1862.0144 | http://www.jstor.org/stable/112333 | null | null | Biography | 44.083891 | Geography | 35.205081 | Biography | [
57.86884307861328,
11.1585111618042
] | XIII .
" Explorations in Spitzbergen , undertaken by the Swedish Expedition in 1861 , with the view of ascertaining the practicability of the measurement of an Arc of the Meridian .
" By Dr. OTTO TORELL , Professor of Zoology in the University of Lund .
Communicated by the President .
Received June 2nd , 1863 .
In the year 1858 I made a voyage to Spitzbergen , in company with two other naturalists , in order to investigate the Natural History of that country .
I was thereby induced to study the history of the various Arctic expeditions that had gone out from England .
In Beechey 's and Barrow 's works I saw mentioned a suggestion which attracted my attention in a high degree .
A letter is there given from Captain Edward Sabine to Mr. Davies Gilbert , in which the writer , on his return from his celebrated Pendulum Expedition , proposes to explore Spitzbergen , with the view of ascertaining whether the measurement of an arc of the meridian could be carried out there* .
An arc from Ross Islet to Hope Island would comprise nearly 4- ?
of latitude-equivalent to an arc of 9 ?
in the mean latitude of France , and of 7 ?
in the mean latitude of Great Britain .
The difficulties opposed by climate and ground were not considered by Captain Sabine to be so great as not to be surmounted ; and he offered , in company with another officer and a sergeant of Artillery , to show either the feasibility or , once for all , the impossibility of the undertaking .
A special advantage is pointed out by Spitzbergen being divided into two nearly equal parts from north to south , thus very materially facilitating communications between the different angular points .
Admiral Beechey says that Captain Sabine 's plan was placed before the Royal Society in 1825 by Sir John Herschel , taken into consideration in the autumn of the same year , and warmly supported by Mr. Davies Gilbert , Sir I-Humphry Davy , the then President , and by other members of the Royal Society .
The reasons why it was not carried out are not mentioned ; but Sir John Herschel leaves us to infer that Captain Sabine was called upon to display his powers in another scientific undertaking of a more arduous though not less important kind .
This explanation appeared to be natural , and thus the whole matter was shelved for many years .
The plan in question seemed to me so simple and practical , and at the same time so useful in a scientific point of view , that I could not help espousing it with a very warm interest .
In the year 1860 , the Swedish government and Diet , as well as Prince Oscar , granted funds for a new scientific expedition to Spitzbergen .
Being placed at the head of this undertaking , in which a rather large number of scientific men were willing to take part , I did not fail to call the attention of the Academy of Sciences to the plan proposed by General Sabine in 1825 .
The Academy were alive to its importance ; and their two astronomical members , Professor Selander and Assessor Lindhagen , who had themselves taken part in the Swedish-Norwegian triangulation , considered that the explorations ought to be carried out , and for that purpose they issued the requisite directions to two of the participators in the expedition , Messrs. Duner and Chydenius .
To them it was confided to investigate whether suitable angular points could be found from the islands north of Spitzbergen to Hope Island in the South , either along the western coast of Spitzbergen or through iHinloopen Strait and Weide Jans Water , which nearly divide Spitzbergen into two from north to south .
One went on board the ship which , according to the plan , was to explore the north of Spitzbergen and Hinloopen Strait , and the other on board the other ship which was to explore the west of Spitzbergen and Weide Jans Water .
At the end of May 186 1 the two vessels reached Amsterdam Island , in nearly 80 ?
latitude ; and at the commencement of June they passed Verlegen Hook , and anchored in Treurenburg Bay , whence Parry , in 1827 , made his celebrated attempt to reach the North Pole .
But the polar ice immediately afterwards pressed against the coast , and imprisoned both vessels more than a month in Treurenburg Bay .
The pack was so close that no boat excursions of any extent could be made .
The explorations for survey were a good deal impeded by this circumstance ; for the investigation of the western coast of Spitzbergen could not be commenced until a much later period than intended .
The survey of Weide Jans Water could not be carried into effect , owing to drift ice , adverse winds , and calms .
Mr. Duner , to whom this undertaking was allotted , as well as the investigation of the practicability of the survey along the western coast of Spitzbergen , came to the conclusion that no impediments existed for carrying out the triangulation from Ross Islet to Amsterdam Island , but that the mountains surrounding Magdalena Bay are so steep and difficult or impossible of access , that the continuation of the survey southwards must be considered , if not absolutely impossible , at least so difficult and entailing such heavy expense , that its execution along that coast will probably never be carried into effect .
Mr. Chydenius , who was to explore the northern portion of the arc , presumed to be measurable from Ross Islet to Hope Island , was more fortunate in his work .
During sundry boat excursions and ascensions of many mountains from the northernmost part of Spitzbergen to the termination of Hinloopen Strait , he succeeded in completely solving the problem as to that part of Spitzbergen , comprising nearly the half of the arc to be measured .
The survey was carried out courageously and energetically under circumstances of frequent difficulty , as well in the drift ice as in crossing the glaciers of the interior .
The accompanying Ymap makes a detailed description unnecessary , and I therefore confine myself to stating that all the lines of the sights in the network marked with continuous lines are , with one single exception , observed , and that Mr. Chydenius has had opportunities of convincing himself that though not all the lines of the sights in the network marked with dotted lines are observed , yet nothing prevents the angular points connected by them from being seen one from the other .
The triangles connected by continuous lines of the sights are nine in number .
Their angles are computed by Mr. Chydenius in an accompanying Table .
All the angular points are selected on moderately high and accessible mountains , situated close to , or not very far from the coasts , and the distances between them are not greater than will admit of the signals being easily seen .
Mr. Chydenius found the ground , as well in Low Island as to the west of Treurenburg , to be favourable for measuring a base .
As the survey , so far as carried out , proves that , for executing the measurement of an arc of the meridian , no impediments exist which may not be overcome by courage and perseverance , there remains the question whether the part not yet explored may be expected to be equally favourable ; the reply to this cannot , of course , be fully given until a similar survey has been made of the still unknown portion ; there are , however , means of partially judging of the prospects of success .
Mr. Chydenius considers himself almost justified in stating with certainty that the mountains marked X and X on the map will be found to be visible from Weide Jans Water .
He is inclined to think that the easiest communication may be made through Lomme Bay .
The distance from I-inloopen Strait to Weide Jans Water cannot be great .
According to statements which , however , we were unable to verify , there is said to be a strait connecting these two sheets of water , and a vessel is reported to have sailed through it .
Mr. Lamont is also of opinion that Weide Jans Water is open to the north .
This , if found to be true , would tend greatly to facilitate the work .
It is also probable that the network can be drawn from the Waigat Islands at the southern embouchure of Hinloopen Strait to the Walter Thymen Bay , through the latter to Weide Jans Water , and further to Hope Island .
There still remains the question as to the facilities that the land on the two sides of Weide Jans Water may afford for the survey .
Those walrus-hunters whom I have interrogated regarding that part of the country , are unanimous in their opinion as to the mountains on the western side being similar to those on the west coast , that is to say , as inaccessible as possible .
But the country to the east of the said Water is described as a tableland , in which accessible mountains may be found in several places .
There are therefore well-founded reasons for thinking that the whole arc will be found measurable if the survey is continued .
Mr. Chydenius has offered to furnish the remaining part of the exploration .
The Swedish Academy of Sciences consider the completion of the survey so important , that they have petitioned Government to supply funds for carrying it into effect during the present or next year .
There is every probability that the money will be granted , and , if the result turn out as expected , that necessary steps will be taken for executing the measurement of the arc itself .
The Swedish Government has , at the instance of the Academy of Sciences , already furnished means for preliminary investigations in reference to another gecdetic enterprise , namely , for the Swedish share of the proposed large middle-European triangulation from Palermo to Trondhjem , and have asked the Estates for money for executing the measurement .
Should , then , the survey in Spitzbergen also be carried out , an important contribution will be made , not only to ascertain the compression of the globe in the vicinity of the North Pole , but also for the much-sought-after knowledge of the real form of the earth on different portions of its surface ; and the undertaking will to a certain degree complete the results both of the projected middle-European triangulation and of the Russo-Scandinavian already effected .
If the triangulation in question be executed , it will not be the only result arising from several years ' scientific labours in Spitzbergen .
It is superfluous here to allude to many investigations of importance which may be made ; it is sufficient to keep in mind the situation of Northern Spitzbergen , distant scarcely 10 ?
of latitude from the North Pole .
There are well-founded reasons for thinking that the execution of the measurement in question may be looked forward to .
And if we seek for the origin of the whole matter , we can trace it in Captain Sabine 's well-planned and lucidly explained project , which he submitted to the examination of the Royal Society in 1825 .
|
112334 | 3701662 | On the Magnetic Disturbance Which Took Place on the 14th of December 1862 | 663 | 668 | 1,862 | 12 | Proceedings of the Royal Society of London | Balfour Stewart | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0145 | null | proceedings | 1,860 | 1,850 | 1,800 | 6 | 65 | 2,421 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112334 | 10.1098/rspl.1862.0145 | http://www.jstor.org/stable/112334 | null | null | Meteorology | 42.739828 | Fluid Dynamics | 29.489678 | Meteorology | [
43.00812911987305,
10.534761428833008
] | XIV .
" On the Magnetic Disturbance which took place on the 14th of December 1862 .
" By BALFOUR STEWART , M.A. , F.R.S. Received May 19 , 1863 .
On the 14th of December 1862 , a magnetic disturbance occurred about 6 o'clock in the afternoon , and was registered by means of the Kew magnetographs .
As usual it was accompanied by an auroral display and by earth-currents , and the latter phenomena were observed at Greenwich by means of a system of telegraphic wires which had recently come into the possession of the Astronomer Royal .
By the kindness of Mr. Airy , the Kew Observatory has been favoured with a copy of the curves which represent the earth-currents collected at Greenwich during the progress of this disturbance ; and a comparison of these with the Kew magnetograph curves will form the subject of the following paper .
It will , however , first be necessary to state the arrangement adopted at Greenwich .
There are two wires proceeding from the Observatory , one ending near Croydon and the other near Dartford ( nearly at right angles ) ; and these are well insulated throughout their entire length , and have good earth-connexions at their extremities .
From these , by means of galvanometers , the intensity of earthcurrents is recorded for two very favourable directions ; and from these again the intensity of those currents which flow in the magnetic meridian , and in a direction perpendicular to it , may be very easily deduced .
The standard for direction is the current which flows through the wire of a battery from the zinc pole , and which is called the zinc-current .
With this explanation the earth-current diagrams appended to this paper will be quite intelligible ; and with regard to the magnetic curves , it is only needful to remark that increasing ordinates denote decreasing declination and decreasing horizontal force , and that the normal lines , which have been furnished through the kindness of General Sabine , denote the position which the curves would have occupied had no disturbance supervened .
But before proceeding to compare together the two sets of curves , it will be necessary to advert to a peculiarity of disturbances which enters as an essential element into all such discussions .
It has been found by General Sabine that if the disturbances of declination be divided into two categories , easterly and westerly , these obey very different laws of daily variation , and also that this difference is not of the same description for all stations ; so that we are compelled to view a magnetic disturbance as the resultant effect of two disturbances of different character , superimposed upon one another .
General Sabine has likewise stated his opinion that this duality of action may perhaps be due to the disturbing force entering the earth at two or more points , one denoting magnetism of a more permanent kind , and the other magnetism of an induced description .
A study of the Kew disturbance-curves tends to give confirmation to such an idea ; for in these it is seldom found that the whole body of force which produces a disturbance is one which preserves the same type throughout and only varies in intensity .
Even if we suppose that this type will vary with the hour of the day , we shall find , if we take disturbances which last for several days , that the type of force at a given hour of the first day is in very many cases different from that during the same hour of the second .
When , however , we confine our attention to very abrupt changes of force , we find that the disturbance-type which these display retains more of the same character throughout a disturbance .
In order to explain this , we may perhaps suppose that there are two sets of magnetic particles in the earth-one set being of the nature of soft iron , and the other similar to hardened steel .
Now only the first of these would be acted on by any very sudden change in the disturbing force , since it would require time in order to influence the second set .
We may thus perhaps account for the fact that any very sudden change is of one type , since it only influences one set of particles .
Let us now consider what will take place if a disturbance of the same primary nature continues for any length of time .
IIere the hard-iron particles will also be influenced to an extent compounded of the time and of the average value of the disturbing force during that time .
The magnetic needle , therefore , will now be acted on by the joint influence of these two sets of par .
ticles , whereas at the beginning of the disturbance it was only acted on by one of them , namely , the soft-iron ones .
The type of force will therefore have changed if the hard-iron particles are differently distributed in our globe from the soft-iron ones ; and if , instead of two , there are many sets of particles , we shall have a very complicated effect .
Now this duality of disturbing forces must be considered when we attempt to ascertain the connexion between such forces and earthcurrents , since we are not entitled to suppose that one of these two forces is related to earth-currents in precisely the same manner as the other .
A small soft-iron force may be comparable to a large hard-iron one as far as an earth-current is concerned ; or the reverse may be the case .
When , however , there is a very rapid change of disturbing force , since this affects the earth through only one set of particles , we shall by its means be better able to trace the bond of connexion between a single type of magnetic force and the corresponding earth-current .
Rapid changes of force are therefore of peculiar value in such an investigation .
Bearing this in mind , let us endeavour to connect together the phenomena of earth-currents and magnetic disturbances by two successive hypotheses , one of which , it would seem , must represent the truth unless there be some new link of connexion between magnetism and electricity with which we are unacquainted .
The first hypothesis is that in which earth-currents are supposed to give rise to magnetic disturbances according to the laws by which a current acts upon a magnet .
This may be called the theory of direct action .
By the second hypothesis , earth-currents are supposed to be induced , or secondary currents generated in the crust of the earth by those small but rapid changes in terrestrial magnetism which consti .
tute disturbances .
This may be called the theory of induced action .
Now , first , on the theory of direct action .
Zinc-currents going to the south should correspond with magnetic disturbances decreasing the declination ; and zinc-currents going to the east should cIorrespond with an increase of horizontal force ; but we find by the diagrams that while on this hypothesis the disturbance of the horizontal-force needle will be tolerably well accounted for by the east and west cur .
rents , the same correspondence does not hold between the north and south currents and the declination-disturbance .
But I do not think that this circumstance , rightly viewed , tells either in favour of or against the hypothesis .
A glance at the earth-current curves will show that the ordinates of the one bear generally a fixed proportion to those of the other , showing us that the total current has flowed backwards and forwards along one line* ; and though it is equally apparent , by a glance at the magnetic curves , that the same type of force has not been preserved throughout the disturbance , yet the explanation of the unity of type in the earth-currents may be that these are twisted into a line of motion , owing to the disposition of the conducting strata of the earth 's surface , just as a current can only move backwards or forwards along an insulated wire .
Indeed a little reflection will show us that earth-currents are not local phenomena ; so that if we endeavour to estimate quantitatively their influence on the magnet according to the hypothesis of direct action , we must first extend our field of observation , and obtain their value in other countries besides our own .
But to return to our comparison of curves .
We see that for the greater part of the disturbance both the horizontal force and the declination were very much above their normal lines , while on the other hand the currents were frequently crossing their zero lines , and that both currents were simultaneously and for a long portion of their time very near zero , although during this time the magnetic disturbance was considerable .
Next , with respect to a very abrupt disturbance which commenced about 8h 50m , the corresponding earth-current curves are exceedingly powerful , alternately passing and repassing the zero line to nearly the same distance on both sides , while the absolute disturbance of the horizontal force , and probably of the declination , was not very great .
We have thus , in the first place , a very sluggish action of earthcurrents , while the magnetic disturbance was considerable , and in the next place a very violent action of the former when the absolute disturbing force was by no means excessive ; and we may add that at 9h 50m both earth-currents were near zero , while both elements of the earth 's magnetism were much disturbed .
For all these reasons this comparison of the curves is unfavourable to the hypothesis of direct action .
Let us now consider the other hypothesis , or that of induced action , and we shall find the following points in its favour .
1st .
That in this disturbance , for at least one hour , both elements of the earth 's magnetic force remained at a considerable distance from their normals , and that during this time the earth-currents observed were exceedingly small .
Now , on the hypothesis of induced action , the earth-current effect depends not on the absolute value of the disturbing force , but on its rate of change ; and if during this period we examine the horizontal-force curve , we shall find the abruptness of change not so great as in those cases where greater earth-currents were produced , while in the declination-curve the abruptness of change during this period is exceedingly small .
2nd .
A reference to the diagrams will show us that in general the most abrupt magnetic disturbances are those which are accompanied by the greatest earth-currents , and that in particular a very abrupt disturbance , which took place about 8h 501 , was accompanied by very strong earth-currents , alternately positive and negative , those of the one name being nearly as powerful as those of the other , while on the other hand the corresponding magnetic disturbances were on an average decidedly on one side of the normal lines .
On the other hand , the following fact seems at first to tell against the theory of induction .
An inspection of the curves will show that we have currents remaining on one .
side of the zero-line for some length of time , during which the magnetic disturbances have nevertheless changed in both directions .
When , however , we reflect on this circumstance , we are led to see that since we have two sets of disturbances taking place simultaneously , so we must also have two sets of earth-currents .
Now one of these disturbances , which we may perhaps call the soft-iron one , reproduces those small and rapid changes which take place in the primary force , while on the other hand the hard-iron disturbance averages these small changes and presents us with a disturbance-wave of long period .
Precisely , then , as in the magnetic curves we have waves of short period superimposed upon waves of long period , so will it be in the earth-current curves .
Those currents due to the soft-iron disturbances will be superimposed upon those due to the hard-iron ones , with this difference , that we are not entitled to assume that the proportion in intensity between the two simultaneous earth-currents must be precisely that which exists between the rates of change of the two corresponding simultaneous disturbances .
It will be apparent that this feature of duality ought also to be presented by the aurora ; and here it is well known that we have at least two phenomena , one of a more fitful and the other of a more permanent character , namely , the streamers and the auroral arch .
We may suppose the first of these phenomena to correspond to the soft-iron , and the second to the hardiron disturbances .
Indeed it is questionable whether the different 1863 .
] 667 varieties of aurore are confined to these two ; for General Sabine has informed me that he himself , along with the late Sir Edward Parry , observed at Lerwick in the Shetland Isles in 1818 , at the same instant , two auroral arches crossing one another at an angle .
But , be this as it may , when we reflect that there are many kinds of particles in our earth , some of which may be affected more rapidly than others by a primary magnetic force , we shall cease to wonder that the phenomena presented are of a complicated description .
All these considerations have induced me to think that it is lost labour to attempt a quantitative comparison when our observation of the magnetic disturbances and their corresponding earth-currents is confined to one locality ; and it will be seen from this paper , that while endeavouring to uphold the hypothesis of induced action , I have done so by a comparison of a general and qualitative rather than by one of a quantitative nature .
|
112335 | 3701662 | Further Observations in favour of the View That Nerve-Fibres Never End in Voluntary Muscle | 668 | 671 | 1,862 | 12 | Proceedings of the Royal Society of London | Lionel S. Beale | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0146 | null | proceedings | 1,860 | 1,850 | 1,800 | 5 | 59 | 1,635 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112335 | 10.1098/rspl.1862.0146 | http://www.jstor.org/stable/112335 | null | null | Biology 3 | 46.390171 | Neurology | 26.60868 | Biology | [
-70.53460693359375,
5.873867034912109
] | XV .
" Further Observations in favour of the View that Nervefibres never end in Voluntary Muscle .
" By LIONEL S. BEALE , M.B. , F.R.S. , Fellow of the Royal College of Physicians , Professor of Physiology and of General and Morbid Anatomy in King 's College , London ; Physician to King 's College Hospital , &c. Received June 5 , 1863 .
Few anatomical inquiries of late years have excited more interest than the present one .
Since my paper published in the 'Philosophical Transactions ' for the year 1860 , several memoirs have appeared in Germany .
In my paper just published in the last volume of the 'Transactions , ' I have replied to the statements of Kiihne and K61liker , but I had not succeeded in actually tracing the very fine nucleated fibres I had demonstrated from one undoubted nerve-trunk to another .
As a demonstration , therefore , my conclusions were defective , though the only explanation to be offered of facts I had observed was that included in the view I propounded in my first paper .
The question between my opponents and myself upon this matter is not one of interpretation , but a question of simple fact .
I assert that the fine nerve-fibres can be followed much further than the point where Kiihne and Kolliker maintain the ends or termina668 June 18 , tions are situated , if the specimen be so prepared as to prevent destruction of these most delicate fibres , and the refractive power of the medium be such as to enable us to see them .
I propose to present to the Royal Society next session a paper in which I shall demonstrate the truth of the conclusions I have arrived at ; but as my specimens are already prepared , and during the last few months several drawings have been made , I hasten to give a short statement of facts , in order that those who have been led to conclusions opposed to my own may have an opportunity of studying the very same muscle .
The great width and refractive power of the large elementary fibres of the pectoral of the common frog render it impossible to follow for any great distance amongst them nerve-fibres of the 61 th of an inch = -000187 " ' in diameter ; and I have there .
fore long been searching for a very thin voluntary muscle , with fine fibres , which , like the bladder of the frog , could be examined without the necessity of making thin sections , and thereby deranging the relation of all the finest and most delicate structures .
Such a muscle I have found in the extensive mylo-hyoid of the little green tree-frog ( Hyla arborea ) .
The elementary fibres of this muscle are scarcely more than the 3o1th of an inch = -0036 " ' in diameter ; and as there are but two layers , the fibres of which are at right angles to each other , all the structures in the muscle can be demonstrated most beautifully .
The very long thin muscular fibres are not too close for exact observation .
The vessels can be readily injected.* These specimens have been prepared upon the same plan as others , and are preserved in glycerine , which enables me to press the thin muscle and separate the fibres further from each other , while the finest fibres of the nerves are prevented , by the viscid medium , from breaking or from being so compressed amongst the other tissues as to be destroyed or rendered invisible .
The muscle must be prepared when quite fresh , otherwise the fine nucleated fibres are completely disintegrated .
The capillaries were injected as in the other cases* .
In this thin muscle , networks formed by bundles of dark-bordered fibres , consisting of from two to five or six , may be very easily shown , and with high powers ( 700 to 3000 diameters ) the very fine nucleated fibres resulting from the division and subdivision of these in a dichotomous t manner , can be readily demonstrated .
In this thin muscle I have often followed individual fine nucleated nerve-fibres , now over , now under muscular fibres , sometimes crossing transversely , sometimes obliquely , and sometimes running for a certain distance parallel to the fine muscular fibre .
The drawing accompanying this paper renders further description unnecessary .
I shall enter into full detail in my communication next session ; but as the summer is the period to obtain specimens of the Hyla , I am anxious my fellow-labourers in Germany should at once be acquainted with the advantages of the thin muscle alluded to ; and I cannot too strongly recommend this beautiful little frog , which they have the advantage of procuring more readily than Englishmen , for microscopical investigation .
All the tissues are beautifully distinct , and I challenge those who are interested in these questions to discuss them with me , selecting the tissues of this animal for special study .
EXPLANATION OF THE PLATE .
Distribution offinest nucleated nerve-fibres to the very narrow elementary muscular fibres of the mylo-hyoid of the little green tree-frog ( Hyla arborea),.magnified 1700 diameters .
Drawn on the block by the author .
The elementary muscular fibres are marked g , h , i , 7c .
k is a very young one , slightly stretched ; i is a fully-formed muscular fibre ; h , another stretched in its central part .
The nuclei of these fibres exhibit some differences in size and form .
Nucleoli are distinct in all , and in the fibre marked g the nuclei , which were.coloured by carmine , exhibit three different intensities of colour , the dark central spot , " nucleolus , " being most intensely coloured , as indicated by the shading in the drawing .
7,3"O iii:~i I i , i -.B C1 1/ i":~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ ' a~~~~~~~~~~~~~~~ G~~~~~~~/ l 'Ki I 1 !
/ 11/ ' / / % 1/ Y'~ / / ' ' , ; 712 Vk/ ~~~~~~~~~7 PI Dl o~ibLrof ( 1 ' , / 02 Ic f1217 CAI rVolt ~-cv W41e I/ tc 111 OLCtlu ( o 10 fo e y-ofb I , ,~~~~~~~~~~~~~~~~~ " C22/ ~rs .
Povv1 e al oLn LIlh d2or1d/ of ea/ h / uAC bb A o/ ofala redi blod-corpuscl .
) SCALE .
) , IOf aii Enqlish l llcl l uq-~rkm x ' 11-00 diameters .
I I0iIii .
1/ 1,1 5-1 .
'k I I\ I/ III ?
~ , ?
/ " ~ , j / " \ a is a nerve-fibre which was followed over more than twenty elementary muscular fibres from a dark-bordered fibre .
One of the subdivisions of this fibre is seen atf , where it again runs with a very fine dark-bordered fibre ( o ) .
The darkbordered fibre ( o ) was some distance higher up in the specimen , but its place has been altered in order to avoid the necessity for a still larger drawing .
Above ba nucleus of a very fine nerve-fibre is seen .
Such nuclei lie upon the surface of the muscular fibres , external to the sarcolemma .
The nucleus often appears as if it were within the sarcolemma ( c ) , but the fibres proceeding from each extremity render such a position impossible .
The relation of these nerve-nuclei to the sarcolemma is seen at I in profile .
The nuclei , as well as the fibres for a certain distance , often adhere to the sarcolemma very firmly ; but in the thin mylo-hyoid muscle the course of the fibres over or under , but always external to the muscular fibres , may be readily traced if the muscular fibres be separated slightly from each other , as represented in the drawing .
At d fine nerve-fibres accompanying the fine fibre continued from the darkbordered fibre , as described in the ' Philosophical Transactions ' for 1862 , are represented .
Such fibres are also seen at e and f. m , n , and o dark-bordered fibres , with nuclei near their distribution .
m would probably pass over sixty or seventy muscular fibres , and n over perhaps twenty , before it divided into fibres as fine as those seen at b , e , f , 1 .
pa very fine capillary vessel with a nerve-fibre running close to it .
qa bundle composed of six very fine nerve-fibres near their distribution .
These fibres exhibit a very distinctly beaded appearance , which is also observed in many other fine fibres in different parts of the specimen .
Traces of connective tissue are seen in all parts near the fine nerve-fibres and around the muscular fibres .
Here and there some very fine connective tissuefibres , which were not altered by acetic acid , are represented .
These represent the remains of fine nerve-fibres , which existed in a state of functional activity at an earlier period .
The drawing , with the exception of the position of the nerve-fibre ( o ) above mentioned , is an actual copy from nature .
The relative position of the muscular fibres , the form and general characters of the so-called nuclei , and the position and size of the nerve-fibres and their nuclei have been carefully preserved .
I have traced the very fine nerve-fibres in so many instances from one trunk to another ramifying at a very considerable distance , that I cannot believe any true terminations or ends exist .
|
112336 | 3701662 | Note on the Minute Structure of the Grey Matter of the Convolutions of the Brain of Man, the Sheep, Cat, and Dog | 671 | 673 | 1,862 | 12 | Proceedings of the Royal Society of London | Lionel S. Beale | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0147 | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 34 | 934 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112336 | 10.1098/rspl.1862.0147 | http://www.jstor.org/stable/112336 | null | null | Biology 3 | 49.345198 | Neurology | 45.948711 | Biology | [
-78.25985717773438,
9.252556800842285
] | XVI .
" Note on the Minute Structure of the Grey Matter of the Convolutions of the Brain of Man , the Sheep , Cat , and .
Dog .
" By LIONEL S. BEALE , M.B. , F.R.S. , &c. Received June 18 , 1863 .
By a new process of investigation , I have succeeded in demonstrating the connexion between the nerve-cells and fibres in the grey matter of the convolutions and in other parts of the mammalian brain , and have followed individual fibres for a much greater distance 1863 .
] 671 than can be effected in sections prepared oy other processes of investigation which I have tried .
In many instances one thick fibre is continuous with one or other extremity of the " cell , " while from its opposite portion from three to six or eight thinner fibres diverge in a direction onwards and outwards .
This arrangement is particularly distinct in the grey matter of the sheep 's brain .
The broad extremities of the cells for the most part are directed towards the white matter of the hemisphere .
The cells have no cell-wall ; and the matter of which the fibre is composed is continuous with that of which the outer part of the " cell " consists .
The so-called " granular matter , " or " granular matrix , " which is described as existing in considerable quantity in the grey matter around the cells and between the fibres , results , I think from the disintegration of the finest nerve-fibres and cells ; for in the specimens I have prepared , the tissue intervening between the cells is seen to be composed entirely of nerve-fibres .
The majority of these fibres are not more than the oo th of an inch in diameter ; and many fibres , whose continuity with cells can be demonstrated , are as fine as this at a distance of not more than I o1th of an inch from their origin .
The slightest displacement of the thin glass covering the specimen will often destroy these delicate fibres , and nothing but amorphous granular matter results .
The apparently free nuclei in the more superficial part of the grey matter are really the nuclei of cells , with every one of which fibres are in connexion .
There are no cells with less than two fibres in continuity with them .
In the brain of a young animal it is easy to find many cells connected together by broad bands of fibres , which vary much in length and thickness ; but in the adult a positive connexion between two contiguous cells can be demonstrated only here and there .
As the cells separate further and further from each other , the fibre becomes so thin and long , and it changes the plane in which it ramifies to such an extent , that it cannot often be traced for any great distance .
The fibres are formed as the cells , originally continuous , become separated further and further from each other .
In all parts of the nervous system the so-called " cells " ( often termed " nuclei " in peripheral parts ) are structurally continuous with each other through the fibres .
67 The fibres are not offsets or outgrowths which grow centrifugally from different adjacent cells and then join or anastomose with one another , but they result , on the other hand , from the moving away from each other of cells which were originally continuous ; so that a very thin fibre of o-1 th of an inch in diameter , and perhaps three or four thousandths of an inch in length , represents the broader and shorter bands or cords of communication which existed at an earlier period of development , when the cells were much closer together .
It has been stated that nerve-cells do not exist in the white matter ; but numerous cells are present in this tissue for the distance of perhaps the sixth of an inch or more beneath the grey matter .
I do not propose now to enter into detail ; the arrangement of the cells and fibres will be accurately represented in drawings ; for it is not possible for me to convey an accurate idea of the structure of this elaborate tissue by description .
I may be permitted to offer the following general conclusions resulting from observations upon the grey matter of the convolutions of man , the sheep , cat , and dog .
1 .
The numerous nerve-cells of the grey matter are all connected or give origin to at least two fibres .
2 .
These fibres , wide near their origin , gradually diminish in thickness until they are not more than the th of an inch in diameter .
3 .
The granular matter said to be so abundant in the grey matter consists of fine and very delicate nerve-fibres , which are easily broken down when thin sections of this soft tissue are submitted to microscopical examination without special preparation .
4 .
It is probable that the cells of the grey matter of the convolutions are connected together ; but in the adult the cells are not often connected with those cells which are situated nearest to them .
5 .
There is no reason for supposing that the nerve-cells , here or elsewhere , influence any nerve-fibres save those which are structurally continuous with them .
1863 , ] 673
|
112337 | 3701662 | On the Change in the Elastic Force of a Constant Volume of Dry Atmospheric Air, between 32\#xB0; F. and 212\#xB0; F., and on the Temperature of the Freezing-Point of Mercury. [Abstract] | 674 | 674 | 1,862 | 12 | Proceedings of the Royal Society of London | Balfour Stewart | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 1 | 12 | 229 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112337 | null | http://www.jstor.org/stable/112337 | null | null | Thermodynamics | 81.084858 | Fluid Dynamics | 8.066785 | Thermodynamics | [
-5.826540470123291,
-16.550880432128906
] | XVII .
" On the Change in the Elastic Force of a Constant Volume of dry Atmospheric Air , between 32 ?
F. and 212 ?
F. , and on the Temperature of the Freezing-point of Mercury .
" By BALFOUR STEWART , M.A. , F.R.S. Received June 18 , 1863 .
( Abstract .
) The author gave a detailed description of his apparatus , and of the method employed in drying the air .
The result of his experiments gave as the coefficient of increase of elasticity of air of constant volume for 1 ?
F. 0'002040 , this being slightly different from that given by Regnault , which is 0'002036 .
He also finds that the temperature of the freezing-point of mercury is constant , and that its value on Fahrenheit 's scale , as given by an air-thermometer , is -37§ 93 , while as recorded by a standard mercurial thermometer it is -38 ?
'00 .
It is probable that this difference is owing to an anomalous contraction of mercury before it freezes , similar to the corresponding expansion of water ; but this effect in the case of mercury seems to be very small , and it may be said that a mercurial thermometer properly graduated , will denote the true temperature , even down to the freezing-point of the mercury itself .
|
112338 | 3701662 | On the Degree and Weight of the Resultant of a Multipartite System of Equations | 674 | 676 | 1,862 | 12 | Proceedings of the Royal Society of London | J. J Sylvester | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0149 | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 34 | 764 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112338 | 10.1098/rspl.1862.0149 | http://www.jstor.org/stable/112338 | null | null | Formulae | 49.458833 | Thermodynamics | 34.932513 | Mathematics | [
-5.826050758361816,
-16.564128875732422
] | XVII .
" On the Change in the Elastic Force of a Constant Volume of dry Atmospheric Air , between 32 ?
F. and 212 ?
F. , and on the Temperature of the Freezing-point of Mercury .
" By BALFOUR STEWART , M.A. , F.R.S. Received June 18 , 1863 .
( Abstract .
) The author gave a detailed description of his apparatus , and of the method employed in drying the air .
The result of his experiments gave as the coefficient of increase of elasticity of air of constant volume for 1 ?
F. 0'002040 , this being slightly different from that given by Regnault , which is 0'002036 .
He also finds that the temperature of the freezing-point of mercury is constant , and that its value on Fahrenheit 's scale , as given by an air-thermometer , is -37§ 93 , while as recorded by a standard mercurial thermometer it is -38 ?
'00 .
It is probable that this difference is owing to an anomalous contraction of mercury before it freezes , similar to the corresponding expansion of water ; but this effect in the case of mercury seems to be very small , and it may be said that a mercurial thermometer properly graduated , will denote the true temperature , even down to the freezing-point of the mercury itself .
XVIII .
'On the Degree and Weight of the Resultant of a Multipartite System of Equations .
" By Professor J. J SYLVESTER , F.R.S. Received May 25 , 1863 .
Let there be ( l n ) equations each homogeneous in any number of sets of variables , and suppose that the degrees of the several equations in respect to these sets are respectively a , b , c,. .
, , a l , , c l ) , ? . .
, le a Le t*no e 1 +o , 1+f3 , 1+y,. .
1+ X , then in order that the system may have a resultant , since the number of ratios to be eliminated is +/ 3 +y+ ... +X , this sum must be equal to n. Let ai +bi + cir+. .
+c:w=L , and let LL , , L2 , ... L= P , then 1st , the degree of the resultant in question in regard to the coefficients of the rth equation will be the coefficient of r. 7 .
ry ... in P Lr 2nd .
As regards weight .
By the weight of any letter in respect to any given variable is to be understood the exponent of that variable in the term affected with the coefficient ; and by the weight of any term of the resultant in respect to such variable , the sum of the weights of its several simple factors ; each term in the resultant in respect to any given variable has the same weight ; and this weight may also be proved to be alike for each variable in the same set , and may be taken as the weight of the resultant in respect to such set .
This being premised , we have the following theorem : The value of the weight of the resultant in respect to any particular set of the variables , ex. gr. the ( 1 + a ) set , will be the coefficient of pf+ .
a. ry. .
X. in P. In the particular case where a=f3=y ... =X , the above expressions for the degree and weight evidently become polynomial coefficients .
Thus , ex. gr. , if we suppose each equation linear in respect to the variables of each set , the degree of the resultant in respect to the coefficients of any equation will be rr(a+3+y ... +X ) 7r .
7r .
Try..7rX and its weight in respect to the ( 1 +a ) set will be r(l+a+/ 3+ ... + x ) 7r(l -a)7r,8 .
ry * .
*r(X ) In particular if each set is binary , so that a=-3=y ... X* 1 , the degree becomes 7r(n ) , and the weight r( + .
The above eores ae , I believe , altogether new .
The above theorems are , I believe , altogether new .
It may just be noticed ( as a passing remark ) that the total degree in the general case is the coefficient of..rY ... , xinP { + +'*'+ and the total weight the coefficient of the same argument in P +-+ Ra +a R
|
112339 | 3701662 | Some Remarks Appended to a Report on Mr. Hopkins's Paper on the Theory of the Motion of Glaciers | 676 | 679 | 1,862 | 12 | Proceedings of the Royal Society of London | John F. W. Herschel | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0150 | null | proceedings | 1,860 | 1,850 | 1,800 | 4 | 26 | 1,394 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112339 | 10.1098/rspl.1862.0150 | http://www.jstor.org/stable/112339 | null | null | Fluid Dynamics | 42.517263 | Geography | 21.450137 | Fluid Dynamics | [
15.726004600524902,
-0.8267326354980469
] | XIX .
" Some Remarks appended to a Report on Mr. HIopkins 's Paper 'On the Theory of the Motion of Glaciers'* " .
By Sir JOIIN F. W. I-ERSCHEL , Bart. , F.R.S. ( Referee ) .
Received January 31 , 1863 .
A few remarks arising out of the perusal of this paper may perhaps not be considered as out of place on the present occasion .
They are not meant as in any way impugning the author 's views of the laws determining the fracture and disruption of glacier masses , or their application to glacier-phenomena in general , but in relation to the somewhat mysterious process of regelation itself , and to those generally recognized and most remarkable facts of the gradual conversion of snow into more or less transparent ice , and the reunion of blocks and fissured or broken fragments , under the joint influence of renewed pressure and of that process ( whatever its nature ) , into continuous masses .
If regelation be really a process of crystallization , it seems exceedingly difficult to imagine how the molecules forming the cementing layer between two juxtaposed surfaces can at once arrange themselves conformably to the accidentally differing axial arrangements of those of the two surfaces cemented .
A macled crystal is indeed a crystallographical possibility ; but then the axes of the two individuals cohering by the made-plane have to each other a definite geometrical relation in space , as is well exemplified in the case of the interrupting film in Iceland spar .
At the temperature at which " regelation " takes place ( viz. the precise limit between the liquid and solid states ) , it seems to me very possible that the cohesive forces of the molecules of the cemented surfaces may be so nearly counteracted as to bring those surfaces into what may be so far regarded as a viscous state as to permit ( not indeed a sensible and finite change of figure of a small portion of the mass without fracture , but ) a certain freedom of movement in the individual molecules , to some sensible depth within the surface , so as to allow of a gradually progressive deviation of their axes from exact parallelism , and thus to effect a transition from one crystalline arrangement to another-not by macling , but by curvilinear distortion , such as may be conceived to prevail in pearl-spar and other similar disturbed forms of crystals .
Nay , I can conceive it possible that by very long continuance at this exact temperature ( especially if aided by tremors short of disruption propagated through the mass , which , as we see in the crystallization of cold wrought iron in the axle-trees of railway carriages , powerfully favour the crystalline rearrangement of molecules even in the most rigid solids ) the contiguous blocks may influence each other 's crystallization to a greater and greater depth through the medium of the cementing film , thus tending continually to straiten the curve of the connecting chain of axes , and after a very long time to bring the two blocks into perfect conformity , so as to form an uninterrupted crystal ; and this , or something like this , I take to be the process by which the snow of a never is converted into the imperfectly transparent and sometimes fully transparent ice of a glacier .
Tremors of the kind here alluded to would not be wanting in a glacier in continued process of displacement , and in some part or other of which disruptions consequent on violent strain are momentarily taking place .
On the subject of the temperature of the interior of a glacier , I would observe that there will be found in the archives of the Royal Society , on the occasion of the Committee for recommending objects of inquiry to Lieut. Foster during one of his Polar expeditions , a recommendation of mine that the expedition should be furnished with a set of boring-implements for the purpose of piercing some very large and compact mass of ice , with the expectation of finding it much below the freezing-temperature .
The heat of summer , it was suggested , would all be carried off in the water resulting from surfacemelting ; while the intense cold of a polar winter would penetrate the interior , and thus give rise to a mean temperature very far below that of the external climate .
The implements ( if I remember rightly ) were furnished , but Lieut. Foster reported that no mass of ice sufficiently large could be met with so free from fissures as not to be permeated by infiltering water during the summer months ; and if any results were obtained , they were not striking or definite enough to be worth recording .
That the lower surface of a glacier in contact with the earth is in a constant state of fusion , even in those cold regions , is proved by the phenomena recorded by Dr. Kane of the Mary Minturn River in lat. 78 ? ?
54 ' , and the feeder of the Kane Lake , lat. 78 ? ?
18 ' , which never ceases to flow , summer or winter .
Admitting this as a general fact , the sliding of a glacier on its bed is an obvious necessity ; and that it should be unaccelerated is no more a matter of wonder or difficulty of conception than the unaccelerated descent of the weight of a clock which is never abandoned to its own impetus , but brought to rest after every momentary descent by the action of the scapement , -or the unaccelerated fall of a body in a resisting medium when the resistance becomes equal to gravity , or of a weight gradually and uniformly lowered by the hand .
Perhaps the more general way of conceiving it would be to regard the whole glacier as a mass propped up against a support anyhow inclined , and prevented from tumbling over sideways by lateral stays .
Such a mass would rest in its position , if duly supported either by a baseabutment , or by a heap of its own debris ; but if these were slowly abraded , destroyed , or picked away , the whole mass would descend bodily in the exact manner of the withdrawal of support .
On the disruption of a nearly homogeneous elastic solid in a state of strain , I would add a remark which seems to me of some moment , as explanatory of the greater cohesive strength which is well known to be imparted to cements , especially those of a resinous or gummy nature , by the admixture of extraneous matter in fine powder .
If in such a solid there be one portion , however small , weaker than the rest , the strainbeinguniform , a crack will originate in that place .
Now a crack , once produced , has a tendency to run-for this plain reason , that at its momentary limit , at the point on which it has just arrived , the divellent force on the molecules there situated is counteracted only by half the cohesive force which acted when there was no crack , viz. , the cohesion of the uncracked portion alone .
But if a crack anywhere produced be stopped from running by encountering a solid particle of greater cohesive force , fracture will no longer be determined by the accidental deficiency of cohesion at some weak point , but by the average resistance of the whole cementing mass .
It would , I think , be interesting to determine , on the more transparent portions of glacier ice , by the simple and easily applied test of polarized light , whether a definite crystalline structure prevail in its interior , and if so , in what direction the axis lies in relation to the lines of fissure in the crevasses .
Nor is there any reason why the idea above thrown out respecting the mutual modification of structure of two masses cemented by regelation , at or near their plane of junction , should not be subjected to a similar test .
|
112340 | 3701662 | On the Absorption and Radiation of Heat by Gaseous and Liquid Matter.--Fourth Memoir | 679 | 683 | 1,862 | 12 | Proceedings of the Royal Society of London | John Tyndall | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0151 | null | proceedings | 1,860 | 1,850 | 1,800 | 5 | 63 | 1,924 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112340 | 10.1098/rspl.1862.0151 | http://www.jstor.org/stable/112340 | null | null | Thermodynamics | 42.118513 | Measurement | 15.33479 | Thermodynamics | [
4.222079753875732,
-20.937355041503906
] | XX .
" On the Absorption and Radiation of Heat by Gaseous and Liquid Matter."-Fourth Memoir .
By JOHN TYNDALL , F.R.S. Received June 18 , 1863 .
In his former researches on the absorption and radiation of heat by gaseous matter , the author compared different gases and vapours at a common thickness with each other .
In the first part of the present communication he determines , in the case of several gases and vapours , the absorption effected by different thicknesses of the same gaseous body .
His least thickness was 0-01 of an inch , and his greatest 49'4 inches ; thus the thickness varied from 1 to nearly 5000 .
The apparatus employed for the smaller thicknesses consisted of a hollow cylinder , with its end closed by a plate of rock-salt ; into this fitted a second hollow cylinder , with its end closed by a second plate of salt .
One cylinder moved within the other as a piston , and by this means the plates of salt could be brought into flat contact with each other , or separated to any required distance .
The distance between the plates was measured by means of a vernier .
The cylinder was placed horizontal , being suitably connected with the front chamber used in the author 's former researches , and the source of heat employed was a copper plate , against which a steady sheet of gas-flame was caused to play .
The absorptions of carbonic oxide , carbonic acid , nitrous oxide , and olefiant gas were determined by this apparatus , and such differences as might be anticipated from former experiments were found .
Olefiant gas maintained its great supremacy over the others at all thicknesses .
A layer of this gas , 0'01 of an inch thick , effected an absorption of about 1 per cent. of the total radiation .
To show the competence of the apparatus to measure an absorption of this magnitude , it is only necessary to state that the galvanometric deflection corresponding to this absorption was 11 degrees .
Were it worth while , it might be shown that the absorption by a plate of the gas not more than f-01-th of an inch in thickness is capable of measurement .
A layer of olefiant gas 2 inches in thickness intercepted nearly 30 per cent. of the entire radiation .
Such a layer , encompassing the earth as a shell , permitting the passage of the solar rays , and preventing the escape of the terrestrial ones , would probably raise the surface of the earth to a stifling temperature .
A layer of the gas three-tenths of an inch in thickness intercepts 11'5 per cent. of the radiation .
Such a layer , if diffused through 10 feet of air , would be far more attenuated than the aqueous vapour actually existing in the air ; still it would effect an absorption greater than that which the author has ascribed to the atmospheric vapour within 10 feet of the earth 's surface .
In the presence of such facts , arguments drawn from the smallness of quantity of the atmospheric vapours are entirely devoid of weight .
For larger thicknesses of gas and vapour , a tube was employed , which was divided into parts capable of being used separately or together .
The mode of proceeding was this:-A brass cylinder 49'4 inches long had its two ends stopped with rock-salt ; a source of heat was attached to it exactly as in the author 's experiments described in former memoirs .
The pile and the compensating cube also occupied their old positions ; but instead of determining the absorption effected in a column of gas or vapour equal in length to the whole tube , the tube was now divided into two independent compartments by a third plate of rock-salt .
Let us call the compartment furthest from the pile the first chamber , and that nearest to the pile the second chamber .
The experiments were commenced with the first chamber very short , and the second chamber long ; and the plate of salt was subsequently shifted so as to lengthen the first chamber and shorten the second one , the sum of the lengths of both chambers being preserved constant at 49'4 inches .
The absorption effected in the first chamber acting alone was first determined ; then the absorption effected by the second chamber acting alone ; and finally , the absorption effected when both chambers were occupied by the gas or vapour was determined .
This arrange meant enabled the author to examine the influence of the sifting which occurred in the first chamber on the absorption effected by the second one .
The thermal coloration of the various gases was rendered very manifest by these experiments the heterogeneity of the obscure calorific flux being demonstrated , and the selective action of the gases on particular constituents of the flux exhibited .
A stratum of carbonic oxide 8 inches thick being placed in front of a tube containing 41'4 inches of the same gas , those 8 inches intercept 6'02 per cent. of the whole radiation ; the same 8 inches being placed behind the column 41'4 inches in length , the absorption effected is almost nil .
So with carbonic acid : 8 inches in front absorb 6'25 per cent. , while behind they absorb a scarcely measurable quantity .
Similar remarks apply to the other gases , the reason manifestly being , that when the 8-inch stratum is in front , it intercepts the main portion of the rays which give it its thermal colour , while when it is behind , these rays have been in great part withdrawn , and to the remainder the gas is transparent .
From analogous reasoning we conclude that the sum of the absorptions of the two chambers , taken separately , must always be greater than the absorption effected by a single column of gas of a length equal to the sum of the two chambers .
This conclusion is illustrated in a striking manner by the results ; and it is further found that if the mean of the sums of the absorptions of the two chambers , taken separately , be divided by the absorption of the sum , the quotient is the same for all gases .
It is also to be inferred from the foregoing considerations , that the sum of the absorptions must diminish as the two chambers become more unequal in length , and must be a maximum when they are equal .
In these days a special interest attaches to the radiation from any gas through itself , or through any other having the same period of radiation .
The author records the results of an elaborate series of experiments on this point .
The experimental tube , 49*4 inches long , was divided into two compartments by a partition of rock-salt .
The compartment nearest to the pile was filled with the gas which was to act as absorber , while the chamber most distant from the pile contained the gas which was to act as radiator .
This latter gas was warmed by the destruction of its own vis viva within the chamber .
The radiation was what the author has called dynamic radiation .
The lengths of two chambers were varied , the radiating column being lengthened , and the absorbing one shortened at the same time .
The experiments were carried out with a considerable number of gases and vapours .
The experiments with the vapours were thus executed .
First , the chamber nearest the pile was occupied by vapour of a certain pressure ; the other chamber was then occupied by the same vapour at the same pressure .
The entrance of the vapour was so slow , and its quantity was so small , that the dynamic radiation due to the destruction of its own vis viva was almost insensible .
The needle being at zero , dry air was allowed to enter the chamber most distant from the pile ; the air became heated , communicated its heat to the vapour , and the latter radiated it against the pile .
It is quite evident that not only does this case resemble , but it is of the same mechanical nature as that in which a vibrating tuning-fork is brought into contact with a surface of some extent .
The fork , which a moment before was inaudible , becomes at once a copious source of sound ; it communicates its motion to a body of sufficient dimensions to transmit it in large quantities to the air .
What the sounding-board is to the tuning-fork , the vibrating compound molecule is to the elementary atom .
The tuning-fork swinging alone is in the condition of the elementary atom radiating alone , the sound of the one and the heat of the other being insensible ; but in association with the particles of acetic or sulphuric ether , the elementary atom is in the condition of the tuning-fork applied to its sound-board , communicating through the molecule motion to the luminiferous ether , as the fork through the board communicates it to the air .
These experiments show the great opacity of a gas to radiations from the same gas .
They also show , in a very interesting manner , the influence of attenuation in the case of the vapours .
The individual molecules of a vapour may be powerful absorbers and radiators , but in thin strata they may constitute an open sieve , through which a large quantity of radiant heat may pass .
In such thin strata , therefore , the vapours , as used in the experiments , were generally found less energetic than the gases , while in thick strata the same vapours showed an energy greatly superior to the same gases .
A few striking results are recorded by the author in illustration of the influence of a lining within the experimental tube on the radiation .
A ring of blackened paper , for example , not more than 11 inch in width , placed within a polished brass tube , radiated , when dry air was permitted to enter the tube , a quantity of heat sufficient to urge the needle of the galvanometer through an arc of 56 ?
; while , when the ring was removed , the radiation from the whole surface of the tube produced a deflection of only 7 ?
'5 .
The author finally examines the diathermancy of the liquids from which the vapours made use of in his experiments were derived ; and the result leaves no shadow of doubt upon the mind , that if any vapour be a strong absorber , the liquid of that vapour is also a strong absorber .
The phenomenon is one in which the individual molecules are implicated , the molecule carrying its power as a radiant and an absorbent through all its states of aggregation .
The order of absorption in liquids and vapours is precisely the same .
These facts revive thoughts regarding the connexion between radiation and conduction , to which the author has already given expression .
In a future memoir he hopes to throw additional light on this important subject .
|
112341 | 3701662 | Account of Observations of Atmospheric Electricity Taken at Windsor, Nova Scotia | 683 | 707 | 1,862 | 12 | Proceedings of the Royal Society of London | Joseph D. Everett | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0152 | null | proceedings | 1,860 | 1,850 | 1,800 | 25 | 649 | 10,292 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112341 | 10.1098/rspl.1862.0152 | http://www.jstor.org/stable/112341 | null | null | Meteorology | 55.374682 | Electricity | 19.116162 | Meteorology | [
36.99692916870117,
2.4902734756469727
] | XXI .
" Account of Observations of Atmospheric Electricity taken at Windsor , Nova Scotia .
" By JOSEPH D. EVERETT , M.A. , F.R.S.E. , Professor of Mathematics , &c. in King 's College , Nova Scotia .
Communicated by Professor WILLIAM THOMSON .
Received June 18 , 1863 .
1 .
The observations here described were taken at my house , which is on the College hill , Windsor , in latitude 44§ 5S ' 34 " N. , and longitude 64§ 8 ' 30 " E. They were taken at a landing-window looking N.E. , whose sill is 27 feet above the ground .
There is a very clear view from the window , and no trees , buildings , or other obstacles to screen it from the fill effect of atmospheric electricity .
The ground slopes away on the N.E. , E. , S.E. , and S. , and is nearly level in other directions , rising slightly , however , for the first 20 yards on the N.W. The surrounding country is undulating , with the exception of a stretch of flat alluvial soil which runs past the base of the College hill , and to which the ground slopes away from 683 1863 .
] my house in the directions above indicated , the fall amounting to from 60 to 70 feet .
The flat in question connects the two rivers Avon and St. Croix , which unite just below Windsor , and is scarcely , if at all , above high-water mark , being protected from inundation by dykes .
The view from my house is bounded in the distance on all sides by ranges of thickly wooded hills , whose average height is about 500 feet , and nearest distance about three miles .
2 .
The apparatus used for collecting the electricity of the air was Professor Thomson 's water-dropping collector , which consists of an insulated can of copper , having a brass pipe leading from it , through which the water can be discharged by turning a tap .
The can stands upon a shelf just inside the window , and the pipe projects through a hole 14 inch in diameter in a board which is inserted under the lower sash of the window .
The pipe extends nearly horizontally outside the window to the distance of 3 feet 6 inches from the sill ; and the water , when turned on , flows from the end in a stream so finle , that two or three hours are required to discharge a pailful of water .
The end of the pipe is about level with the sill of the window .
It is assumed that the effect of the stream of water flowing from the pipe is to reduce the pipe and can to the same electrical potential as the air at the place where the water breaks into drops .
The time required to reduce the can to the potential of the air is not more than a minute .
In my earlier observations I observed the electricity of the air as soon as I could after turning on the water ; but in looking over my observation-book , I found the electricity recorded was uniformly weaker at the first observation than at the second , taken about a minute later .
In my later observations I always allowed a full minute .
3 .
In the commencement of winter the frost interfered with the system of water-dropping .
I first tried to obviate the difficulty by leaving the water running ; but a little always remained in the pipe after the can was emptied , and by freezing burst the pipe .
I then shortened the pipe by removing some joints of it .
This prevented the bursting of the pipe , the remaining portion being of stouter material than that removed ; and I continued to take observations , with the pipe thus shortened , from Nov. 17th to Dec. 2nd ; but as the weather grew colder , the water froze in that portion of the pipe which was inside the window ; and after thawing it on two or three 684 [ June 18 occasions by the heat of a spirit-lamp , I determined to dispense , if possible , with water-dropping , and collect the electricity of the air by a burning match .
Accordingly , from Dec. 2nd to March 30th I employed matches such as are used with Professor Thomson 's Portable Electrometer ( consisting of rolls of blotting-paper prepared with nitrate of lead ) , the burning match being fixed on the end of the water-dropping pipe .
The effect of shortening the pipe is to weaken the electricity collected , in a constant ratio , which I have ascertained , by observations taken alternately with the pipe shortened and restored to its full length , to be about 1 to 3-1 .
This difference has been allowed for in reducing the observations , as it was very desirable to furnish my tabulated results in a form easily admitting of comparison by inspection .
I have , nevertheless , inserted the letter S in the column " Remarks " against all observations taken with pipe shortened .
I have in like manner compared , by alternate observations , the results obtained respectively by water-dropping and burning match , and my observations lead to the inference that the results obtained by both methods are the same .
The letters M and W , when they occur in the column " Remarks , " denote respectively that the observations against which they stand were taken with burning match and water-dropping .
( See Table IV .
) 4 .
For testing and measuring the electricity thus collected I have used the " Station Electrometer , " except in a few cases , when I have employed the " Portable Electrometer .
" Both instruments are inventions of Professor Thomson .
The former consists of a Leyden jar , having within it a needle of aluminum suspended by a glass fibre , and connected ( by platinum wires dipping in sulphuric acid ) with the inner coating of the jar .
In the neighbourhood of the needle are two brass plates , also connected with the inner coating of the jar , called the " repelling plates , " because their function is to repel the two ends of the needle , causing it to rotate , and thereby twist the glass fibre .
A brass cage surrounds both the needle and the repelling plates .
It hangs from glass pillars , which insulate it from the jar ( and therefore also from needle and repelling plates ) ; and an arm of brass attached to it projects through a hole to the outside of the jar , furnishing the means of connecting the cage with the object to be tested .
This projecting arm is surrounded by a hollow cylinder of pumice soaked in sulphuric acid , for the purpose of drying the air which enters the jar , and thus preserving insulation .
The insulation thus obtained is so good that the jar loses , on the average , only 2 or 3 per cent. per diem .
5 .
The force of repulsion between the needle and the repelling plates depends not on the potential of the jar absolutely , but on the difference between this and the potential of the cage , being for any given position of the needle proportional to the square of the difference of potentials .
In taking an observation , the force of repulsion is ascertained by applying torsion to the glass fibre until the near end of the needle is brought into a line between two sights , one of which is on the plate of glass which covers the jar , and the other on the bottom of the cage .
The amount of torsion applied is read off , and is assumed to measure the force of repulsion in the sighted position of the needle ; hence the square root of the number of degrees of torsion measures the difference between the potential of the inner coating of the jar and the potential of the cage ( the latter being the same as that of the body tested ) in terms of a unit which is constant for any one electrometer .
In accordance with a convention which has been adopted by Professor Thomson , I have always multiplied the degrees of torsion by 10 before extracting the square root .
Thus , if E denote the number of degrees of torsion required to bring the needle to the sights when the cage is connected with the earth , and A the number required when the cage is connected with a conductor to be tested , the potential of the inner coating of the jar will be V/ 10 E , and the potential of the conductor tested will be V/ 10 A ; hence the potential of the body tested will be V/ lOEl'10 A. It is by this last formula that the numbers under the heading " Electricity of Air " in my tabulated results have been calculated .
If A is greater than E , the formula still holds , and the negative sign indicates that the electricity of the conductor tested is of opposite kind to that with which the jar is charged .
E is called the earthreading , and A the air-reading .
6 .
The portable electrometer , which is more convenient for use when the electricity of the air is very strong , also contains a needle and repelling plates , surrounded by a cage which is insulated from them , the whole being enclosed in a Leyden jar ; but the needle , 686 [ June 18 , instead of hanging freely by a glass fibre , is attached to the middle of a fine wire of platinum , whose two ends are secured in such a manner as to keep it always tight .
The needle and repelling plates are put in connexion with the body to be tested , the cage being connected with the inner coating of the jar , an arrangement which , though opposite to that adopted in the Station Electrometer , requires the same formula to be applied in reducing the readings .
7 .
The best possible test of the accuracy of the method of reduction above described is to observe the potential of the same conductor with two electrometers , and try whether their indications ( thus reduced ) differ in a constant ratio when the charges of their jars are varied .
I have applied this test , giving charges of different strength , sometimes of the same kind and sometimes of opposite kinds , the conductor tested being a short wire of copper or brass connecting the electrodes of the two instruments .
These experiments were performed for the purpose of ascertaining the ratio in question , with the view of reducing all my observations to a common standard ; and I have also investigated this ratio by connecting the jars of the two instruments , and taking earth-readings ; but this method is less convenient because it involves the admission of undried air into the jars , thus impairing insulation , and rendering accurate observation difficult ; whereas in the former method of observing , if performed in favourable weather , the insulation is as good as perfect .
As it is important to establish practically the accuracy of the method of reduction pursued , I give in extenso all the comparisons that I have made by the methods just described .
8 .
In using the Station Electrometer , I have given a fresh charge to its Leyden jar about once a week : when charged too highly , it is not sufficiently retentive ; when not high enough , the instrument is not sufficiently sensitive .
With a charge of fifty units , which is my average working charge , a difference of 1 ?
in the angle of torsion is equivalent to 1 of a unit of charge , so that if the difference between air-reading and earth-reading is 1 ?
, the strength of atmospheric electricity is 1 .
The average strength of atmospheric electricity observed has been from thirty to forty times greater than this , and has in a few cases been 800 times greater .
Hence it is obvious that readings to whole degrees are abundantly sufficient ; and I have not thought it necessary to aim at greater minuteness , more especially 3c as the variation generally amounts to two or three degrees every minute .
9 .
Of late each observation has consisted of an earth-reading , followed by five air-readings , taken at intervals of a minute .
During the first three months of observation the number of consecutive readings was irregular , and the interval between them was not always the same .
The loss of charge in ten minutes is practically insensible , and is sometimes more than counterbalanced by changes in the zero of torsion produced by the strain upon the fibre during the observation .
The only case in which any considerable loss occurs is when the electricity of the air is very strong negative ( that of the jar being positive ) , causing a very high air-reading .
The jar holds very well when the reading is 360 ?
( corresponding to 60 units ) ; and I generally give it a charge of about this amount , renewing it when it has fallen a little below 250 ?
( or 50 units ) .
10 .
The Station Electrometer stands on the shelf at the distance of about a foot from the can .
In taking earth-readings , the electrode is connected with one of the brass foot-screws which support the instrument , the connexion being made by a brass wire .
In taking air-readings , the electrode is connected with the can by means of a copper wire .
The square roots are generally taken on the spot by a table which serves for all whole degrees from 0 ?
to two revolutions .
11 .
The Station Electrometer has never been removed from its place except during very cold weather , when the sulphuric acid at the bottom of the jar sometimes became frozen over , so that the needle was prevented from turning ; and it was necessary to remove the instrument to a warm room , sometimes to thaw the ice , and sometimes to prevent it from freezing .
The ice in question is , I am informed , not frozen water , but a definite compound of sulphuric acid and water .
It was most liable to form when the acid had been for a long time unchanged , but I have seen a little of it when the acid had been less than a week in the jar .
It never formed unless the temperature of the instrument was as low as about 20 ? .
12 .
On the first occasion of its formation , being taken by surprise , and not using proper precautions , I broke the glass fibre which supported the needle : this was on the 3rd of December .
A new fibre was put in-on the 6th , and the sights were adjusted to suit the new fibre on the 8th , the observations of atmospheric electricity being 688 taken with the Portable Electrometer in the meantime .
On several subsequent occasions the Portable Electrometer was used in consequence of ice having formed in the Station Electrometer .
On all other occasions the observations have been taken with the Station Electrometer , except when the electricity was too strong or too variable to be conveniently measured by it .
On one occasion , in the first month of the observations ( Oct. 22nd ) , in showery weather , the earth-reading being one revolution and 19 ?
, the negative electricity of the air was so strong that six revolutions were not nearly sufficient to bring the needle to the sight .
Electricity of such strength is very common during showers either of rain , hail , or snow , being always positive during snow , generally negative during hail , and generally negative ( in some instances alternating with positive ) during heavy rain .
On such occasions I have generally had recourse to the " Portable , " which is less sensitive .
13 .
On some occasions , when the electricity of the air has been strong , it has been so violent in its fluctuations from second to second , that the needle of the " Station " was quite unmanageable from the extent and rapidity of its vibrations .
On such occasions , which are denoted by the word " vibration " in the column " Remarks , " I had recourse to the Portable Electrometer , whose needle , in the same state of the atmosphere , frequently exhibited no vibration .
Sometimes , however , the needle of the " Portable " has been violently agitated , and on these occasions , which only occurred when the electricity observed was very strong and of opposite kind to that in the jar , I have always found that the jar was discharging .
On a few occasions , especially on the 6th and 7th of January , the needle of the " Station , " though not trembling as in the cases above alluded to , has been remarkably unsteady , the air-reading changing by several degrees every two or three seconds .
14 .
In the Table of Comparisons of Electrometers , " Station I. " denotes the Station Electrometer with its first fibre ; " Station II .
" denotes the Station Electrometer with its second fibre ; and " Portable " denotes the Portable Electrometer .
The most probable values of the ratios of their indications , as shown by their comparisons , may be assumed to bePortable : Station I. : : 1 : 85 Portable : Station II.:::3 1 Hence Station I. : Station II .
: : 1 : 365 .
1863 .
] 689 If we assume , from the comparisons of long and short pipe , that Short pipe : Long pipe : : 1 : 3'1 , we have Station I. with short : Station II .
with long : 1 : 1 13 Portable with short : Station II .
with long : : 1 : 9'6 .
All the numbers in my tabulated results are given in terms of Station II .
with long pipe , and the reductions have been effected by means of a Traverse Table to single degrees on the following assumptions : Station I : Station II .
: : Distance : Departure for 22 ?
Portable : Station II .
: : Distance : 10 x Departure for 18 ?
with sort with long : : Diff. Lat. : Dist .
for 29 ?
with shortJ * with long of Portable jf Station II .
1h shorta : with ong , : : Dist .
: 10 x Diff. Lat. for 21 ? .
I with shortJ with long These ratios , when stated in numbers , are respectively 1 : -375 , 1 : 3-09 , 1 : 1-14 , 1 : 934 ; whereas those above , designated as most probable , are 1 : 365 , 1:3'1 , 1 : 1'13 , 1 : 96 .
15 .
The cage of the Station Electrometer was taken out and replaced on January 13th and April 10th , an operation which involves a readjustment of the repelling plates , and may thus affect the sensitiveness of the instrument .
On the latter occasion a slight change was also made in the position of the upper sight , tending to render the instrument rather less sensitive ; but I do not think the effects of these changes have been sufficiently great to be worth taking into account .
One at least of the electrometers seems to be affected by some uncertain disturbing cause , which renders it more sensitive on some days than on others .
This is well exemplified by the comparisons of January 14th and January 19th , the mean results obtained on the two days respectively differing by 8 per cent. Even on the same day results obtained with different charges do not precisely agree , and the discrepancies are much greater than could arise from errors of reading .
They do not follow any easily ascertained law ; and I am inclined to attribute them to imperfect elasticity in one or both of the fibres-a cause which may also have produced discrepancies between results on different days , for the zero of torsion has nqt always been tested when the comparisons were made ; and 690 [ June 18 , as the instruments have been left standing with different amounts of torsion on the fibres at different times , the zero of torsion may have changed .
This cause would principally affect the Portable Electrometer , whose zero of torsion has always been assumed to be 30 ?
, except on May 2nd , when it was very carefully tested , and found to be 30 ?
'1 .
The zero of torsion for the Station Electrometer has been so frequently tested , that no sensible correction can be needed for it beyond what has been made .
That the Portable Electrometer is affected by some such disturbing cause will be seen by reference to the comparisons on February 1 1th , where the earth-readings of the " Portable " are 51'0 , 51'8 , 51 2 , the increase from the first reading to the second apparently depending on the increased torsion which was applied in the interim , and the subsequent fall being assisted by the diminution which was made in the torsion between the second reading and the third .
The " Portable " also seems to hang a little ( see comparisons on November 4th ) .
16 .
Besides errors from want of exactness in reducing all the observations , except those taken with Station II .
, to units of that instrument , and those arising from changes in the Electrometers themselves , it is probable that others have been produced by circumstances affecting the collection of the electricity from the air , the place where the water-stream breaks into drops being subject to small variations , depending on the wind and the head of water in the can .
In like manner , when burning matches are used , the place where the smoke breaks away depends upon the wind and the length of the match , the latter being sometimes six and sometimes only three inches at the commencement of an observation .
Rain or snow falling on the pipe has also doubtless a disturbing effect , equivalen to a shortening of the pipe ; but the effect cannot be great ; for I have tested that during a shower of rain , when the water in the can was not allowed to flow out , a strong artificial charge given to the can and pipe , though of the opposite kind to that of the rain , was dissipated with extreme slowness ; but when the water was turned on and a fresh charge given , the loss was extremely rapid-say thirty times as fast as before .
This observation has been confirmed by observing that even when the electricity of the air during heavy snow or rain was excessively strong , as collected by water-dropping , very feeble indications were obtained if the water was turned off .
It is s1863 .
] 691 obvious that the law of distribution of electricity on the surface of a conductor gives the end of the pipe a great advantage over other portions of it as regards power of collecting electricity from the air .
Notwithstanding that the tendency of rain or other downfall is to make the electricity appear weaker than it really is , by virtually shortening the pipe , the observed electricity is generally much stronger during heavy showers than at any other time .
17 .
The errors resulting from these various causes , though not insignificant in themselves , are very small in comparison with the variations which really occur in the electrical potential of the air , as will be seen by the most cursory glance at the tabulated observations .
18 .
My observations have generally been taken regularly at three stated times in the day , viz. , between 8 and 9 A.M. , between 2 and 22 P.M. , and between 9 and 9 P.M. ; and in many instances observations have been taken at other hours as well .
On Sundays some of the observations have generally been omitted .
Either during or immediately before or after each electrical observation , I have also observed barometer , dryand wet-bulb thermometer , cloud , wind , and state of weather generally .
The barometer used is an Aneroid of the usual size , nearly new and in good condition .
I have ascertained , by experiment , that it is affected by temperature , the disturbance being in the same direction as for a mercurial barometer .
It has also an index error of about *06 , reading too low by this amount ; but I have not applied any correction for either cause ; and it would scarcely be worth while to do so , as very little connexion appears to exist between the fluctuations of the barometer and those of atmospheric electricity .
19 .
My two thermometers ( dryand wet-bulb ) are mercurial with unusually long degrees .
They are placed outside the window of a room in the second story , in which there is never any fire ; and are read through the window , from which they are about six inches distant .
The window faces the north-west , and the thermometers are well protected from radiation except from the window , while at the same time exposed to a free current of air .
I have carefully tested the thermometers in melting snow , which showed that at 32 ?
the dry-bulb read *4 too high , and the wet-bulb *7 too high .
I have also tested them in water at various tempera[June 18 , 69 tures beside a thermometer which has been tested at Kew Observatory ; and as the errors at other points of the scale were found not to differ much from those at 32 ?
, I have applied a uniform correction of 4 to the readings of the dry-bulb , and of --7 to those of the wet-bulb .
In the tabulated observations 1 have entered the corrected reading of the dry-bulb thermometer , and the corrected difference between dry and wet .
My observations of cloud are recorded in the usual way , the figure in the column " Amount " denoting the number of tenths of the sky that are covered with cloud .
In the column " Kind " the abbreviations ci .
, cu .
, st. , nim .
, are used to denote cirrus , cumulus , stratus , nimbus .
The direction of the wind has been inferred from observations of smoke and clouds , or from other obvious sources .
The force of the wind has generally been set down by estimation , 1 denoting a light breath , 2a moderate wind , 3a rather high wind , 4a gale , 5a violent gale .
Where the velocity is given in inches per hour in the column " Remarks , " it has been observed with a hemispherical cupanemometer .
20 .
The entries of electricity are in three columns .
The first contains the mean of all the observations which compose the group , these observations being generally taken at intervals of a minute ; the second column contains the highest potential observed ( that is , the strongest positive or the weakest negative ) ; and the third column contains the lowest potential observed ( that is , the strongest negative or weakest positive ) .
When a greater number of observations have been taken consecutively , they have been broken up into groups ; and in grouping I have been careful , as far as practicable , to avoid including positive and negative in the same group ; but sometimes , when the electricity was weak and oscillating , I have allowed them to enter the same group ; and in these instances I have obtained the mean by dividing the algebraic sum by the number of observations .
As regards the number of observations to be combined in one group , my arrangement has been somewhat irregular , depending generally on convenience as regards the pages of my observation-book .
The time entered corresponds nearly to the centre of each group .
It is sometimes given in hours and quarters , sometimes in hours and minutes .
1863 .
] 693 21 .
For the sake of showing the variations of atmospheric electricity from minute to minute , I subjoin all the observations taken on the 10th day of each month , from October to March .
With the exception of the evening of February 10th , these are fair samples of ordinary observations .
I also subjoin the observations which were taken on the 26th of November , as a specimen of very great and rapid changes in atmospheric electricity .
In all these instances the electrical potential of the air is given in units of the electrometer with which it was observed .
The readings of dry and wet bulb are also given without correction .
( See Table I. ) 22 .
I also subjoin Tables of all the observations ( or rather the mean highest and lowest of each group ) taken during rain , snow , hail , sleet , and fog .
These numbers are merely copied from the complete Table of observations already given , and thus collected for greater convenience of reference .
( See Table II .
) It will be observed that the electricity found is almost invariably positive during snow .
Out of 25 days on which observations were taken during snow , there were 23 on which positive electricity only was observed , on the remaining 2 days both positive and negative being observed .
Of 28 days on which observations were taken during rain , there were 9 on which positive only was observed , 7 on which negative only , and 12 on which both kinds were observed .
There were only 2 days on which observations were taken during hail , and on both of these both kinds of electricity were observed , but with a great preponderance of negative .
On 2 days observations were taken during sleet .
In one instance the electricity found was positive , and in the other it changed from weak positive to weak negative .
On 5 days observations have been taken during fog , and the electricity found was always positive , generally much above the average strength .
Light rain , unless accompanied by mist , has never shown strong electricity ; but heavy rain , as also moderate rain with mist , is in the majority of instances marked by very strong electricity .
I have not been able to ascertain , by inspection , any connexion between the direction of the wind during rain and the accompanying electricity .
694 [ June 18 , 23 .
Altogether there are 20 days ( out of about 170 ) on which negative electricity has been observed ; but on every one of these days positive electricity was observed also .
With the exceptions of December 10th and 19th , negative electricity has only been observed either during downfall ( i. e. rain , hail , sleet , or snow ) or immediately before or after it .
In these two exceptional instances the sky was entirely covered with nimbi , and the negative electricity observed was weak .
In the latter the observation was taken about 9 P.M. ; and the next following observation , taken between 8 and 9 A.M. the next morning , showed positive electricity of unusual strength .
There are only 2 days ( February 4th and March 14th ) on which the strength of electricity , when there was no downfall or fog , has been as high as 10 , and on these two occasions the temperature of the air was below zero .
The average strength of electricity , giving equal weight to all observations , and excepting those taken during downfall or fog , has been 4'2 or 4'3 , the averages for the respective months being-Oct .
3-3 , Nov. 3*1 , Dec. 4-0 , Jan. 4'2 , Feb. 5'6 , March 5-5 .
24 .
With the view of investigating the diurnal range of atmospheric electricity , I have added , for each month , all observations taken during the same hour , and have divided the sums by the numbers of observations .
By " observations " I mean , here and during the remainder of this section , the numbers representing the mean electrical potential for each group of readings , as entered in the complete tabular statement already given , except when there are two or more such entries for the same hour , in which case their arithmetical mean has been adopted and reckoned merely as one observation .
Again , dividing the day into three portions-before noon , noon to 6 P.M. , and after 6 P.M. , -I have divided the sum of all observations taken in the same portion of the day , for each month , by the number of observations ; and I have , in the same manner , found the mean potential " at all hours " by dividing the sum of all observations taken during a month by the number of observations .
It will be seen that for every month of the six the electricity is weaker after 6 P , M. than in either of the previous portions of the day .
( See Table III .
) 25 .
The average potential at each hour for the 6 months may be found either ( 1 ) by dividing the sum of all observations taken at the 1863 .
] 695 same hour during the 6 months by the number of observations , or ( 2 ) by taking the arithmetical means of the monthly means .
Whichever method be adopted , the results for some of the hours will , from paucity of observations , be liable to much uncertainty .
As a check upon results obtained by these two methods , and to remove errors arising from the greater average strength of electricity in some months than in others , I have ( 3 ) divided the sum of observations at each hour for each month by the mean of observations " at all hours " for that month , and , after adding the corresponding sums for the 6 months , have divided by the number of observations .
This method of reduction I conceive to be the fairest of the three , as it amounts to multiplying each observation by a factor inversely proportional to the mean electrical potential for the month in which it is taken .
It gives the mean potential at each hour , supposing the general mean derived from observations at all hours to be unity .
The means obtained in this way are headed " Reduced Means " in the annexed Table of Diurnal Range , those obtained by the other two methods being given in the two preceding columns .
All three methods agree in furnishing the following results:1 .
That between 7 and 8 A.M. the strength of electricity is below the mean .
2 .
That between 8 and 9 A.M. its strength is above the mean , and takes a very decided maximum .
3 .
There is apparently a minimum between 10 and 11 A.M. ; but observations are few .
4 .
That from 1 to 7 P.M. the strength is above the mean , with the apparent exception of the hour 4-5 .
5 .
That from 7 P.M. to midnight the strength is below the mean .
The mean here referred to is the mean of all observations , and is probably not the true mean value for the 24 hours .
[ Subjoined is a selection from the Tables which accompany the Paper ; the complete series is preserved in the Archives of the Royal Society .
] 696 [ June 18 , TABLE I.-Extracts from the Observations .
October io , i86z .
November io , I862 .
Station Electrometer with first fibre .
Portable Electrometer .
Electricity .
Remarks .
Electricity .
Remarks .
Dry bulb , 56 Wet bulb , 48 Sky nearly covered with cirro-cumuli ; bright , but not sunshine .
Dry bulb , 57 Wet bulb , 50 Dry bulb , 55'5 Wet bulb , 48'5 Very cloudy and dark , notwithstanding full moon .
Dry bulb , 53 Wet bulb , 484 Still very dark .
Dry bulb , 52 Wet bulb , 48 Sky entirely clouded , but light ; moon just visible behind clouds .
h. m. 7 49 A.M. 49§ 50 52 521 53 54 55 56 57 58 59 8oI12 8'42 A.M. 43 2 14 P.M. 15 3 48 49 9'7 -6'9 --4'7 5 .
' 5'9 5'4 -9'3 --0 ' -+.3 -0'7 +0'8 +0-8 +o-7 +o'S +0'2 +06 +0'7 +0'3 +0'3 Bar .
29*43 Dry , 40'5 Wet , 39'0 Overcast , nimbi , cumuli , and blue sky .
W.S.W. I Clearing up .
Bar .
29'45 Dry , 39-6 Wet , 37-8 Heavy cum .
, nim .
, and blue sky .
Bar .
29'47 Dry , 38'9 Wet , 36-8 Bar .
29-58 Dry , 37-2 Wet , 34-1 Station Electrometer .
3 54 55 55i 56 93 P.M. +2 ' +2-8 +2'7 +2'4 Overcast .
W. 2 Bar .
296 I Dry , 36'7 Wet , 33-4 Snowing lightly .
N.W. I Bar .
29'72 Dry , 33-2 Wet , 32'3 Much rain , with wind , during the night .
1863 .
] h. m. 9 38 A.M. 39 40 41 43 44 45 10 I A.M. 34525 r.M. 7 11 I 12 13 14 16 17 18 i8 I9 20 21 23 24 6 55 P.M. 56 57 59 7I8 47 P.M. 49 52 o0 38 P.M. 40 41 42 43 46 + 7-9 + 8-8 + 9'4 +10-1 + 8-6 + 2'2 + II'0 + 6'3 + 7'I + 9'2 + 8'7 +1 '5 + 13'3 + I4'o +I6'I +13'4 +1I4'9 + i6'i + 15 ' +15-8 + 14'4 +I4'I + 4'x + 5'z + 5'7 + 6-i + 5'7 + 6-x + 76 + 7-7 + 7'3 + 4'5 + 5'5 + 6-6 + 7'5 + 8- ' + 6-o TABLE I. ( continued ) .
[ June 18 , December I0 , I862 .
January Io , 1863 .
Station Electrometer with second fibre .
Station Electrometer with second fibre .
Electricity .
Remarks .
Electricity.t Remarks .
10 nim .
, &c. Calm .
Bar .
29-96 Dry , 28-6 Wet , 27-2 A little snow has fallen during the night .
9 nim .
I S.W. Bar , 29g90 Dry , 32'6 Wet , 29'7 January io , 1863 .
Station Electrometer with second fibre .
4 cum .
and ci.cum .
, calm .
Bar .
30'45 Dry , Io'o Wet , 9'4 b. m. I 47 P.M. 472 48 49 50 54 I6 P.M. 15 17 18 I9 95 P.M. 16 17 18 20 21 22 23 +2'9 +2'9 +23-8 +2-8 +3-3 +3-8 +3'3 +3'4 +2'9 +2'6 +2'9 +2'7 +2'9 +2-8 +2'5 +2.1 +2*1 Bar .
30-38 Dry , 23'9 Wet , zI-0 9 str .
IWo str .
and ci.-cum .
Calm .
Bar .
30'36 Dry , 22*0 Wet , 20'3 io cloud .
I S. Bar .
30oI7 Dry , 27'0 Wet , 25'3 February so , I863 .
Station Electrometer with second fibre 85 A.M. 52 53 54 55 56 29 P.M. 10 II 12 13 14 I5 I6 +24o'0 +23'5 +25'7 +-30 ' +32-1 3I 4+ 1'7 + " 7 + 1'3 + 1'3 + I'5 + I'6 + 2'2 + 2'6 Snowing fast .
Calm .
Bar .
29-86 Dry , 27-8 Wet , 27'4 Not snowing .
10 mm. Io nim .
( snow-clouds .
) Calm .
Bar .
29'46 Dry , 39-I Wet , 38'6 Portable Electrometer .
About Ioh .
56m .
P.M. the mean of five minutes ' observation was +27'0 , the highest observed being above +30'0 , and the lowest being +z24 ' .
h. m. 7 57 A.M. 58 59 8oI251 P.M 52 53 54 55 56 57 9I P.M. 23456789 I0 +1 I --0'2 o7 --O'I +3'0 +3'5 +4'0 +3'7 + 3'4 +3*3 +2'9 +2-9 +2'9 +2-9 +3'0 +3'0 +2'8 +2'5 -+z2 +Z-8 8 21 A.M. 22 23 24 25 26 27 28 29 II 50 51 51 52I2 53 531 +6*i +7-5 +7-3 +6'7 +6.8 +7'I -47'I +7'3 +7'3 +2'8 +3'4 +3'5 +3'7 +3"9 +4'2 +3.8 4-j 3 . ?
TABLE I. ( continued ) .
February o , x863 .
Station Electrometer with second fibre .
Before and after the observation I drew sparks in abundance from the can .
The electricity was extremely rapid in its variations during the observation .
The mean was set down from estimation , only the mean , highest , and lowest being recorded .
Electricity .
Remarks .
h. m. 1I 15 P.M. 16 17 18 19 20 +i4'3 +-15'0 + I6-2 +xI2'8 +12-8 + 8'3 + 7'6 Bar .
29'70 Dry , 13'8 Wet , 132 ' Snowing , with violent wind ( 4 N. ) , the whole time , from ioh .
56m .
to Ih .
2om .
March xo , 1863 .
Station Electrometer with second fibre .
8 42 A.M. 43 44 45 46 47 11 44 A'M .
45 46 47 48 I 26 P.M. 27 28 29 30 9 X8 P.M. 19 20 21 22 23 24 +6'4 +7'0 +6'7 +6'3 +5'4 +5'3 +5'5 +5'3 +5.2 +5'o +44 +4'4 +3-9 +3.8 +3-7 + 3'5 +3'9 +4 " +4'3 +4'5 +4'7 +4'9 +4.6 7 cum .
and nim .
Calm .
Bar .
29'98 Dry , 25'7 Wet , 24'3 8 cum. .
I W. Bar .
30 ' Dry , 27'4 Wet , 24.2 8 cum .
I W. Bar .
30 ' Dry , 28-9 Wet , 25-2 10 nim .
at beginning of observation .
Sky almost entirely clear at end of observation .
Calm .
Bar .
30'io Dry , 20-0 Wet , I9'0 November 26 , 1862 .
Station Electrometer .
All these observations taken with short pipe .
Electricity .
Remarks .
h. m. 7 53 A 54 55 56 57 58 59 8 32 33 34 35 2 I9 r 20 21 22 23 237 24 24V 25 L.M. -5'8 5'4 --54'8 -4-8 -3 6 --3'5 3'0 -3'0 -20'2 -22'0 -22'0 -22'0 Raining steadily , but not heavily .
10 nim .
I E. Bar .
29'88 Dry , 38'0 Wet , 37'4 Rain and cloud as above .
I S.E. Bar .
29'88 Dry , 38'7 Wet , 38'I ( Thick mist .
+.M .
-123-8 calm .
+ 4'o i Bar .
29a'6 + 7'9 I Dry , 40'5 k Wet , 40oI + I4'2 Raining .
+17'2 +4I'7 +68'5 +75'6 Rain heavy ] +70I ' +70'I negative out of range , Rain still stronger heavy .
than -28'3 r. Portable Electrometer .
h. m. 2 29a P.M. 30 3 32 33 34 35 36 37 38 39 40 41 42 43 --3'6 -3'8 -3 I --3'3 3'3 -3-3 -4'0 -4-0 -4'0 -4.0 -4'0 -4.-1 -4 .
' -4'I -4'i -3'3 -2'6 1863 .
] 4 TABLE I. ( continued ) .
[ June 18 , November 26 , I862 .
November 26 , 1862 .
Portable Electrometer .
Portable Electrometer .
All these observations taken with All these observations taken with short pipe .
short pipe .
Electricity .
Remarks .
Electricity .
Remarks .
Rain beginning .
Rain heavy .
Rain lighter .
Bar .
29-62 Dry , 4I- ' Wet , 40 .
Raining .
Mist clearing up .
Mist gone .
Very heavy rain .
, t , , Heavy rain .
Very heavy rain .
Heavy rain .
Very heavy rain .
, , , dark .
Heavy rain .
h. m. 3 24 25 26 27 28 zg 29 30 4456789 +0-2 -o-9 -3'I -3'5 -3-5 --256 -5'4 -3'9 --o.4 -0-4 -o'4 --04 Wind N.W. I Heavy rain .
Very heavy rain , y )i Very heavy rain .
Bar .
29-6i Dry , 41-4 Wet , 41-6 Rather misty .
Flash of lightning and peal of thunder at 4h .
2m .
P.M. Needle trembling .
Very heavy rain .
Heavy rain .
Moderate rain .
Peal of thunder at 4h .
17m .
*6 of rain fell before 6 P.M. Station Electrometer .
9 47 P.m. +-oI Io nim .
48 +4-o 3 S.W. 49 +o03 Bar .
29'42 52 +0-3 Dry , 50-5 53+0'5 Wet , 50'0 54 +0-'5 h , m. 2 44 45 452 46 47 48 51 52 53 54 55 56 57 33 P.M. 4567 72 89 10 II 12 13 I4 '5 17 I7 18 I9 20 21 22 23 --3'4 +2z-6 +5-o +2-1 + ?
-3 + I'4 +0-6 -O ' I --o'8 -o-8 -o-8 -o-8 -o-6 -0o -2-8 -2'7 +4'5 +6-9 +6-9 +6-1 +6-9 -4'7 --8.7 87 +0-8 +6-9 --5'0 -0'2 -0'9 -2-5 --3'5 -2-6 -3 .
' -1.5 TABLE II.-Observations during Rain .
Electricity .
Mean .
Highest .
Lowest .
Remarks .
Oct. hm ii 8 II A.M. + 5'0 + 5'5 4'6 Light rain .
9 56 2'4 + 3'1 + I'6 Light rain .
13 4 21 P.M. 2'3 + 2'6 + 2'I Light rain .
7 23 + 09 +Io 0-8 Rain .
8 57 + 0-4 07 + 0-3 Rain .
14 73 A.M. 3'8 ... ... Fine rain .
9 37 + 5'3 + 5'3 + 5'z Scotch mist .
17 2 15 P.M. + 2'0 2'7 I'3 Fine rain .
10 15 + 2z6 + 3'2 + 2'I Light rain .
20 7 30 A.M. '3 o ' 2'7 Light rain .
7 52 + 62 +7'4 + 4.6 Rain and mist .
3 15 P.M. 5'2 + 0'4 --'6 Light shower .
22 I I5S + 0'2 +1ro O'I Rain .
2 45 + 3'6 + 4'I + 3'0 Mist and fine rain .
4o+ 3'9 + 5'8 + 2'6 Light rain .
23 29 P.M. 2'6 +2'9 +I'9 A few drops .
27 2 25 PM .
6'5 3'1 9'9 Heavy rain .
2 32 13 '8 io'8 -8'5 Heavy rain .
2 43 -I19'8 -I3'9 -247 Shower at end of observation .
Nov. [ and close .
63 58 P.M. '8 I'I 'o Heavyrain , gloomy , 5 31 0'9 '2 Heavy rain .
98+ 0'9 -+ o'6 Rain ceasing .
880 A.M. + 2'5 + 3'0 + I'9 Rain .
[ ingtoheavy .
" 47 + 3'0 + 3'9 + IX6 Light rain , increasII 52 + 2'5 + 4'0 + OI Rain lighter .
II 57 0'7 +05 '5 Rain lighter .
12 48 P.M. -+ '9 + 2'0 + '8 Light rain .
94+ I4 -+ 17 + I'I Light rain .
13 7 41 A.M. I-6 0 ' 2'3 Light rain .
7 48 + o8 + i-6 +o-x Light rain .
17 2 13 P.M. --20'4 -13'2 --25'0 Rain .
2 23 --20o ' -II'4 -297 Rain .
2 30 --38'5 -3 I'5 42'5 Rain .
2 36 -4I'5 -34'5 -46'1 Heavy rain .
8 42 56 4'2 7'2 Rain .
19 98 P.M. 22 4+ 0'3 5'6 Heavy rain .
[ and close ) .
20 7 37 A.M. + 4 ' +5'0 + 34 Rain ( very dark VO.,. .
3D .
TABLE II .
( continued ) .
Electricity .
Mean , Highest .
Lowest .
Remarks .
, t , ___ _ ... , - .
Nov. hm 20 95 A.M. --6 -2'4 -242 Heavy rain .
9 22 -32'0 --28'9 34'3 Ieavy rain .
95 -29'2 --276 -30'9 Heavy rain .
9 5P.M .
+ 33 3'3 5+ 3.0 Rain ; very dark .
22 2 P.M. + r8 + I'8 + 1'8 Rain .
5 37 i6 *I'4 Ig Heavy rain .
8 36 + 0'5 + 0'7 -+ o3 Heavy rain .
2,6 7 56 A.M. 4'8 3'4 66 Rain .
8 34 -24'7 --23'1 -25'2 Rain .
2 23 P. , .
+43'7 +8 64 + 4'6 Heavyrain and thick mist , changing in a minute from -8 6'4 to strong negative .
2 34 -34'7 -z89 ' 38'3 Light rain and mist .
2 42 -33'6 -24'3 -383 Not raining ; mist .
2 47 +zo'3 +24-3 + 5'6 Rain andmist .
[ up , 2 56 -iIr'9 0'9 -26'1 Rain ; mist clearing 38 +58-5 +64'4 +42'0 Very heavy rain ; mist gone .
3 10 -43'9 ... ... .
, .
Very heavy rain .
3I -8I-2 z ... ... ... Very heavy rain .
3 13 +39'5 +64-4 + 7'5 Very heavy rain .
3 x8 --2'2 1'9 -327 Very heavy rain .
3 26 -20.5 + I'9 -32'7 Very heavy rain ; dark .
A flash of lightning and peal cf thunder between these observations .
4 6 , -i6'5 09 --50'4 Heavy rain .
Apeal of thunder at 4h .
171m .
P.M. , being after the observation .
Needle agitated during the early part of observation .
Dec. Ii61 56 P.M. +4 i5 + 1'2 Mist and fine rain .
Jan. 69 15 P.M. + 3'3 + 4'2 + 2'5 Drizzle .
7 Io 30 A.M. 3'4 + o*8 -IIxx Light rain .
9 30 A.M. -23'9 -II '9 --30'4 Raining .
2 OP .
M. -13-6 -o'7 4'9 Raining .
I6 |4 15 P.Ivr .
+ I'Z + I9 o ?
'6 Raining .
11 30 6 7'7 6*-5 8'6 Raining .
TABLE II .
( continued ) , Electricity .
Mean .
Highest .
Lowest .
Remarks .
Jan. hm 29 8 15 A.M. 67 4'8 9'8 Very heavy rain .
2 15 P.M , + 2'7 + 4'7 ?
'9 Rain .
95 5'7 5'4 6-o Light rain .
Feb. 66o P.M. -30'8 -275 -36'5 Pouring rain .
7 15 -32*6 -31'2 --35'2 Pouring rain .
9 15 -z 28 -i 8'9 24'4 Pouring rain .
20 8 40 A.M. 3'i -I'2 39 Rain .
27 2 41 P.M. -20'9 -19* -24'3 Rain .
2 46 8-9 2z8 2o Rain .
2 57 +I6'4 +-215 + 2-z1 Rain .
April 55 11 P-N.M .
+ -43 + 4'6 + 3'7 Drizzle , rathermisty .
68 45 A.M. --25'7 -210 ' -33*2 Rain , rather misty .
Observations during Snow .
4o '9 I ... ... .
0'5 o ' 0'7 + 0.5 + o06 + 0'3 4I'9 + 2'3 + I'7 4o'3 + 2'7 + 3'8 +z4-8 +-31'2 + 4'0 + 6-9 + 13'I + 19'3 +-22 I+ 2-6 +18-9 + o'6 + 2-8 + 4'0 +26-0 +35'8 + 5'I + 8'2 +21'5 +3I'z + 34'3 + 3'0 +20 I+ 02 ' +2-5 + 3'4 +22.6 +30'0 + 3'4 + 6-x + 6-8 + 14'8 +I5 6+ 2'I +I8'4 Snowing lightly .
Snowing lightly .
Snowing heavily .
Snowing lightly .
Snowing .
Snowing lightly .
Snowing lightly .
Snowing fast .
Snowing fast .
Snowing .
Snowing lightly .
Snowing lightly .
A little snow .
A little snow .
Snowing lightly .
Snowing lightly .
3 D2 Nov. 10 27 Dec. I469 20 Jan. 7 12 14 hm93 P.M. IO P.M. 17a 14 2 i6 P.M. 8 44 A.M. I 53 P.M. 87 A.M. 9 25 8 13 A.M. 9 P.M. 9 13 2 30 P.M. 5030 P.M. 9 15 P.lm .
TABLE II .
( continued ) .
Electricity .
Mean Highest .
Lowest .
Remarks ... .
_ .
_ , .
_ , .
_ .
+ 7'6 +x6'4 +II'0 + 2'7 +35'0 +26'4 +27 ' 8 +83'4 +-38'3 + IO'I + 3'6 +-13'3 + 8'2 +35'7 + 4'9 + 5'2 + 8'7 +17'5 +15'6 + 7'5 + 8.8 + 7'0 + 54 + 78 + 7'3 +IZ'I + 2'7 +49'3 +30'6 +3 '4 +92'7 +46'4 -T I0'7 + 3'7 +17,6 +xI7'6 + II'2 +48-6 + 5'7 + 7'2 +10*0 +30'6 +2I'3 +13'2 + 8'I + 9'7 + 7'9 + 6-3 + 7'4 +15-6 + 9'9 + 2-6 +27'5 +23'2 +23'5 +74'2 } +-23'5 I+ 3'5 +9'5 } + 9'6 + 5 " +27'6 + 4- ' + 3'6 + 7'9 + 7'6 + 12'7 + 7'2 + 6-6 + 8-1 + 6'4 + 4'7 Positive , out of range , violent agitation of needle , sparks passJ ing spontaneously .
+-63'3 I +85'3 | +4 4 ' +35'o +-26-5 +28'7 +-20'I +29'8 +37'o +41'3 +4I'5 +42'2 +3I'7 +3I'7 +-20 8 +30-6 +40'3 +43'2 +-45'0 +28'5 +24'8 +26'5 + 8-6 +29'0 -+34'5 +39'5 +37'0 Snowing .
Snowing .
Snowing .
Snowing .
Snowing lightly .
Snowing .
Snowing fast .
Snowing , with violent N. wind .
Snowing without intermission .
Snowing & drifting .
Snowing lightly .
Snow directly after .
Snowing lightly .
Snowing lightly .
Snowing .
Snowing lightly .
Snowing lightly .
Snowing .
Snowing .
Snowing .
Snowing .
Snowing lightly .
Snowing , with stiff breeze from S.E. Snowing .
Snowing .
Snowing .
Snowing .
Snowing .
Snowing .
Snowing .
Snowing .
[ June 18 , Jan. 27 Feb. 36 I0 12 13 21 March 38 II 31 April 2hm8 30 A.M. 2 I5 P.M. 4 45 9 30 9 30 A.M. 2 15 P.M. 90 A.M. II 0 P.M. II 15 2 I3 P.M. 4 24 8 56 A.M. 8 44 A.M. 2 38 P.M. 92 A.M. 2 26 P.M. 2 29 P.M. 9 28 9 4I 5 12 P.M. 8 46 96 A.M. 2 33 P.M. 9 35 9 35 P.M. 9 43 27 P.M. 494 21 4 25 4 30 4 35 4 40 4 46 TABLE II .
( continued ) .
Electricity .
Mean .
Highest .
Lowest .
Remarks .
April hm78 19 A.M. -(29'9 ) -Io9 -(65'2 ) Snowing .
96 +57'5 +65'7 +53'5 Snowing .
9 32 +22'6 +28'7 + 6'5 Snowing .
10 5+ I'5 -+ I'6 + I'5 Snowingverylightly .
2 42 P.M. I'I 0*9 I13 Snowing lightly .
2 53 3*I + 4'7 + i-4 Snowing .
9 25 4+ 8'6 + 9'3 + 7'9 Snowing lightly .
Observations during Hail .
Nov. 72 28 P.M. +4II+ 4'5 1+ 3'5 Hail .
4 30 strong negative .
Hail .
4 56 + 3'9 + 4 ' + 3'7 Hail .
6I -13'3 ?
0 ' -20'4 Hail .
6 Io 6'2 3'4 9'9 Hail .
6 25 -io'5 22 ' -2I'O Hail .
6 4I -I 3'3 9'9 -I9'8 Hail .
6 50 7'4 5'6 9'6 Hail .
7I -I6'I 9'9 -I9'8 Hail .
78 -28'4 -25'3 -3o0'o Hail lighter .
iI 12 + I'8 + 1I9 + i-6 Hail light..March 98 47A.M .
-22'I -Io'2 -33'0 Hail .
April [ after .
88 47 A.M. 3'2 ; I'I Hail immediately Observations during Sleet .
Feb. 63 45 P.M. +54 + 7* + 4'3 Sleet .
March 9I8 P.M. +xo + I'r + o'2 Sleet .
iI 0'5 -4 o-6 Sleet .
Observations during Fog .
Nov.z8 II 7 P.M. +78 +7'9 + 7'7 Fog .
29 8 28 A.M. +-io'6 +-3'8 + 8'I Dense fog .
10 22 + 7I 7 ' I+ 7 ' 71 Dense fog .
Dec. 27 8 45 P.M. +7'I 8'3 6'i Dense fog .
Jan. 39 45 A.M. +-3'I +15'I + '7 Fog .
12 45 P.M. + x8'4 .
-I9'7 +-I6'2 Fog .
20 +I'2 +0 + o06 Mist .
5o -+I2'8 +I8'6 + 5'3 Fog .
9 15 +-20'0 +23'2 16'7 Very dense fog .
49o A.M. -+07 +-"I3 + 9'5 Fog .
2 15 P.M. +-I88 +220 +-I7'0 Fog .
50 +-24'8 +-26'2 22'3 Dense fog. .
t ~~ ... ... ... . .
, 705 TABLE III.-Diurnal Range .
October .
November .
ber .
er j January iFebruary .
March , All six months . ?
Hour .
11 '\O 6 to 7 A.M. i +2'1 ... ... 2 ' ?
+i+ '63 7to 8 13 +2'7 12 + 3 ' " 5 +2''5 3+ 4 ' 33 +3'0 +.3 " + '85 8Sto 95 +5'0 7 4-3'8 x5 -4'9 '5 + 4'7 6 +7 'o 13 +5'9 71 +5'4 +5'2 + -2 9 to 10 1 +-3'6 6 3'8 3 -3'6 93 3'6 4 +4 + 4 ' 6 +i'09 10 to I3 +33'5 +3 ' 1 +2'0 5+ 3'3 1 +4'I '+ 3'3 +3'2 + '85 II to i ... ... 3 +4'2 +2'6 + 4'o 2 +5'3 3 4'9 o +4'4 +4'2 +-o03 iz to I P.M. .
+2-5 3+ 3'8 i+6-3 -4'8 6 +4'2 +4'4 4+ '92 I to 2i +42 5 +2'7 6 6'4 7+ 5'2 2 +6'o 3 +4'4 23 +4'9 +4'8 +-'I9 2 to 3 13 +-4 ' 19 +3 ' 15 +4'5 9+ 4"'19 +5'6 8 45'2 103 +4'5 +44 4+'4 3 to 4I '3 ' 5 2'2 I +3'8 2 +I2'4. . ? .
*9 I 4'7 +5'4 +-127 4to 6 +3'0 +2'8. .
3+ 4'2 2 +5'4 4 +-53 I6 6 4+4'x +4- ' + '941 5to 65 +3'3 '. .
21+ 5.9..72 .
-4 ' o +4:7 +5 ' +I'12 6to 2 +4'4 I 5'6 *. .
4 4-4'2 ' .
' *4 .
+-4'7 8 +4'5 +4'7 +I'18 7to 83 +2-3 ... ... .
I 2'9 +6 ... .
i5 43'2 +-3'7 + '78 8to9 6 +3'0 '6 +3'0 7 3-5*51 20 +3'3 +3'6 ?
'*91 9 to Io 2 +2'4 9 +2'I 13 +2'3 20 + 3'2 22 +5'I 13 5'4 89 +3'6 +3'4 + '79 Io to II 4 +2'8 2 +2'0 II+ 2'5 I +3'8 4 +4'3 12+ 3'2 3+ '77 I to 1 , I9 +9 ... +.-4'4 3 44'7 2 +3'6 2 +4'0 '9 +3'9 +-3'7 + '87 Before noon .
33 +3'4 29 +3'5 25 +41 30 + 4'I 28 6 29 +6'3 174 4 -4'3 , Noon to 6 P.M. 27 +3'7 31 +2'9 22 +5'0 36 + 49 26 +5'8 27 +5'I 169 +4'5 After 6 P.M. 28 +2'7 'I 426 21 +-2'8 429 -j 3'4 77 -+5 ' 20 +-5'0 1434 +3'6 At all hours .
88 +3'3 78 +3- ' 68 +4 ' 0 95 4'2 8 45'6 45'5 i48 4'3 44 5 84 ' +56 76 +5-s5 486 +4'3 *Kt 0 c1-i 0C CO PTABLE IV.-Comparisons of Match and Water .
April znd , 1863 .
Snowing , z st. o0 nin .
Barom. 29'49 .
Dry , 30-7 ; Wet , 29-4 .
Match .
Ii Water.._ , 43'7 28'7 28'7 f 28-7 28'o 26-5 ) +29-0 ) 29-7 t 29-6 30-6 30 ?
1 J +40-7 43'2 1 40-5 39'5 42'5 28'72 29'80 4128 hm4 24 P.M. 242 25 251 26 4 3314 34 344 35 354 4 45 451 46 461 47 +20o-7 i8-6 20-8 20-r4 J +38-3 ) 40'3 37-2 I 34'7 34'5 +42'5 45'o 44'5 37'0 387 37-00 4-I'54 Mean for Match = '8= 33'27 .
3M ean for Water=-998 62z 3z'87o 3 April 28th , I863 .
Calm .
2 ci.-cu .
Barom. 29'74 .
Dry , 36-6 .
Wet , 34-6 .
Water .
Matoh .
hmhm7 47 A.M. +7-3 7 55 A.M. +69 48 7'4 55-2 6-8 49 7'z2 7'28 56 6-8 682 50 72 56 6-8 5I 7'3 ) 57 6-8 J80 A.M. -+-67 86 A. M. 77 7 oi 6-6 6i 7-8 i 6-3 644 7 7'9 7'96 I6-3 72 8-I 2 63 )8 8.3 J8 ii A.M. +8'4 Ix } 8-4 12 8-3 8'34 I22 8-4 13 82z Mean for Match i4 ' -=7'39 .
220 Mean for Water==2 7'3 3 1863 .
] hm4 20 P.M. 20I 21 z2I 22 4 29 P.M. 294 31 4 39 P.M. 3940 404 4 '
|
112342 | 3701662 | On the Brain of a Bushwoman; and on the Brains of Two Idiots of European Descent. [Abstract] | 708 | 713 | 1,862 | 12 | Proceedings of the Royal Society of London | John Marshall | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 6 | 98 | 2,234 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112342 | null | http://www.jstor.org/stable/112342 | null | null | Neurology | 56.451814 | Anatomy 2 | 9.642964 | Neurology | [
-88.95980834960938,
9.77625846862793
] | XXII .
" On the Brain of a Bushwoman ; and on the Brains of two Idiots of European Descent .
" By JOHN MARSHALL , F.R.S. , Surgeon to University College Hospital .
Received June 18 , 1863 .
( Abstract .
) The author having described the mode of preparation and dissection of the three brains , divides his paper into two parts , one relating to the Bushwoman and her brain , and the other to the idiots and their brains .
1 .
The Bushwoman 's brain .
The Bushwoman was aged , and about 5 feet high-unusual for her race .
The form of the cranium is a long narrow ovoid-less dolichocephalic , however , than the Negro skull ; the face is high-cheeked , and the nose very small and flattened .
The frontal sinuses are absent , and the walls of the cranium are thick-so thick that its internal capacity is less than would be expected from its outward form and size , being equal to 35 oz. av .
of water , or 60*64 cubic inches , which , for the height of the Bushwoman 's body , is decidedly , but not very small .
The actual weight of the preserved encephalon proved to be 21'77 oz. av .
, which would probably represent , as the author shows , 31*5 oz. for the weight of the recent brain enclosed in its membranes .
Allowance being made for the height of the body , this is less by 8'5 oz. than the average weight of the brains of European females of the same age , as estimated from the Tables of Dr. Boyd , published in the Philosophical Transactions for 1861 .
The cerebrum proper probably weighed , in its recent state , 27'25 oz. , the cerebellum 3*45 oz. , and the pons with the medulla oblongata *8 oz. The ratio of the cerebrum to the cerebellum was as usual , 7*7 to 1 ; that of the cerebrum to the body was probably as 1 to 52 , and that of the cerebellum to the body as 1 to 418 , instead of the usual ratios of 1 to 41 , and 1 to 328 .
An examination of the general form of the cerebrum shows that it is small , but long-defective in width , and especially in height .
Its outlines and surfaces are angular and flat instead of rounded and 708 filll .
The frontal region is very narrow , shallow , much excavated below , and compressed laterally near the entrance of the Sylvian fissure .
The parietal region is low , but prominent laterally ; the occipital region is long , but defective in height ; and the temporal region is long , but narrow .
The cerebrum overlaps the cerebellum by '5 inch , which is as great an absolute overlap as is usual in European brains , but less relatively to the length of the brain , which is very long in the Bushwoman .
The fissures , lobes , and convolutions are then described at length , and compared with those of the ordinary European brain , with those of the Hottentot Venus 's brain figured by Gratiolet , and with those of the young Chimpanzee .
It is impossible to give in an abstract even an outline of the facts recorded in this part of the paper .
The general result of the inquiry is to show that the fissures are rather more complex than in the brain of the Hottentot Venus , but much less so than in the European .
They are rather more complex on the left than on the right side of the brain .
They are widely separated from those of the Ape 's brain .
The author concludes-1 .
That all the convolutions proper to man are present , but , as compared with the European brain , are much more simple , and less marked with secondary sulci .
The greatest deficiency is in the occipital and orbital convolutions .
2 .
That the convolutions , taken generally , are rather more complex than those represented in Gratiolet 's figure of the Hottentot Venus 's brain , which may be partly due to the obliteration of details in the latter during its long period of preservation .
3 & 4 .
That the resemblance between the Bushwoman 's brain and the Hottentot Venus 's brain is sufficient to justify the conclusion that the latter was not an idiot , or a defectively developed individual ; but both brains , as compared with the European , have an infantile simplicity , characteristic partly of sex , but chiefly of race .
5 .
That the convolutions being more simple , can be more easily traced and compared on the two sides than usual , but still show abundant evidences of the asymmetry characteristic of man .
6 .
That there is a greater difference between the Bushwoman 's cerebrum and the highest Ape 's cerebrum than between it and the European cerebrum ; but a less specific difference between it and the European than between the Chimpanzee and the Orang ; and , of course , much less than between the highest and lowest Quadrumanous brains .
There is , however , less difference between the Bushwoman and the highest Ape than between the latter and the lowest Quadrumanous animal , 7 .
The general results , the author thinks , justify the expectation that characteristic differences of degree of cerebral development may hereafter be found in the several leading races of mankind .
The author then proceeds to describe the colour and relative proportions of the grey and white substance , the commissures , ventricles , and ganglionic masses .
The commissural fibres of the corpus callosum are very deficient in the Bushwoman ; and the other commissures are also small .
The body and anterior cornu of the lateral ventricle are also small ; but the posterior cornu and its contained parts are very large .
In the cerebellum , the median parts appear to be somewhat less developed than the hemispheres .
Its transverse commissural fibres are more largely developed than the same system of fibres in the European brain ; the Chimpanzee standing , in this respect , still lower .
The laminae of the cerebellum are even more numerous than in the European specimen with which the Bushwoman 's brain was compared .
The cerebellum seems to be more perfectly developed than the cerebrum .
2 .
The Idiots ' brains .
Some account is first given of the age , height , and bodily and mental condition of these idiots , one of whom was a wloman , aged forty-two years , and the other a boy of twelve .
The former was able to walk , though badly , to nurse a doll , and to say a few words ; whilst the latter could not walk , nor handle anything , nor articulate a single word .
In the idiot woman , the weight of the recent encephalon was 10 oz. 5 grs. , of which the cerebrum weighed 7'6 oz. , the cerebellum 1'95 oz. , and the pons with the medulla oblongata '42 oz. In the idiot boy , the recent encephalon weighed 8'5 oz. , the cerebrum 5'85 oz. , the cerebellum 2'25 oz. , and the pons with the medulla oblongata '4 oz. These are the two smallest idiots ' brains the weights of which have been recorded .
Calculations are then entered upon by the author to show the probable ratios , in the two cases , of the weight of the encephalon , the cerebrum , and the cerebellum to that of the body , and of the re .
lative weight of the cerebrum to the cerebellum .
The result of this inquiry is to prove that the entire encephalon was , in each case , about one-fourth of its normal proportional weight .
The cerebrum was much more defective than the cerebellum .
The idiot boy had relatively more cerebellum , and the idiot woman more cerebrum .
On studying the general form , dimensions , and relative position of the parts of the encephalon , it appears that the entire brain in the idiot woman resembled very closely , at first sight , both in its general mass and in the form of its anterior part , the brain of the Chimpanzee ; but a closer comparison shows great differences .
The cerebellum especially is of very great size , forming about one-fourth of the entire mass , and , instead of being covered by the cerebrum , has about '35 inch of it exposed posteriorly .
A detailed description is then given of the fissures , lobes , and convolutions , which are compared with those of the healthy brain and with those of the Chimpanzee .
Only the most general conclusions arrived at can here be given .
Of the lobes , the temporal are remarkably large ; the parietal seem to be next highly developed ; whilst the occipital and frontal are the smallest .
According to the author1 .
The idiots ' cerebra are not merely diminutive organs , having all the proper parts on a smaller scale , but these parts are fewer in number , less complex , and different in relative proportion and position .
2 .
Nevertheless all the primary and connecting convolutions proper to the human cerebrum are represented in the idiots , but are very remarkably simplified .
3 .
The degree to which the convolutions of those parts are developed follows the order observed in the lobes themselves .
4 .
The convolutions of the idiot woman are more developed than those of the idiot boy , except those of the parietal region .
5 .
The peculiarities in the idiots ' cerebra are due to arrest of development occurring at some period of foetal existence .
6 .
Judging from external appearances generally , it might be supposed that this period was about the latter half of the seventh month , and somewhat earlier in the boy than in the woman .
But a closer examination shows that the malformation is not due to a simple arrest occurring so late in foetal life , but commences much earlier in the parts at the base of the cerebrum , and then influences the evolution of the superficial parts of the hemispheres .
The corpora striata appear to be specially affected , and through these the whole hemispheres , but the frontal lobe especially .
The interest of this observation in a general physiological view , and especially in regard to the mental condition of idiots , is pointed out .
7 .
It is not certain whether the idiots ' brains had undergone any local evolutional change as the result of education or training .
8 .
It is certain that they had increased somewhat in size after the general cessation of evolutional changes in their form .
9 .
The idiots ' brains differ the woman 's being more developed on the whole , especially in the temporal regions .
Her mental powers were also greater .
10 .
These idiot brains are somewhat less developed than the two microcephalic cerebra figured by Leuret and Gratiolet .
11 .
The convolutions in the idiots ' brains are more simple than those of the higher Apes , and approach , in this respect , those of still lower Quadrumana .
But the points of difference between the idiots ' brains and those of the Quadrumana are very decided , They are human cerebra , although so imperfectly developed .
They show a general conformity to the cerebral plan of the Primates generally ; but already they manifest special human characters .
In regard to the internal structure of the cerebrum and cerebellum , many facts are noticed .
The commissural fibres of the corpus callosum are very imperfectly developed .
The lateral ventricles and their contents generally are fairly developed ; but the corpora striata are very small .
The cerebellum is well developed in all its parts in both idiots , but is not perfectly so in either .
It is larger in the idiot boy ; but the transverse commissural fibres are much less developed in him than in the woman .
In accordance with Malacarne 's statements , the laminae are fewer in number in both idiots ' brains than in the perfect brain .
The cerebellum is not merely larger , but much more developed in its form than the cerebrum , and it certainly continued to be developed to a much later period .
In a postscript-note , dated August 6th , 1863 , the author gives an account of the examination of two idiots ' brains preserved in the museum of St. Bartholomew 's HIospital , and also of a series of wax models of foetal brains in the museum of Guy 's Hospital .
The result of the additional information so obtained is entirely to confirm the descriptions and explanations given of the structure and mode of formation of the idiot brain ,
|
112343 | 3701662 | On Mauve or Aniline-Purple. [Abstract] | 713 | 715 | 1,862 | 12 | Proceedings of the Royal Society of London | W. H. Perkin | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 52 | 1,040 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112343 | null | http://www.jstor.org/stable/112343 | null | 112,025 | Chemistry 2 | 91.690559 | Biography | 6.526013 | Chemistry | [
-46.47456359863281,
-56.5089111328125
] | XXIII .
" On Fermat 's Theorem of the Polygonal Numbers .
" By the Right Hon. Sir FREDERICK POLLOCK , F.R.S. , Lord Chief Baron .
Received June 18 , 1863 .
[ An abstract will be given in a future Number .
] COMMUNICATIONS RECEIVED SINCE THE END OF THE SESSION .
I. " On Mauve or Aniline-Purple .
" By W. H. PERKIN , Esq. , F.C.S. Communicated by J. STENHOUSE , LL. D. , F.R.S. Received August 19 , 1863 .
( Abstract .
) The discovery of this colouring matter in 1856 , and its introduction as a commercial article , have originated that remarkable series of compounds known as Coal-tar colours , which have now become so numerous , and , in consequence of their adaptability to the arts and manufactures , are of such great and increasing importance .
The chemistry of mauve may appear to have been rather neglected , its composition not having been established , although it has formed the subject of several papers by continental chemists .
Its chemical nature also has not been generally understood ; and it is to this fact that many of the discrepancies between the results of the different experimentalists who have worked on this subject are to be attributed .
On adding a solution of hydrate of potassium to a boiling solution of commercial crystallized mauve , it immediately changes in colour from purple to a blue violet , and , on standing , deposits a crystalline body , which , after being washed with alcohol and then with water , presents itself as a nearly black glistening body , not unlike pulverised specular iron ore .
This substance is a base which I propose to call Mauveine ; it 1863 .
] 713 dissolves in alcohol , torming a violet solutionl , which immediately assumes a purple colour on the addition of acids .
It is insoluble , or nearly so , in ether and benzole .
It is also a very stable body , and decomposes ammoniacal salts readily .
When heated strongly it decomposes , yielding a basic oil .
Its analysis has led to the formula C27* 24 N4 .
Hydrochlorate of Mauveine.-This salt is prepared by the direct combination of mauveine with hydrochloric acid .
From its boiling alcoholic solution it is deposited in small prisms , sometimes arranged in tufts , possessing a brilliant green metallic lustre .
It is moderately soluble in alcohol .
Carbon , hydrogen , nitrogen , and chlorine determinations have led to the formula C27 H24 N4 H C1 .
I have endeavoured to obtain a second hydrochlorate , but up to the present have not succeeded .
Platinum-Salt.-Mauveine forms a perfectly definite and beautifully crystalline compound with bichloride of platinum , which , if prepared with warm solutions , separates in the form of crystals of considerable dimensions .
It possesses the green metallic lustre of the hydrochlorate , but on being dried assumes a more golden colour .
It is very sparingly soluble in alcohol .
The analysis of this salt has led to the following formula , C27 t124 N4 , IPt C13 .
Gold-Salt.-This substance separates as a crystalline precipitate , which , when moist , presents a much less brilliant aspect than the platinum derivative ; it is also more soluble in alcohol than that salt , and when recrystallized appears to lose a small quantity of gold .
Its analysis has given numbers agreeing with the formula C27 H N4 , H Au Cl , .
Hydro6bromate of Mauveine.-This salt is prepared in a similar manner to the hydrochlorate , which it very much resembles , except that it is less soluble .
Carbon , hydrogen , and bromine determinations give results agreeing with the formula 27 24 N4 , H Br .
Hydriodate of iMauveine .
In preparing this salt from the base , it is necessary to use hydriodic acid which is colourless , otherwise the free iodine will slowly act upon the new product .
It crystallizes in prisms , having a green metallic lustre .
It is more insoluble than the hydrobromate .
Its analysis has led to the formula C27 H24 N. , HI .
Acetate of Mauveine.-This salt is best obtained by dissolving the base in boiling alcohol and acetic acid .
It is a beautiful salt , crystallizing in prisms possessing the green metallic lustre common to most of the salts of mauveine .
Combinations of this substance gave numbers agreeing with the formula C2 , ,,24 NCH 0 .
24 4 ' 24 2 ' Carbonate of Mauveine.-The tendency of mauveine to combine with carbonic acid is rather remarkable .
If a quantity of its alcoholic solution be thrown up into a tube containing carbonic acid over mercury , the carbonic acid will be quickly absorbed .
To prepare the carbonate , it is necessary to pass carbonic acid gas through boiling alcohol containing a quantity of mauveine in suspension ; it is then filtered quickly , and carbonic acid passed through the filtrate until cold ; on standing , the carbonate will be deposited as prisms having a green metallic lustre .
This salt , on being dried , gradually loses carbonic acid .
From experiments that have been made with this salt , it would appear to have the composition of an acid carbonate , viz. C27 H11 N H , C03 .
In the analysis of salts of mauveine great care has to be taken in drying them thoroughly , as most of them are highly hygroscopic .
I am now engaged with the study of the replaceable hydrogen in mauveine , which I hope will throw some light upon its constitution .
From its formula , I believe it to be a tetramine , although up to the present I have not obtained any definite salts with more than one equivalent of acid .
Mauveine , when heated with aniline , produces a blue colouring matter , which is now under investigation .
A salt of mauveine , when heated alone , also produces a violet or blue compound .
1863 .
] 715
|
112344 | 3701662 | Notes of Researches on the Intimate Structure of the Brain.--Third Series | 716 | 722 | 1,862 | 12 | Proceedings of the Royal Society of London | J. Lockhart Clarke | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1862.0155 | null | proceedings | 1,860 | 1,850 | 1,800 | 7 | 82 | 2,663 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112344 | 10.1098/rspl.1862.0155 | http://www.jstor.org/stable/112344 | null | null | Neurology | 66.878792 | Biology 3 | 29.429338 | Neurology | [
-81.67594909667969,
9.331242561340332
] | II .
" Notes of Researches on the Intimate Structure of the Brain."-Third Series .
By J. LOCKHART CLARKE , F.R.S. Received September 1 , 1863 .
Structure of the Valve of Vieussens.-The valve of Vieussens consists of four different kinds of layers .
The most inferior layer is composed of epithelium , which is continuous with that of the fourth ventricle .
The second layer is a stratum of longitudinal nerve-fibres , continuous with the white substance of the inferior vermiform process of the cerebellum .
The third layer consists of a multitude of round , granular nuclei of about the 3500th of an inch in diameter , traversed by fibres derived from the subjacent layer .
These nervefibres , in my preparations , may be seen in the most unequivocal manner to divide and subdivide into small branches , to which the nuclei are attached as by stalks .
The fourth or uppermost layer is chiefly granular , but is also interspersed with nuclei of the same kind .
Along its under side , where it joins the preceding layer , is a row of large multipolar cells , which are connected by their processes with the nuclei of both layers* .
Structure of the Cerebral Convolutions .
In the human brain most of the convolutions , when properly examined , may be seen to consist of no less than eight distinct and concentric layers .
This laminated structure is most marked at the end of the posterior lobe .
On cutting off the rounded point of this lobe in the human brain , by a transverse section , at about the distance of an inch , measured along the side of the longitudinal fissure , I found , at this part , that the stratified appearance was very indistinct in the upper and outer convolutions , while it was still clearly observable in the inner and lower convolutions which rest on the cerebellum .
It was most conspicuous in the convolution that lies over the bottom of the posterior notch of the cerebellum , and which runs outward and upward , and then winds inward , to reach the surface at the side of the longitudinal fissure .
In vertical sections of convolutions taken from the end of the posterior lobe , where the laminated structure is most marked , the first or superficial layer is a comparatively thin stratum of fine and closely-packed fibres , intimately connected externally with the pia mater-with which they are very liable to be torn away-while internally they are continuous with fibres radiating from the grey substance .
The second layer is of a pale or whitish colour , and several times the thickness of the one just described .
It consists , first , of fibres running parallel with the surface , both around the convolution and longitudinally ; secondly , of fibres radiating across them from the grey substance beneath , and crossing each other with different degrees of obliquity ; and thirdly , of a small number of scattered nuclei , which are round , oval , fusiform , or angular , and have their longer axes in different directions , but mostly within-outward .
The third layer is of a grey colour , from two to four times as thick as the one above it .
It is densely crowded with cells of small size , but of different shapes , in company with nuclei like those of the preceding layer .
The cells are more or less pyriform , pyramidal , triangular , round and oval , or fusiform .
The pyriform and pyramidal cells-especially in the outer portions of the layer-lie for the most part with their tapering ends toward the surface ; and the oval and fusiform cells have generally their longer axes and their processes in a similar direction .
In the deeper portions of the layer , however , their position is more irregular , many of them lying with their longer axes parallel with the surface , and in connexion with a multitude of fibres which run in the same direction and in great number along the layer .
They contain each a comparatively large granular nucleus , which frequently nearly fills the cell .
Two , three , four , or more processes spring from the broader ends of the pyramidal cells , and run partly toward the central white substance , and partly in the plane of the layer , to be continuous with nerve-fibres in different directions .
The fourth layer is of a much paler colour .
It is crossed , however , at right angles to its plane , by narrow long and vertical groups of small cells and nuclei of the same general appearance as those of the preceding lamina .
These groups are separated from each other by bundles of fibres radiating toward the surface from the central white substance , and , together with them , form a beautiful and fan-like structure .
This layer is distinguishable from the vOL .
XII .
3E one immediately above it by a tolerably sharp outline , but internally it gradually passes into , or blends with , the next one below it , or the fifth lamina .
This fifth layer consists of the same kind of vertical and radiating groups of small cells and nuclei ; but the groups are broader , more regular , and , together with the bundles of fibres between them , present a more distinctly fan-like arrangement .
The sixth layer is again paler , and somewhat whitish , but contains some cells and nuclei which have a general resemblance to those of the preceding layers and are arranged only in a faintly radiating manner .
The seventh layer is of a reddish-grey colour , of about the same depth as the preceding , and contains the same kind of cells and nuclei , but in much greater numbers , and mixed with some others of rather larger size : only here and there they are gathered into the small elongated groups which give the appearance of radiations .
On its under side it gradually blends with the central white layer , into which its cells are scattered for some distance .
Both this and the preceding lamina are traversed by nerve-fibres which run along their planes , or parallel with the surface of the convolution .
The eighth layer is the central white stem or axis of the convolution .
As just stated , it contains , for some distance below its summit , a gradually dirinishing number of scattered cells and nuclei , extending from the lower side of the next upper layer .
The cells are all separate , and disposed with their longer axes at right angles to the curved surface of the convolution , and therefore in the direction of the fibres radiating from the central white stem , with which some , at least , are continuous* .
Course of the Fibres of the Central White Substance through the Convolutions .
From the central white stem bundles of fibres diverge in all directions , in a fan-like manner , toward the surface of the convolutions .
As they pass between the long and vertical groups of cells ( already mentioned ) in the inner grey layers , some of them become continuous with the processes of the cells , and others turn round to become horizontal , both in a transverse and longitudinal direction as regards the convolution , and with different degrees of obliquity .
While the bundles themselves are by this means reduced in size , their component fibres become finer as they approach the surface , in consequence , apparently , of branches which they give off , to be connected with cells in their course .
When they arrive at the outer grey layer , they are reduced to the finest dimensions , and form a close network , with which the nuclei and cells are in connexion* .
Through this layer , however , many of them pass in straight lines , and , in company with processes from some of the cells , traverse the next outer and white layer , in which part of them turn round the circumference of the convolution-part run longitudinally and with various degrees of obliquity , but parallel with the surface , decussating with the former-others appear to form loops by returning to the grey iamina from which they proceed-while the rest continue their vertical course , crossing each other at different angles , and reaching the surface , where they become continuous with the compact and thin stratum of fibres which forms the first layer of the convolution , and is in immediate connexion with the pia matter .
While the bundles of fibres diverge on all sides from the central stem of white substance , another system of fibres , springing from each side of the base of the stem , curve inward and form a beautiful arch over its summit , where they decussate each other , and partly constitute the innermost pale layer .
The fibres of the stem itself are crossed transversely and obliquely by a variable number of others of different diameters ; and in longitudinal sections ( that is , in sections made in the length of the convolutions ) these transverse and oblique fibres are frequently seen to increase in number toward the base of the white substance , where they decussate each other at every possible angle .
Such is the structure of the convolutions at the extremity of the posterior lobe , in which the laminated appearance is most marked .
In almost all other convolutions , however , eight laminae , although sometimes indistinct , may be brought into view by means of solution of potash or soda .
Sometimes , as in certain parts of the posterior lobe itself , one can scarcely make out more than seven layers , there being only one broad layer of arciform fibres running along the grey layer outside the white central stem .
It is an error to call the layers containing these arciform fibres ( for I shall so name them ) the white layers of the convolution , for they are always interspersed with numerous cells , with processes of which they are continuous .
In some parts of the brain ( on the vertex for instance ) the second ( from the centre ) of the arciform bands of fibres is very broad and strong , and thickly interspersed with large and small cells of different shapes .
These arciform fibres of the convolutions run in different planes , transversely , obliquely , and longitudinally .
Where a convolution bends round upon itself at a right angle , a section made at the angle contains them in abundance ; but here the separate fibres forming the arciform bands are very short , being cut in their passage .
The curved arciform fibres , then , establish an infinite number of communications in all directions between different parts of each convolution , between different convolutions , and between these and the central white substance .
I have already shown that the more superficial layer of grey substance contains numerous arciform fibres , but finer and less strongly marked .
But the convolutions at the extremity of the posterior lobe differ from the rest , not only in the greater distinctness of their several laminae , but also in the appearance of some of their cells .
On advancing forward , the convolutions contain a great number of cells of a much larger kind .
In a section , for instance , taken from a convolution at the vertex , and in a vertical line passing through the optic thalamus , the greater number of the cells differ but little from those at the extremity of the posterior lobe ; but amongst these cells , in the two inner bands of arciform fibres , and the grey layer between them , I found a number of much larger , triangular , oval , and pyramidal cells scattered about at variable intervals .
' The pyramidal cells ' are very peculiar .
Their bases are quadrangular , directed toward the central white substance , and give off four or more processes , which run partly toward the centre to be continuous with fibres radiating from the central stem , and partly parallel with the surface of the convolution , to be continuous with arciform fibres .
The processes may frequently be seen to subdivide into minute bralches which form part of the intervening network , as I have described on former occasions .
The opposite end of each pyramidal cell tapers gradually into a straight process which runs directly towards the surface of the convolution , and may be traced to a surprising distance , giving off minute branches in its course , and becoming lost in the surrounding network .
Many of these cells , as well as those of a triangular , oval , and pyriform shape , are as large as those of the anterior grey substance of the spinal cord .
In other convolutions I again found the vesicular structure somewhat modified .
In the surface convolution , for instance , at the side of the longitudinal fissure , on a level with the anterior extremity of the corpus callosum , all the three inner laminse are thronged with pyramidal , triangular , and oval cells , of considerable size , and in much greater number than in the situation last mentioned .
Between these , as usual , is a multitude of the smaller cells .
The cells of the convolutions in man certainly differ in some respects from those of the larger mammalia-from those , for instance , of the ox , sheep , and cat .
In the early foetal brain of mammalia and man the structure consists of one uninterrupted nucleated network .
As development advances , separate layers may be distinguished .
In a foetal sheep 2 ?
inches long , for instance , I distinguished six layers in a transverse section of the brain , extending from the vertex to the interior of the lateral ventricle .
The first , second , and third corresponded to those which I have described in the convolutions of the adult human brain , and still consisted of roundish nuclei connected by a network of fibres .
The third of these layers consisted chiefly of a dark and dense stratum of nuclei , exactly similar to that which the caput cornu posterioris of the spinal cord presents at the same period of development .
The fourth layer consisted chiefly of elongated and radiating groups of nuclei .
The fifth layer was dark , containing nuclei and a dense stratum of transverse fibres .
The sixth layer was composed of epithelium , uninterruptedly connected with the network of the preceding layers , and having precisely the same appearance as the epithelium of the cord at the same period of development .
On the Structure of the Cerebellum.-The observations of Gerlach on the minute structure of the cerebellum are in the main confirmed by my own .
I must state , however , that the outer grey layer con sists of an exceedingly fine network of fibres interspersed and connected with nuclei .
This network is partly formed by the minute ramifications of the processes which proceed from the large nucleated cells along its inner border , and which completely reach the surface , communicating with each other in their course .
In my preparations this arrangement is very distinctly seen .
The facts contained in these notes will be illustrated , as soon as possible , by appropriate drawings .
|
112345 | 3701662 | Obituary Notices of Fellows Deceased | i | lxvi | 1,862 | 12 | Proceedings of the Royal Society of London | null | nws | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 66 | 811 | 29,535 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112345 | null | http://www.jstor.org/stable/112345 | null | null | Biography | 82.344363 | Reporting | 5.32451 | Biography | [
30.23993492126465,
81.53855895996094
] | OBITUARY NOTICES OF FELLOWS DECEASED BETWEEN 30TH Nov. 1S60 AND 30TH Nov. 1861 .
WILLIAM BALY was born at Lynn , in Norfolk , in 1814 , of parents distinguished for their intellectual culture and literary tastes .
IHe was educated in the Lynn Grammar School , and was apprenticed to Mr. Ingle ( now Dr. Ingle , of Emsworth ) , an active and esteemed practitioner of that town .
In 1831 he entered as a pupil of University College , London , and in 1832 at St. Bartholomew 's Iospital .
At the former he attended the lectures , and at the latter the practice , necessary for the usual diplomas of the College of Surgeons and the Apothecaries ' Hall .
At both schools alike he distinguished himself by earnest and successful work ; and at the end of his pupilage he attached himself to St. Bartholomew 's , where he devoted himself zealously to the study of clinical medicine , chiefly under the guidance of Dr. Latham and Dr. Burrows , who even then observed so much of good promise in him that they advised him to prepare to venture on the life of a physician in London .
Accordingly in 1834 , after obtaining the Diploma of the College of Surgeons and the Licence of the Society of Apothecaries , he went to Paris with a view to the further prosecution of his studies , and , after a winter spent there , to Heidelberg , and thence to Berlin , where he graduated as Doctor of Medicine in 1836 .
On his return to England he settled in London , with the view of establishing himself in practice .
During the first four years of this period of his career he was occupied with the translation of Miiller 's ' Handbuch der Physiologic , ' a task which he executed with the same scrupulous care as he gave to all his later works ; for he not only rendered the German into English of a better style , but he thoroughly studied and worked through the book , repeating many of the observations it described , and examining many of its doctrines .
His annotations to that work , if published separately , would have gained for him the reputation of being an expert and original physiologist .
In 1840 , through the recommendation of Dr. Latham , Dr. Baly was appointed to visit and report on the state of the Milbank Penitentiary , where dysentery was very prevalent .
This led in the next year to his appointment as Physician to that establishment .
The post was of immense advantage to him .
It gave him sufficient means of living , while he had very little private practice .
The number of sick under his care was often large ; their diseases had peculiar interest ; and he was brought into contact with Government officers , many of whom could appreciate his trustworthiness and rare ability .
For nearly twenty years during which he held this appointment , among all the changes to which the prison was subjected in its discipline and purpose , and in all the varieties of administration under successive Home Secretaries , inspectors , and governors , he was always well esteemed , always trusted , and very generally referred to as a principal medical adviser of Government on questions of the hygiene of prisons .
The chief results of his studies at the prison are comprised in his numerous Reports ; but more especially in a most elaborate paper on the " Diseases of Prisons , " in the twenty-eighth volume of the 'Medico-Chirurgical Transactions , ' and in his ' Gulstonian Lectures on Dysentery , ' published in 1847 .
To the same studies also may be referred much of the knowledge displayed in the Report on Cholera , drawn up in conjunction with Dr. Gull , at the desire of the College of Physicians .
In 1841 Dr. Baly became Lecturer on Forensic Medicine at St. Bartholomew 's Hospital .
He held that Lectureship for fourteen years ; and though , as his simultaneous work at the prison showed , he never forgot that the real business of his life was in Practical Medicine , yet he worked assiduously and conscientiously at the duties of this subsidiary appointment .
In 1846 Dr. Baly was admitted a Fellow of the College of Physicians ; in 1847 a Fellow of the Royal Society ; in 1854 he became Assistant-Physician to St. Bartholomew 's Hospital ; and in 1855 , in conjunction with Dr. Burrows , Lecturer on Medicine there .
He was now fairly in the tide of practice , with every prospect of attaining high reputation as a hospital physician , and of multiplying a hundredfold the value of his knowledge by diffusing it among his pupils .
But his social position was , to be yet more eminent , and his influence yet wider .
In 1859 some one of adequate fitness was required who might at first share with Sir James Clark , and then hold alone , the office of Physician in immediate attendance on the Queen and the Royal Family .
Those who were charged to make a just selection for this high office wisely fulfilled their responsible task in the choice of Dr. Baly , whose pre-eminent qualifications for the duty were unanimously admitted by the whole medical profession .
To himself the appointment is said to have been a surprise ; but how well he justified the selection was shown by the proofs of confidence which he received from the Queen and the Prince Consort , and the esteem in which he was held by the whole of the royal household .
With the highest honours of his profession within his reach , trusted by his Sovereign , esteemed by his brethren , and held in affection by his many friends , the pride of his two sisters , who had worked lovingly with him in his laborious days , -his prosperous career was sadly terminated and his valuable life in a moment cut off , on the 28th of January , 1861 , by one of those fatal chances to which railway travelling is still but too liable , but in this unhappy case apparently baffling human foresight .
Dr. Baly 's early death occasioned a wide-spread feeling of grief .
Literally he was mourned from the palace to the prison .
With the sense of bereavement was mingled that of disappointed hope ; for with his clear and vigorous intellect , his well-balanced and cultivated mind , his devotion to the profession of his choice , his severe sense of duty , his assiduous habits , and his freedom from all controversial tendencies , there was sure promise that , had he been vouchsafed a longer life , he would have yet done much for the advancement of knowledge and the good of mankind .
GE0nRG BISHOP was born August 21 , 1785 , at Leicester .
He was well known in the commercial world as the head of the largest manufacture of British wines in the kingdom .
Having a taste for astronomy , he erected an observatory in 1836 at his residence , South Villa , in the Regent 's Park .
He received the services of such observers , among others , as Mr. Dawes and Mr. Iind , who soon gave his observatory a European name .
Without entering into details on double stars , nebulae , &c. , we shall but say that the South Villa observatory claims eleven of the small planets , ten discovered by Mr. Hind and one by Mr. Marth .
It is now removed to Twickenham by Mr. George Bishop , Jun. Mr. Bishop was successively Secretary , Treasurer , ald President of the Astronomical Society ; he was elected a Fellow of the Royal Society in 1848 .
He died June 14 , 1861 .
HIe will stand high among those of his day ( no small number ) who have devoted commercial wealth to the increase of knowledge ; and will be remembered with all the additional honour due to uprightness and benevolence .
Sir WILLIAM CUBITT was the son of a miller of Dilham , in Norfolk , and at an early age was apprenticed to a joiner .
After some years spent in the exercise of his trade , and in the works required for repairing the mills of the district , he entered the factory of Messrs. Ransom of Ipswich .
In their employment Sir William became practically acquainted with the details of Civil Engineering ; and about this period of his life he invented the self-winding apparatus of windmills , and the now well-known instrument of prison discipline , the tread-wheel .
About 1826 he removed to London and began business on his own account as a civil engineer , and in time attained the foremost rank in his profession .
The works executed by Sir William Cubitt on the Norfolk and Lowestoft Navigation , on the Severn Navigation , the South-Eastern and the Great Northern Railways , the landing-stages at Liverpool , the new Rochester Town Bridge , the Berlin Water-works , &c. , may be referred to as illustrations of his practical skill ; and it is not too much to say that the manner in which the South-Eastern line is carried between Folkestone and Dover is one of the boldest pieces of engineering of which we have examples in England .
In 1851 Sir William was charged with the superintendence of the working details of the Great Exhibition building , and for his exertions on that occasion he received the honour of knighthood .
Sir William Cubitt was born in 1785 , and died October 13th , 1861 .
The date of his election into the Royal Society is April 1 , 1830 .
Dr. WILLIAM HENRY FITTON , who , died in London on the 13th of May , 1861 , was born in Dublin in January 1780 .
His family was originally of Cheshire , but had long been settled in Ireland .
After passing through his school education , he entered Trinity College , Dublin , and in 1798 , through:his proficiency in classics , obtained the Senior Scholarship .
IIe took his Degree of Bachelor of Arts in 1799 .
Although originally intended for the Church , Mr. Fitton chose a medical career , and with that view pursued his studies in the University of Edinburgh , where he also attended the Lectures of Professor Jameson on Natural History , and made the acquaintance of various young men , zealous in study , who afterwards attained to distinction in science and literature .
After taking his Doctor 's degree , he passed some time in London , studying medicine and chemistry , and in 1812 removed with his widowed mother and his three sisters to Northampton , where he began practice as a physician .
After eight years ' stay in Northampton , he married a lady who brought him the means of living independently of his profession , and he accordingly withdrew from practice , and took up his abode in London , where he dwelt for the rest of his life , occupied chiefly with his favourite pursuit of geology , and contributing , by his personal qualities and accomplishments , and by his open hospitality , to promote useful and agreeable social intercourse among the scientific men of the metropolis .
From his youth up Fitton was devoted to geology .
Before he left Ireland he collected fossils , determined barometrically the height of the chief mountains , and made excursions into Wales to study its mineral structure .
H-is first publication on the science was a memoir " On the Geological Structure of the Vicinity of Dublin , " communicated to the GeologicAl Society in 1811 , and printed in the first volume of its 'Transgctions .
' From 1817 to 1841 he contributed to the ' Edinburgh Review ' a series of articles which present a just and elllightened commentary on the progress of geological science for the eventful thirty years of which they treat .
But the researches on which the reputation of Dr. Fitton as a geologist will most deservedly and most enduringly rest , " are those by which , during twelve active years of his life ( from 1824 to 1836 ) , he laboriously developed the true descending order of succession from the Chalk downwards into the Oolitic Formations , as exhibited in the south-east of England and in the adjoining parts of France .
Before these labours commenced geologists had only confused notions as to the order of the strata beneath the Chalk , as well as of the imbedded fossil remains of each stratum .
It was Fitton who made the Greensand Formations his own , by clearly defining the position and character of the Upper and the Lower Greensands , as separated by the Gault * .
' This statement is from a recent notice of Dr. Fitton , containing further interesting information on his life and labours , and proceeding from an authority unquestionable , both as regards personal knowledge of the man , and just appreciation of his work .
Dr. Fitton was elected into the Royal Society in 1815 .
He belonged also to the Linnean , Astronomical , and Geographical Societies .
Of the Geological Society he was one of the most active and distinguished Fellows ; he served for some years as Secretary , and eventually attained to the honour of the Presidency ; and in 1852 , when he had for some years ceased from active labour , the Society " conferred on their veteran associate the highest honour in their gift , the Medal founded by his dear friend Wollaston .
" Sir JOHN FORBES was born in December 1787 , at Cuttlebrae , in the parish of Ruthven , Banffshire .
In 1799 he went to the Academy of Fordyce , where he formed that friendship with Sir James Clark which remained a source of life-long pleasure to both .
Obtaining a Bursary ( founded by an ancestor of his mother 's ) to the Grammar School at Aberdeen , he proceeded thither in 1802 ; and in the following year he entered at Marischal College in Aberdeen , where he remained until 1806 .
From Aberdeen he went to " Edinburgh , where he obtained a surgical qualification ; and in 1807 he entered the medical service of the Navy , in which he served , chiefly in the North Sea and in the West Indies ( where he was present at the taking of Guadaloupe by Sir P. H. Durham , to whom he acted not only as flag-surgeon but as secretary ) , until 1816 .
Being placed on half-pay at the general reduction which took place at the conclusion of the war , he returned to Edinburgh , where he spent a year and then graduated .
On the recommendation of Professor Jameson he settled at Penzance as the successor of Dr. Paris , and there he remained until 1822 , giving his attention not merely to professional but also to scientific pursuits , especially meteorological and geological investigations .
His " Observations on the Climate of Penzance " and his papers on the " Temperature of Mines " are still quoted as of standard value ; and two papers on the " Geology of the Land 's End " give further evidence of his zeal and sagacity as a student of Nature .
It was during the last year of his residence at Penzance that he published his translation of Laennec 's great work on 'Auscultation , ' which was at that time but little known and still less appreciated in this country , but which impressed Dr. Forbes 's mind with a sense of its value that was soon justified by the general voice of the more enlightened part of the profession .
In 1822 he removed to Chichester as successor to Sir William Burnett ; and there he continued for twenty years , obtaining the principal practice in the town and in the neighbouring district of Sussex ; while there too he formed that friendship with Dr. Conolly which led to their subsequent association in two medical works of great importance .
The first of these was the 'Cyclopiedia of Practical Medicine , ' the publication of which was commenced in 1832 and completed in 1835 , under the joint editorship of Dr. Tweedie ( to whom the original idea of the work is due ) , Dr. Forbes , and Dr. Conolly .
Besides undertaking a large share of the editorial labour , Dr. Forbes furnished to this ' Cyclopaedia ' several articles of high excellence , which contributed in no small degree to establish its reputation .
Previously to its completion he projected the ' British and Foreign Medical Review , ' associating Dr. Conolly with himself as editor ; the publication of this journal , which commenced in January 1836 , was carried on under their joint superintendence for four years , Dr. Forbes performing nearly all the editorial labour ; and on Dr. Conolly 's removal to Hanwell in 1840 , which occasioned his relinquishment of his connexion with the ' Review , ' Dr. Forbes became its sole editor , and continued to discharge that duty until 1847 .
It was chiefly with the object of improving the 'Review ' that he removed to London in 1840 , giving up a lucrative practice and a high social position at Chichester , under the full consciousness that he could not expect to attain a corresponding status in the metropolis .
In the next year he was appointed Physician to the Prince Consort and to the Queen 's Household , and he continued to hold these appointments until compelled to relinquish them by the failure of his health in 1859 .
HTe was elected into the Royal Society in 1829 .
Although the Review ' never attained a commercial success , yet there cannot be two opinions as to the importance of the benefits it conferred on the medical profession .
Previously to its commencement there had been nothing that deserved to be called full and fair criticism in medical journalism ; the so-called ' Reviews ' being either mere analyses of the books which they professed to criticise , or confined to a general expression of the opinion formed as to their merits or demerits by writers who were too frequently incapacitated by ignorance or prejudice , or by both combined , to pronounce a trustworthy verdict .
It was Dr. Forbes 's constant object to secure the services of the best-informed and most impartial contributors whom he could succeed in enlisting ; and such was the estimation which the 'Review ' soon acquired , not only for its truthful appreciation of the works it criticised , but for the original information contained in many of its articles , that he had no difficulty in assembling around him a staff of able and zealous assistants , over whose productions he exercised a judicious editorial supervision , stamping upon them everywhere his own peculiar marks of justice , accuracy , and vigour .
It was his constant object to give an account of the progress of every department of medical science , wherever and by whomsoever made ; and by this means he largely diffused an acquaintance with the best foreign medical literature among the profession in this country .
Constantly seeking to infuse fresh blood into the organism of which he was the life , he was always glad to avail himself of the assistance of young men who could give the requisite evidence of ability and probity , to whom on his part he afforded the benefit of his wise counsel and kindly aid ; and it would not be difficult to point to several men now holding positions more or less distinguished , who would gladly testify how much of their subsequent success they owe to their early association with the ' Review ' and with its editor .
It was very seldom that he himself wrote more than short 'Notices ' of books , or paragraphs interpolated in the longer articles of his contributors ; but he departed from his usual course in 1846 , putting forth ( avowedly as his own ) a remarkable article entitled " I-omccopathy , Allopathy , and Young Physic ; " the purpose of which was in the first place to expose the errors and absurdities of Homeeopathy , whilst bringing into prominence the " vis medicatrix naturre " as the real agent in its reputed cures , -next to point out that the ordinary routine of medical practice , as carried on by a large proportion of the profession , is scarcely less erroneous in principle and even more mischievous in result , and thirdly , to assert the doctrine that Rational Medicine should be based on the recognition of the curative powers of Nature as the foundation of treatment , and that it should place its chief reliance on those methods which carry out the indications afforded by the " natural history " of each form of disease , that is , the course it would run if uninterfered with by Art .
These views , which he subsequently expanded in a small treatise entitled " Nature and Art in the Cure of Disease , " were put forth in the first instance with an incautious brusquerie which raised a storm of indignation against their author , and damaged the reputation of the 'Review .
' But although what was injudicious in form and manner for a time prevented what was really just and true from obtaining a fair hearing , yet much of the effect which the author strove to produce has gradually developed itself ; for there can be no doubt that the practice of the better-educated portion of the profession is now essentially based on the principles which he enunciated ; and although various influences have cooperated to bring about this reform , yet no small share of its merit must be assigned to the honesty and vigour with which truths were spoken out in ' Young Physic , ' which conservative timidity would have continued to keep in reserve .
The advance of years and other circumstances determined Dr. Forbes in 1847 to relinquish the editorship of the 'British and Foreign Medical Review , ' and to transfer his property in it to its publisher , who has made it his constant aim to keep up the high tone impressed on it by its originator , and to maintain the position he acquired for it as the " leading medical journal , " not only of this country , but of the world .
With the exception of the small treatise just referred to , Dr. Forbes did not make any firther additions to professional or scientific literature ; but he published , under the name of 'A Physician 's Holiday , ' an account of a summer excursion in Switzerland , which acquired a popularity that led him to two further ventures in the same line , respectively entitled 'Memorandums made in Ireland , ' and an 'Excursion in the Tyrol .
' In 1852 the University of Oxford conferred upon him the Degree of D.C.L. , and in 1853 the honour of knighthood was bestowed upon him .
At the end of 1854 , having been requested by Government to organize and superintend a large hospital at Smyrna for the sick of the Crimean war , he accepted the post with alacrity under the promptings of that earnest desire to make himself useful in his day and generation which had shown itself in his previous undertakings , and actively commenced the necessary arrangements ; but with more time for deliberation and consultation with friends he began to question whether his physical powers would be equal to the post , and finally determined to resign it .
Not long subsequently he had the first warnings of that failure of nervous power which progressively increased , until in 1859 he found it necessary to withdraw altogether from active life , and to remove to the residence of his only son at Whitchurch near Reading , where he gradually and tranquilly sank , his death occurring on the 13th of November , 1861 .
Although Sir John Forbes cannot be ranked among those who have advanced the science of medicine by the discovery of new facts or the promulgation of new principles , he must be regarded as having done most essential service to the cause of progress , on the one hand by his ready recognition and zealous diffusion of every novelty of sterling value , on the other by the determined onslaught which he made upon prevalent errors , and the vigorous earnestness with which he pleaded for generally-neglected truths .
In the depth and extent of his knowledge , in his sagacity as a reasoner , in the earnestness of his search for truth , in his fearless courage in proclaiming it , in his single-minded devotion to right and justice , and in the disinterestedness with which he sacrificed all personal considerations to promote the general good , Sir John Forbes combined all the best qualities of a Reformer .
When we add to this estimate his ardent love and extensive knowledge of literature , the general liberality of his sentiments , the wide range of his sympathies , the geniality of his disposition , and that active benevolence which ceaselessly urged him to employ every means in his power for the promotion of objects of public philanthropy , and for the individual benefit of those who had acquired a peculiar claim to his regard , we have such a combination of admirable qualities as could not but command for him the general respect and esteem of his contemporaries and thewarm attachment of a large circle of private friends .
The Royal Society has lost a young and promising associate in Mr. HENRY GRAY , who was cut off by an attack of small-pox on the 8th of June , 1861 , at the early age of thirty-six .
Mr. Gray was Lecturer on Anatomy at St. George 's Hospital , and had been nominated to the office of Assistant Surgeon to the Institution .
During the brief career vouchsafed to him , Mr. Gray laboured assiduously and with much success in Anatomy and Physiology .
In 1849 he gained the triennial prize of the Royal College of Surgeons for an Essay on the " Anatomy and Physiology of the Nerves of the Human Eye , " and soon afterwards he presented a paper to the Royal Society " On the Development of the Optic and Auditory Nerves , " which was published in the 'Philosophical Transactions ' for 1850 .
Another contribution , entitled " On the Development of the Ductless Glands of the Chick , " appeared in the volume for 1852 .
Hle then undertook an important research into the Anatomy and Physiology of the Spleen , in the prosecution of which he was aided by an allotment from the annual grant placed at the disposal of the Royal Society by Parliament for the promotion of science ; and his labours were rewarded by the triennial " Astley Cooper Prize " of ?
300 in 1853 .
Two papers on more strictly professional subjects appeared in the 'Medico-Chirurgical Transactions .
' His last work was a ' Systematic Treatise on Anatomy , ' which was published in 1858 , and has rapidly gone through two editions .
Mr. Gray was , moreover , an accomplished and lucid teacher of anatomy , and much esteemed in private life , so that his early death was very widely lamented by his professional brethren .
His election into the Royal Society took place in 1852 .
EATON IODGKINSON was the son of a farmer at Anderton , in the parish of Great Budworth , Cheshire , where he was born on the 26th of February , 1789 .
When but six years old he lost his father ; and in compliance with the wish of his uncle , the Rev. Henry Hodgkinson , Rector of Arberfield , Berkshire , he was sent to a classical school , in order to fit him for a university course , with a view to his entering the Church .
The youth , however , had little turn for languages , and it was determined to send him to the private school in Northwich to learn mathematics , to which he had shown a strong inclination .
the seems to have profited greatly by the instruction he received there , for in after-life he often expressed his gratitude to his early master , Mr. Shaw , for laying the foundation of his future mathematical acquirements .
In 1811 his mother and family removed to Manchester , where Mr. Ilodgkinson assisted his mother in carrying on business , by which she eventually earned a competency .
In Manchester he had full scope to follow the bent of his mind for mathematical and physical pursuits .
Here also he made the acquaintance of various eminent persons distinguished for their scientific attainments or manufacturing and engineering skill ; and , following the example of some other young men of his acquaintance who were desirous of improvement , he became a pupil of Dr. Dalton , then a private teacher of mathematics in iManchester , and read with him the works of Lagrange , Laplace , Euler , and Bernoulli .
The friendship thus begun continued uninterruptedly until Dr. Dalton 's death .
The erection of the factory of Phillips and Lee first gave occasion to Mr. Hodgkinson 's experimental inquiries into the strength of materials used in construction , which , amongst other results , led him to propose a new form of cast-iron girder .
He discovered that cast iron resists compression with an energy nearly six times as great as that with which it resists extension ; and he accordingly recommended a form of cross section , in which the upper and lower flanges present sectional areas corresponding with the power of resistance to compression and extension respectively ; and this form has now been universally adopted .
At the works of Messrs. Fairbairn and Lillie , then rising engineers , Mr. Hodgkinson obtained the requisite means and facilities for making his experiments .
In 1840 Mr. Hodgkinson communicated to the Royal Society a memoir , entitled " Experimental Researches on the Strength of Pillars of Cast Iron and other Materials , " which was published in the 'Philosophical Transactions ' for 1840 , and obtained for its author the award of the Royal Medal for the year 1841 .
The results of further inquiries were given in a later paper , published in the 'Philosophical Transactions ' for 1857 .
He was elected a Fellow in 1841 .
The formulae he deduced for calculating the strength and deflexion of pillars and beams have been accepted with implicit confidence , and now have a place in all engineering textbooks .
Mr. Ilodgkinson became a Member of the Manchester Philoso .
phical Society in 1826 , and from 1822 to 1844 contributed seven papers to its Memoirs , ' chiefly on the mechanical principles of engineering .
Ie was also an active Member of the British Association for the Advancement of Science , and contributed valuable matter to the 'Transactions ' and 'Reports ' of that Association .
The combination of experimental skill with mathematical knowledge which characterized Mr. IHodgkinson was turned to account on the occasion of the construction of the Conway and Britannia tubular bridges .
He was engaged by Mr. Fairbairn to assist in the experimental inquiry which it was deemed advisable to institute before commencing those great and novel undertakings ; and he contributed valuable formulae to Mr. Stephenson for calculating the true results of the experiments .
It is to the results which were then obtained that we owe the application of wrought-iron plain and boxed girders in the art of construction .
For a similar reason he was in 1847 appointed on the Royal Commission to inquire into the properties of wrought and cast iron , and their application to railway structures .
In 1847 Mr. Hodgkinson was appointed Professor of the Mechanical Principles of Engineering in University College , London , and delivered several courses of lectures , although in later years delicate health interrupted his labours .
Mr. I-odgkinson married in 1841 Catharine , daughter of the Rev. William Johns , of Manchester , an intimate friend of Dalton .
She died childless in little more than a year after her marriage ; and , after remaining a widower till within eight years of his death , he married for his second wife ( who still survives him ) Miss Holditch , daughter of I-Ienry Holditch , Esq. , C , aptain in the Cheshire Militia .
He died at Eaglesfield House , near Manchester , on the 18th of June , 1861 .
FRANCIS PALGRAVE , K.H. , author of ' The Rise and Progress of the English Commonwealth , ' The Merchant and Friar , ' The History of England and Normandy:'-born July 1788 ; died 6th July , 1861 ; the only son of Mr , Meyer Cohen ; assumed the name of Palgrave on his marriage , in 1823 , to Elizabeth daughter of Mr. Dawson Turner of Great Yarmouth .
The bankruptcy of his father , at the beginning of this century , compelled Palgrave to exchange the dream of foreign travel and the expectation of a life of competence for the necessity of working for his living .
But he neither shrank from the duties thus unexpectedly laid upon him , nor neglected that mental cultivation which his father 's unstinted care had commenced .
In his sixteenth year he entered a lawyer 's office , and continued there , on the expiry of his articles , as managing clerk till the year 1822 .
A home education gave early maturity to his abilities .
When but eight years old he translated the ' Battle of the Frogs and Mice , ' attributed to Homer , from Latin into French .
Before he had attained his twentieth year he had contributed many articles to the minor periodicals of the day ; and not many years later he became a regular contributor to the 'Edinburgh ' and 'Quarterly Reviews .
' Writing for the press and writing anonymously were alike distasteful to him ; but as he devoted the whole of his only certain income , that derived from the lawyer 's office , to his father , he was compelled to this means of support .
His early promise of talent did not fail of fulfilment .
lie was endowed with a mind quick to acquire languages , to grasp the laws of physical science , to appreciate the beauties of poetry and art .
He was also gifted with a bright imagination , a thirst for knowledge , and the power of patient industry .
Honesty and simplicity of nature ennobled all he said or did , and true humility made him unwilling to trust his own researches , and ready to receive suggestions from minds however different in stamp from his own .
In 1821 Palgrave submitted to Lord Spencer a scheme for the publication of the national records , which was unanimously approved by the Commission of Records , " many glorious things , " according to Mr. Hudson Gurney 's friendly report , being said of him by all .
This took place in 1822 , and from that time till 1838 he was occupied in the publication of the 'Parliamentary Writs , ' 'Exchequer Calendars , ' and other works of great magnitude and historical importance connected with the Commission .
IHe was also engaged on his own literary undertakings , and in practice as a barrister , chiefly in pedigree cases .
Much labour also devolved on him as one of the Municipal Corporation Commissioners , though he withheld his signature from their report .
He was knighted in 1831 , as an acknowledgment of his contributions to constitutional and parliamentary history ; and was appointed Deputy Keeper of the Public Records in 1838 , a post which he held up to his death .
Previous to his appointment , the national muniments were scattered over fifty-six different repositories , many of them but little fitted for the safe custody of the public archives .
A different system of management , a different scale of charges for searches and copies , prevailed in each .
By the exertion of great activity and perseverance he brought these various establishments under one system , and finally united their contents at the Rolls Estate .
His 'Annual Reports , ' twenty-two in number , afford ample proof of the extent of his official labours .
He was elected a Fellow of the Royal Society in 1821 .
The dates of Palgrave 's writings are as follows:-He brought out in 1831 a short history of English affairs from the acquisition of Britain by the Romans until the Norman Conquest ; and in the year following , the 'Rise and Progress of the English Common .
wealth .
' The C Merchant and Friar ' was his next publication .
In 1841 , after the labour of several years , he furnished Murray with the first edition of the ' Handbook to Northern Italy .
' The first two volumes of the 'History of England and Normandy ' appeared in 1851 and 1857 .
These volumes treat of the Carlovingian empire , the rise of the Capetian dynasty , and the foundation of the Duchy of Normandy .
Materials are left that carry the narrative to the time of Henry I. He also contributed , principally between the years 1815-21 and 1840-45 , upwards of forty articles to the 'Edinburgh ' and 'Quarterly Reviews .
' With the exception of the handbook , one purpose , the elucidation of our national history , runs through his works .
The ' Com. monwealth ' represents the national life of England before the Conquest .
The character of the people and general aspect of the realm is exhibited by an examination of those legal and social institutions which regulated the daily life of the community , as he felt that the attention of historians had hitherto been too exclusively confined to the political action of the times .
The little history of the Anglo .
Saxons was designed to supply that biographical portraiture and narrative detail necessarily excluded from a constitutional history , In the Merchant and Friar , ' Roger Bacon is employed as the expounder of mediaeval philosophy .
Intimate acquaintance with the curious arts of the middle ages , astrology and alchemy , with physical science , both ancient and modern , the archaeological incidents disclosed by study of the city archives , -a sensibility to the beauties of architecture and nature , supplied the author with ample means towards a just comparison of the arts and customs of the past and present .
The illustration of important constitutional principles , as shown , for instance , in the development of trial by jury and of the parliamentary representation of the English counties , even more than a picture of mediaeval society and manners , was his object in this story .
Especially did he wish to impress upon his readers that essential truth , that our " constitution is based , not upon liberty , but upon law , " -that Parliament is not only an assembly of the political estates of the realn , but a judicial tribunal , that High Court to which even the poorest in the middle ages could apply for justice .
In spite of the " wit and wisdom " contained in the 'Merchant and Friar , ' the animated pictures of past times and varied display of knowledge , the outpourings of one who loved study for its own sake , it is but an unknown book .
Further investigation of Anglo-Norman history , and that passion for his subject which springs from long-continued research , led Palgrave to abandon his intention of continuing , in one volume , the 'Commonwealth ' to the accession of the Stuarts , and he devoted himself to investigate the times that lay nearest to the Conquest .
This was , however , to him no brief undertaking .
To the right understanding of the process by which our constitution arose after the Conquest , he felt it necessary to treat fully of the Norman dynasty from its first establishment , and to exhibit the parallel between France under the Capetians , and the German empire after the extinction of the Carlovingian dynasty .
But he was not enabled to complete this great project before declining powers impeded his progress .
Palgrave sought throughout his writings to enforce certain leading historical principles .
Independent study convinced him , at the commencement of his career , " that the states composing Western Christendom were to be considered as carrying on the succession of the imperial authority of Rome , " a doctrine upon which , as he believed , all real conception of mediaeval and modern history depended .
The insight which led him to grasp this important theory , the " great key of medimval history , " and trace its influence upon the general system of human affairs , has entitled him , in the language of one of his reviewers , to a place in the very highest rank of historical inquirers .
He held an opinion of his own upon that vexed question of our history , the position assumed by William and his Normans towards conquered England .
He convinced himself that the idea , upon which Thierry laid such stress , of a bitter war of race against race being waged against the Anglo-Saxons , was greatly overcharged .
To him it seemed that the remarkable fact in English history is the practical union of interests , that the continuity of English national life was never broken by the Normans : hence the vigorous and uninterrupted progress of national power .
The lessons , however , from past times which he sought to enforce were not exclusively historical .
Political economy was a study of great interest to him .
But he never missed an opportunity of pointing out a source of error which , in his opinion , pervaded the whole school the " considering the science of political economy as being entirely subject to calculation , wholly a matter of figures ; whereas in fact the " wealth of nations , " even in the narrowest sense of the term , is quite as much rated by passion and imagination , the imponderable elements which evaporate durin the analysis , and leave no residuum in the crucible .
" Imbued with reverence and deeply stored with the learning of the past , he shrank from that tendency , perhaps more general thirty years ago than now , to contrast triumphantly the progress of modern science with medieval credulity .
IHe inclined the rather to regret the wisdom that still lingered than to boast of the knowledge that had come .
That appeal to ' civilization , " so common with French historians , as the highest standard of human perfection , was specially distasteful to him .
On the contrary , he maintained that all the elements which are really beneficial in nationality are directly at variance with the French idea of civilization-that with national language , national institutions , and national religion it cannot amalgamate .
Art was a subject to which he gave but casual attention ; yet in this his appreciation of what is real , and of true taste , gave him an insight beyond his time .
He early claimed for gothic architecture the place it now holds in popular estimation .
Years ago he suggested that principle in design , since enforced by Mr. Ruskin , that in the physical world the curve is the token of life or organized matter , as the straight line indicates death or inorganized matter .
His article on the " Fine Arts in Florence " ( Quarterly Review , June 1840 ) is a fine example of his range of mind , and contains passages eloquent with picturesque description , and stored with sound historical and artistic knowledge .
Few living men have equalled Palgrave in the extent of his reading , still fewer have surpassed him in sincere and independent inquiry .
His language was vigorous and often pointedly descriptive .
He was capable of vivid biographical portraiture , and of tracing acutely the original development and meaning of laws and titles .
Still he lacked some qualifications towards a great historian .
His habit of mind was rather that of an advocate than a judge , which diverted him from that perfect judgment which characterizes Hallam and Thirlwall .
His feeling for the importance of the laws and social institutions that influenced the daily life of the people prevented him in some degree from grasping the history of the nation as a whole .
The habit of dictating his writings tempted him to a diffuseness and redundancy of style ; and , not unlike Southey , he has left passages in his writings which are fanciful rather than humorous , and hardly worthy of his powers or of history .
This estimate of Palgrave 's literary position has been mainly adopted from a criticism on his last volume in the Edinburgh Review of April 1859 .
Notwithstanding failings such as these , the writer assigns to him a place among the highest rank of historical inquirers , and states that the new light which he has thrown upon the ancient institutions of our land , and his share in enabling us to realize the grand picture of medieval Europe , should secure to him the deep gratitude of every historical student .
He passed , like Scott and Southey , a life of unremitting industry .
As his years were continued from occupation to occu .
pation , without the chasm of a single day , so his hours led him on from work to work the page of history before breakfast , the office in mid-day , his library and books in the evening .
Though he could not rest content save in a round of unremitting activity , friendship and home love were still the salt that made life precious to him .
A man so gifted and true-hearted could hardly fail of meeting with worthy love and honourable friendship ; and in these blessings he amply shared .
The mutual devoted love and noble companionship that was given to him in his wife formed indeedl the keystone of his happiness ; yet friendship was to him no empty word .
Deservedly so , for he could claim the affectionate regard of those that really knew him , above all of Henry Hallam and Sir Robert Inglis , and of Hudson and Anna Gurney .
Nor did he escape the notice of distinguished men .
While quite young , Byron had remarked of him , that he would be at the tip-top of whatever pursuit he embarked in .
Describing an ideal translator of ancient German poetry , Scott mentioned Palgrave 's name .
Later in life we find Dr. Arnold proposing to put questions to him on our history , as the person who could answer them better than any one else .
An animated talker in society , at home he was not less ready to amuse and to instruct .
He was so bright and playful , so exceeding in kindness and indulgence , that he was there as a boy among his children , sharing in their talk , joining in their arguments , or telling stories , allegories of his own invention or scenes from history .
He ever glowed with kindness and sympathy ; but latterly animation was dimmed by sorrow from which there was no recovery , and by the commencement of that gradual decay of mind and body of which he died .
In 1847 he parted with a very dear son for the East ; about five years after that , the best part of his life was buried in his wife 's grave .
The remaining years were chiefly marked by declining powers and the death of friends , and did but speak to the truth of lallam 's sad words , " time can never reinstate us to the position of domestic happiness .
" The latter portion of his official life was , however , smoothed to him by the most considerate kindness of Sir John Romilly , a comparative stranger till his appointment as Master of the Rolls .
A mind such as Palgrave 's , that adhered instinctively to truth for its own sake , however antagonistic to popular fancy , that turned rather towards the oppressed and humble than to the successful , that was naturally averse to party feeling , and distrustful of the idol of the day , -such a mind , so endowed with wisdom not of this world , so many-sided and imaginative , could not expect to be generally appreciated , or to cause any immediate effect , or to reap the fruit of b its labours .
Still , even in this life , he anticipated , in great measure , the reward which is given to those that follow after true knowledge , and strive to guide others in the right way .
General Sir CHARLES WILLIAM PASLEY , K.C.B. , of the Royal Engineers , was born at Eskdale-Muir , Dumfries , on the 8th of September 1780 .
In his early years he displayed the impetuosity and high courage which distinguished him in after life , as well as the perseverance , ability , and liberality for which he became no less remarkable .
Having received a solid preliminary education in Scotland , he joined the Royal Military Academy at Woolwich in August 1796 , and obtained a commission in the Royal Artillery on the 1st of December , l 797 .
He was transferred to the Royal Engineers on the 1st of April 1798 , and on the 2nd of August 1799 he was gazetted as first Lieutenant in that corps .
Between 1799 and 1807 he served in Minorca , Malta , Naples , and Sicily , and was employed on various important services and confidential missions .
He was sent by General Villettes to communicate with Lord Nelson in 1804 ; and after having been promoted to the rank of second captain on the 1st of March 1805 , he served under the Prince of Hesse-Philippsthal in the defence of Gaeta against the French in 1806 , and under Sir John Stuart at the battle of Maida ( in Calabria ) in the same year .
The experience of that battle confirmed the strong opinion which he had always maintained-in opposition at that time to many in the British army-that the English generals would beat the French marshals as soon as they got a chance of doing so .
Captain Pasley took part in the siege of Copenhagen under Lord Cathcart in 1807 , and joined Major-General Leith at Oviedo in the north of Spain in September 1808 .
Hle was employed to reconnoitre the Asturian frontier , and then to communicate with General Blake at Reynosa in November , and he left Soto on the 15th of that month at night as the French entered it .
After joining Colonel Robert Crawford 's Brigade , he was retained by Sir David Baird as his extra aide-de-camp , in consequence of his general attainments and knowledge of the Spanish language .
HTe soon after joined Sir John Moore 's staff in a similar capacity , and was attached to it during the retreat upon , and at the battle of Corunna .
Though a great admirer of Sir John Moore , he was much annoyed at this retreat , and could never afterwards speak of it with patience-his conviction having been that the army ought to have turned round upon its pursuers whilst it was strong , and to have maintained a footing in the Peninsula , instead of waiting to fight at Corunna after it had been seriously weakened by retreat , and then quitting the country .
From his intercourse with the Marquis of Romagna and others , he was also convinced that the Spanish troops might under improved arrangements have been made more useful .
Captain Pasley next accompanied the expedition to Walcheren ; he was employed in reconnoitring the coasts of Cadsand and Walcheren under the fire of the enemy 's batteries ; and he was present at the siege of Flushing in 1809 .
Leading a storming party of 100 men under Colonel Pack , to obtain possession of a French battery on the dyke according to his own proposal , he was first wounded ( though not disabled ) by a bayonet in the thigh , and then , after reaching the top of the dyke , shot through the body by a French soldier from below , belonging to a fresh party of about sixty whom he challenged to surrender to twenty men .
The bullet passed in at one side and out at the other , injuring the spine in its progress , and it was hardly expected at first that he could recover .
Portions of bone , sash , and clothes came out of the wound afterwards by degrees , and it rendered him incapable of duty for more than a year * .
In November 1810 Captain Pasley published the first edition of his ' Essay on the Military Policy and Institutions of the British Empire .
' This work appeared in a time of great national despondency ; and its principal objects were to advocate greater energy and perseverance in prosecuting the war with France , judicious offensive action in the conduct of that war , and especially a more vigorous policy in Spain , and to demonstrate that Great Britain had " sufficient force and a favourable opportunity for destroying the French empire .
" It attracted great attention , and was highly approved on account of the manly and patriotic spirit which it displayed , though the doctrines of political economy which it contained were disputed .
It ran rapidly through four editions , and was favour* He took advantage of this opportunity to teach himself German amongst other things .
ably noticed ( by Mr. Canning as was supposed ) in the 'Quarterly Review ' of May 1811 , in which it is characterized as one of the most important political works that had ever fallen under the observation of the reviewer .
The opinions it expressed were contrasted with the humiliating language then to be found in the pages of the English press , and with the principle of husbanding resources which was alike the watchword and the fatal error of the despondents .
Whilst in command of the Plymouth Company of Royal Military Artificers in 1811 , Captain Pasley set himself to consider how improvements could best be made in the practice of Military Engineering .
He had found on active service the serious disadvantage under which the Royal Engineers laboured , of having no properly educated men at their disposal , and no good system for regulating their operations ; and the remainder of his life was chiefly devoted to the supply of these wants .
Finding that the ordinary modes of instruction were unsuited to his object , he composed an elaborate treatise intended to enable the noncommissioned officers to teach themselves and their men without the assistance of mathematical masters , on a method similar to that of Dr. Bell and Mr. Lancaster , and to go through their courses of geometry in the same manner as their company drills or their small-arms exercises .
The system thus organized was found so successful at Plymouth , that it was introduced on an extended scale into the schools at Chatham in spite of some objections-one critic fearing that the men would become better educated than their officers , and might be consulted by the Generals commanding !
His energy and success , backed by the representations of the Duke of Wellington from the Peninsula as to the defective condition of the Engineer Department in the Field , led to the formation of the Establishment for Field Instruction at Chatham , and to his appointment to the office of Director of that establishment , with the rank of Brevet-Major .
Ile was promoted to the rank of Brevet Lieutenant-Colonel in May 1813 , and he became a Lieutenant-Colonel in the Royal Engineers in December 1814 .
Following up his designs , he completed a work on ' Military Instruction ' in three volumes , of which the first was published in 1814 , and the second and third in 1817 .
The former contained the course of practical geometry before referred to ; the two latter a complete treatise on elementary fortification , including the principles of SX111 the science , and rules for construction , many of which apply to civil as well as to military works .
Finding , in 181 7 , that his men had been " most grossly ill-treated by the Army Bread Contractor , " he was led to inquire into the system under which the army was supplied with provisions ; and in 1825 he printed and circulated , but abstained from publishing , a volume containing the result of his investigations .
The exposure which he thus afforded of abuses that were prejudicial to the soldier , and the improvements that he suggested and was partly the means of introducing , were in themselves services of great value .
In 1818 , he published a volume of " Standing Orders , " containing a perfect code of military rules for the duties of all ranks in the army .
Colonel Pasley organized , during his residence at Chatham ` , improved systems of telegraphing , sapping , mining , pontooning , and exploding gunpowder on land and in water , and laid down rules which , being founded on careful experiment , will always endure , besides preparing pamphlets and courses of instruction on these and other subjects .
The volume which contained his ' Course of Practical Architecture ' was especially valuable .
His work on the 'Practical Operations of a Siege , ' of which the first part was published in 1829 , and the second in 1832 , is still a text-book , and the best that has been written in any language on that subject .
Every operation in it was treated as a separate study ; and it exposed various mistakes into which the French and German authors had fallen .
It was translated into French , and published in Paris in 1847 .
Early in 1831 Colonel Pasley prepared a pamphlet , and in May 1834 he completed a volume of 320 pages , entitled 'Observations on the Expediency and Practicability of simplifying and improving the Measures , Weights , and Money used in this country , without materially altering the present standards .
' He strongly advocated the adoption of the decimal principle of division in all its simplicity for our coinage , as well as for our weights and measures , and opposed with equal ardour the introduction of the French units into this country .
He sent to the press in May 1836 the first sheets of a work containing 'Observations on Limes , Calcareous Cements , Mortars , * In addition to these various occupations , he employed privates of Sappers to teach him the native Welsh and Irish languages .
Stuccos , and Concrete , and on Puzzolannas , natural and artificial , ' of which the first edition was published in September 1838 .
It contained considerable discoveries , the results of experiments at Chatham , and led at once to the manufacture in large quantities of artificial cements , under the different names of " Portland Cement , " " Patent Lithic Cement , " and " ' Blue Lias Cement .
" In connexion with experiments on the explosion of gunpowder under water , Colonel Pasley was led to undertake , and successfully to carry out , the removal of two sunken vessels from the bed of the Thames near Gravesend , in the year 1838 .
HIe received for this service the thanks of the municipal authorities , and was presented with the freedom of the City of London in a gold box .
Emboldened by the success of these operations , he proceeded to execute the more formidable task of clearing away the wreck of the 'Royal George ' from the anchorage at Spithead , and that of the 'Edgar ' from St. Hlelen 's .
The value of the materials recovered from these vessels was more than equal to the expense incurred in their removal .
Portions of six successive sumlners , from 1839 to 1844 inclusive , were devoted by him to this work ; but he never asked for nor received from the Admiralty any remuneration for the important seivices that he rendered in this manner to the navy and the nation .
Colonel Pasley remained at Chatham till the end of the year 1841 , when he was appointed , at the age of 61 , to the office of InspectorGeneral of Railways .
During the twenty-nine years and a half that he was at the head of the Royal Engineer Establishment , there was hardly any subject connected with his profession as a military man and an engineer-of instruction , construction n , or destruction-that did not benefit by his attention .
His presence there was of the greatest advantage to his country as well as to his corps .
The corps of Royal Engineers owes , in fact , its existence in its present condition , as well as its high state of efficiency , to his energy , his example , and his exertions ; and the success of the British army in many a field has been due in no small degree to the system of instruction at which he laboured so devotedly , and which he rendered so perfect .
As the latest example of the advantage of that system we may refer to the recent war in New Zealand , which was brought to a close mainly through the employment of Pasley 's methods , by officers ( one of them his own son ) who had been trained by him at Chatham .
The easy and bloodless capture of the native pahs , which resulted from a systematic employment of the spade , proved at once to their defenders the hopelessness of further resistance .
He became a Brevet-Colonel in 1830 , a Colonel of Engineers in 1831 , and a Major-General in the Army in 1841 .
He received the honorary distinction of D.C.L. at Oxford in 1844 ; and in 1846 , on relinquishing the appointment of Inspector-General of Railways , he was made a K.C.B. for general services .
IHe held the appointment of Public Examiner at the East India Company 's Military Seminary at Addiscombe for sixteen years , up to the year 1855 , and took an active part in its management , contributing materially to the high standard which it reached and at which it was maintained .
IHe was elected a Fellow of the Royal Society as far back as 1816 ; he was also of old standing in the Astronomical , the Geological , the Geographical , the Statistical , and other societies ; and he lost no opportunity of contributing to the advancement of practical science .
He was also a liberal subscriber to a great number of charitable institutions .
He held no public office after 1855 , but occupied himself chiefly in re-editing his works , superintending the construction of pontoon equipages , and in other matters connected with his profession , as well as in advocating the introduction of decimal coinage , devoting a large proportion of his time to the benefit or advancement of his friends and relations .
He was promoted to the rank of LieutenantGeneral on the 11th of November 1851 , and to that of General on the 20th of September 1860 .
He was twice married .
I-is first wife died of consumption in a few months , his second died in 1848 .
Of six children , three survive him .
He was well and hearty up to within a week of his death ; but his long life of labour was brought to a close at his residence at 12 Norfolk Crescent , Hyde Park , from congestion of the lungs , on the 19th of April 1861 .
JOHN T. QUEKETT was born at Langport , Somersetshire , in the year 1815 ; he was the fourth son of the late Mr. Quekett , head master of the Langport Grammar School , and received his early education in that establishment .
Being intended for the medical profession , he was sent to London and apprenticed to his brother , the late Edwin Quekett , lecturer on botany at the London Ilospital , at which institution he pursued his medical studies .
After passing the usual examinations , he , in June 1840 , obtained by competition the appointment of Student of Human and Comparative Anatomy in the Museum of the College of Surgeons , and at the expiration of the term of his appointment became Assistant-Conservator .
While holding these appointments , Mr. Quekett was enabled freely to follow his strong inclination for microscopical research , which had very decidedly shown itself in early youth ; and after having formed a most elaborate and valuable collection of specimens of the tissues of plants and animals , including numerous fine injections of the vessels , in preparing which he was remarkably skilful and successful , he was in 1844 appointed by the Council of the College to deliver annually a Course of Demonstrations , with a view to the exhibition and connected description of the collection , and the explanation of the method and resources of microscopical study .
This collection , numbering 2500 preparations , was purchased by the College .
On the retirement of Professor Owen in 1856 , Mr. Quekett was appointed Conservator of the Hunterian Museum , and also Professor of Histology , which appointments he held till his death , which took place at Pangbourne , in Berkshire , on the 20th of August , 1861 , at the early age of forty-six .
Mr. Quekett was the author of an elaborate treatise ' On the Use of the Microscope , ' published in 1848 , and speedily again in a second edition .
He also prepared the 'Descriptive and Illustrated Catalogue of the Histological Series contained in the Museum of the Royal College of Surgeons of England , ' the first volume of which appeared in 1850 , and the second in 1855 .
In 1852 he published a volume of ' Lectures on Histology , ' which was followed by a second in 1854 .
Besides these separate works , Mr. Quekett contributed numerous papers to the ' Transactions of the Microscopical Society , ' of which he was one of the founders , and , after labouring zealously in its service for nineteen years as Honorary Secretary , was elected President in 1860 .
He was a fellow of the Linnean Society , and was elected into the Royal Society in 1860 .
Although best known for his microscopical pursuits , Professor Quekett had devoted himself very successfully to the observation of facts throughout the whole field of natural history .
In original research the character of his mind led him less towards speculation than to the determination of facts ; and accordingly he has left behind him a rich store of trustworthy materials , the result of his acute and careful observation and faithful record .
His knowledge on all subjects of microscopic investigation was extensive and accurate , and he was ever ready to give the benefit of it to others , and especially to his numerous medical brethren , who continually sought his aid on questions determinable by means of the microscope .
Professor Quekett left a widow and four children , to whom the Council of the College of Surgeons , in consideration of his merits and services , have kindly and considerately granted a liberal pension .
FRIEDRICH TIEDEMANN , Foreign Member of the Royal Society , was born at Cassel , on the 23rd of August 1781 .
In his father , Dietrich Tiedemann , a Teacher in the Caroline College in Cassel , and afterwards Professor of Philosophy in the University of Marburg , he was not only blessed with an affectionate and watchful parent , but enjoyed the advantage of an accomplished and painstaking preceptor , to whose private tuition , indeed , much more than to the teaching of the school and gymnasium , he was indebted for his early educational training , and for a thorough grounding in classical studies .
While yet a boy at the gymnasium of Marburg , to which town his father and family had removed , the young Tiedemann showed a decided turn for those pursuits in which he was destined in after life to become so eminent .
He delighted in dissecting and preparing such animals as he could procure , and was thus naturally led to the pursuit of Zoology and Medicine .
In 1798 he accordingly entered the University of Marburg , where he remained until 1802 , diligently studying medicine and the auxiliary sciences .
The progress he made was , however , owing more to his own ardent love of the work he had undertaken than to the professorial teaching of the University , which , one or two chairs excepted , appears to have been at that time conducted in an irregular and slovenly way .
For better means of studying practical medicine he therefore went to Barnberg , where he made the acquaintance of Dollinger-and thence to Wiirzburg ; and having in the mean time returned to Marburg , he took his Doctor 's degree in that University in 1804 .
Tiedemann 's first essay as a teacher of anatomy was made in 1803 .
In the winter of that year he delivered the lectures and superintended the practical studies in the anatomical school of Marburg , as substitute for Professor Briihl , who was incapacitated by ill health ; and next year , being invited by the Professor , and prompted by his own inclination , he established himself as " Privatdocent " in the University , and gave lectures on Physiology , Comparative Osteology , and on Gall 's Craniology , which then attracted much attention .
Feeling , however , the need of further preparation , he went again to Wiirzburg to work at dissection under Hesselbach , and afterwards to Paris , where he studied hard in the great museum of the Garden of Plants , and attended the lectures of Cuvier , Geoffroy St.-ltilaire , Lamarck , Dumeril , and I-aivy .
On his way to Paris , Tiedemann had made the acquaintance of Soemmering at Frankfort , and gained his favourable opinion ; and now , through the recommendation of that great anatomist , who had in the mean time removed to Munich , he was offered the Professorship of Zoology and of Human and Comparative Anatomy in the University of Landshut .
This offer , flattering as it was to so young a man , he naturally accepted , and to Landshut he accordingly went in 1805 .
There lie found a new and handsome anatomical theatre , but no collection of preparations or other appliances for teaching .
Durinog the first few years of his incumbency therefore he had to labour hard to supply these wants , besides discharging his professorial duties , even to the temporary injury of his health .
The war between France and Austria having broken out afresh in the spring of 1809 , Landshut and its neighbourhood became the scene of active military operations , and Tiedemann , in addition to his regular duties , took charge of one of the temporary hospitals established in the place .
But in spite of the distractions of these troubled times he steadily pursued his scientific work .
In that same year appeared the first volume of his ' Zoologie , ' and in 1810 and 1814 the two parts of the second volume .
The author 's object in this work was to combine zoology with comparative anatomy , and to found the classification of animals upon their organization .
On the part which comprehends Birds he bestowed especial pains , and with a view to the preparation of it made numerous dissections , measurements , and observations of various kinds ; so that it is still valued as a rich store of information on the class to which it refers .
Two of his minor works , the ' Anatomic des Fischherzens ' and the 'Anatomicund Naturgeschichte des Drachens , ' having in the mean time appeared , Tiedemann in 1811 made a journey to the shores of the Adriatic to study the organization of the Echinoderms , a subject which had been proposed for a prize-question by the French Institute .
The issue of his labours was his great work on the Iiolothuria , Asterias , and Echinus , which gained the prize , established his reputation as a Zootomist , and brought him a nomination as Corresponding Member from the Academies of Paris , Berlin , and Munich .
The study of the brain-in its structure and development , its differences among animals , its characters in different races of mankind , its defects and deformities-was a subject on which Tiedemann bestowed much labour , both mental and manual .
In 1813 he published the ' Anatomic der Kopflosen Missgeburten , ' and in 1816 his well-known description of the anatomy and development of the Fretal Brain .
In this work he described the successive stages of development of the human brain , and showed the correspondence of these transitory conditions with its permanent conditions in animals lower in the scale ; and notwithstanding the great advances of this as well as other departments of embryology in later times , Tiedemann 's work is still held in high estimation .
These researches on the brain , so happily begun , were continued through many years of Tiedemain 's life .
The breaking up of the Grand-Ducal Menagerie at Carlsruhe afforded him the opportunity of dissecting several rare animals , and of publishing in 1821 the ' Icones Cerebri Simiarum .
' In 1825 he gave , in two memoirs published in the ' Zeitschrift fiir die Physiologie , ' a comparison of the brains of the Orang Outang and Dolphin with that of Man ; and he has left behind him a large collection of unpublished figures of the brains of animals , which , in the hands of his distinguished son-in-law Prof. Bischoff of Munich , may yet prove serviceable to science .
The comparison of the brain of the Negro with that of the Euro .
pean , to which he next directed his attention , became for Tiedemann a subject of keen interest .
After collecting all the materials to which he could find access on the Continent , he made a visit to England in 1835 , mainly for the purpose of making examinations and measurements of the brains and crania of different races to be found in British collections .
The fruits of these labours he presented to the Royal Society , of which he had a few years before been elected a Foreign Member , in a memoir entitled " c On the Brain of the Negro , compared with that of the European and the Orang Outang , " which was published in the ' Philosophical Transactions ' for 1836 , and appeared afterwards in German as a separate work in 1837 .
From his extensive researches , Tiedemann arrived at the conclusion that , whilst in the majority of cases the Negro 's brain is undoubtedly less than that of the European , there are nevertheless individuals of the negro race in whom the brain is as large as in the Caucasian ; and coupling this result with the fact , shown as he conceived by careful historical and literary inquiries , that there is no province of intellectual activity in which individuals of pure negro race have not distinguished themselves , he draws the inference that there is no impassable limit between Caucasian and Negro which should unconditionally denote the one as the master of the other .
In 1816 Tiedemann accepted a call to Heidelberg , where he undertook the Professorship of Physiology , as well as that of Anatomy .
His physiology was , like HIaller 's , founded on anatomy , observation , and experiment .
It is true that , while a student at Wiirzburg , he was for a time an ardent hearer of Schelling , in the hope of a new illumination of biological science through the German " Naturphilosophie ; 9 but his solid sense and the positive scientific progress he had already made soon led him to distrust the allurements of a vain system .
It was in this practical spirit that , at a riper age , he joined with the accomplished chemist Leopold Gmelin in those elaborate researches which ended in the celebrated experimental Essay on Digestion ( Die Verdauung , nach Versuchen , 1825 ) , in which the names of the anatomist and chemist are so honourably associated .
Tiedemann also entered on the laborious task of preparing a systematic work on physiology on an extended plan , somewhat after the manner of the ' Elementa ' of Haller ; and the first volume , embracing general physiology , was published in 1830 .
The issue of the third volume was prematurely forced upon him by the unauthorized publication of the corresponding part of his lectures ; but the work was not further proceeded with , and the part published , although full of learning , and displaying other excellencies characteristic of the author , and although it was translated both into French and into English , attracted comparatively little attention .
At that time , indeed , the revived and improved use of the microscope in physiology , the more exact application of physical experiment , and other influential causes were about to introduce a mass of new materials into the science , and to involve a fresh handling of the old in any systematic treatise that should be up to the actual state of knowledge ; and it is probable that advancing years and other cares indisposed the author to persevere in what had become an arduous task .
Tiedemann meanwhile did not intermit his labours in human and comparative anatomy .
He had , in conjunction with Oppel and Liboschitz , projected a work on the anatomy and natural history of Reptiles ; but , in consequence of the death of his collaborators , it went no further than the part on Crocodiles , which appeared in 1817 .
In 1820 he published a monography of the Ursine Sloth ; in 1822 his 'Tabulee Nervorum Uteri , ' which he dedicated to the Royal Society , and in the same year came out the Tabulee Arteriarum Corporis Humani .
' This grand work , though not exactly faultless in every point , has , more than any other , contributed to spread abroad the name of Tiedemann ; for the figures it contains have been reduced and copied and disseminated , in collections of anatomical plates and in anatomical systems and hand-books , in every part of the world where anatomy is taught .
A supplement , containing additional figures of varieties in the distribution of the arteries , was published in 1846 .
Besides the works noticed in this brief sketch , Tiedemann was the author of various minor essays and memoirs , published separately , or contributed to Transactions of Societies and Journals .
He was also associated with the two brothers Treviranus in conducting the 'Zeitschrift fur Physiologie .
' A complete list of his writings is appended to a memoir of his life read before the Bavarian Academy of Sciences , by his son-in-law Professor Bischoff , from whence the facts in the present notice have been mainly derived .
In 1807 Tiedemann married the daughter of the Obervoght of Rastatt , whose family name was von Holzing ; and with her he lived in happy union to the end of his days .
She bore him seven children , of whom three survive him .
Unhappily three of his sons were drawn into the revolutionary movement in Baden in 1848 , for which the eldest paid the forfeit of his life , and the other two had to exile them .
selves from their fatherland .
These deplorable events weighed all the more heavily on the old man , as his own political tendencies were strongly conservative .
Added to these family afflictions , a growing infirmity of his eyesight induced Tiedemann to withdraw from public duty , and to retire in 1849 to Bremen , and thence soon after to Frankfort .
There he met with a kind reception from numerous attached friends , and in 1854 he was honoured by the celebration of his " Doctor-Jubilaeum , " on the fiftieth anniversary of his promotion to the Degree of Doctor .
On this occasion not only his immediate friends and countrymen , but men of science in all parts of the world joined in the general testimony of respect ; and a medal , bearing his likeness , was struck in commemoration of the event .
Having recovered a very serviceable degree of vision by a successful operation for cataract , he continued to enjoy his retirement , and to gratify his passion for natural scenery in summer excursions among the Bavarian Alps ; but after a time he became subject to attacks of bronchitis , under which he finally sank on the 22nd of January , 1861 .
Tiedemann , besides a thorough acquaintance with the literature of his special department , possessed a large stock of accurate general information the fruit of diligent reading and personal observation , favoured by a singularly exact and capacious memory .
His private as well as his public life was characterized throughout by elevated sentiment , manly independence , and strict integrity .
We have already mentioned the special honour conferred upon him in his old age ; and as a further evidence of the esteem in which he was held , we may add that he was elected a member of no less than sixty-two learned Academies and Societies .
Hle was also raised to the rank of Privy Councillor by the Grand Duke of Baden , and received orders of Knighthood from Baden , Bavaria , Greece , and Prussia .
His election to the Foreign Memlbership of the Royal Society took place in 1832 .
OBITUARY NOTICES OF FELLOWS DECEASED BETWEEN 30TH Nov. 1861 AND 30TH Nov. 1862 .
PETER BARLOW , Esq. , was born at Norwich in October 1776 , and died at Charlton in Kent on the 1st of March 1862 .
After going through an ordinary school education , he chose mathematics as a special study , and obtained the place of Mathematical Master , and subsequently that of Professor , in the Royal Military Academy at Woolwich .
During the earlier part of his career he gave his attention chiefly to pure mathematics ; and his first original work was 'On the Theory of Numbers , ' which appeared in 1811 .
In that work he shows an acquaintance with the writings of foreign mathematicians to an extent at that time unusual .
In 1814 he published a Mathematical and Philosophical Dictionary ; also his well-known Mathematical Tables , which , besides other cognate matters of use and interest , gives the factors , squares , cubes , square roots , cube roots , and reciprocals of all numbers up to 10,000 .
This work having passed out of print , and a decided opinion being entertained by some discriminating authorities of the practical usefulness of its chief contents , the tables , so far as indicated above , the factors excepted , were republished in stereotype under the sanction of the Useful Knowledge Society in 1840 .
In 1817 Mr. Barlow published a work on the Strength of Materials , based on extended experimental inquiries carried on by himself .
In this way he was brought into friendly relation with the leading engineers and architects of his time , was much consulted in reference to important works of construction , and served on more than one Government Commission on great engineering questions .
He next turned his attention to the subject of magnetism in general , and especially to the deviations of the compass-needle caused by local attraction , and the best means of correcting it .
IHis researches form the subject of his 'Essay on Magnetic Attractions , ' published in 1820 , and of seven papers communicated to the Royal Society from 1822 to 1833 .
These labours of Mr. Barlow were so highly esteemed , and the method he devised for correcting compass-errors , although confessedly not perfect , was at the time deemed of so great practical value , that in 1825 he received the Copley Medal from the Royal Society " for his Various Communications on the Subjects of Magnetism .
" Mr. Barlow also applied himself to the improvement of achromatic object-glasses , and in 1827 communicated a paper on that subject to the Royal Society .
In the further course of his inquiries he was led to try the effect of substituting , for the flint-glass lens of the usual achromatic combination , a concave lens formed of transparent fluid enclosed in a glass capsule having surfaces of appropriate curvature .
The idea of employing fluid lenses , it may be observed , was not new : it had occurred to Newton and David Gregory , and had even been practically applied by Dr. Blair of Edinburgh .
Mr. Barlow made choice of sulphuret of carbon as the fluid , which , with a refractive power about equal , has a dispersive power more than double that of flint-glass .
He demonstrated the practicability of his method by constructing two telescopes on that principle , with a result sufficiently promising to obtain for him the support of the Board of Longitude in the further prosecution of his experiments .
The Council of the Royal Society also , seinsible of the important scientific bearing of Mr. Barlow 's proposal , engaged Mr. Dollond to construct a fluid-lens telescope under Mr. Barlow 's superintendence , and submitted the instrument to be practically tested by competent judges in order to decide on the expediency of constructing a telescope of much larger dimensions on the same principle .
The trial instrument is described by Mr. Barlow in the Philosophical Transactions for 1833 ; and Reports on its performance , by Sir J. Herschel , Mr. Airy , and Captain ( now Admiral ) Smyth , will be found in the Proceedings for December of the following year .
From the trials made , it appeared that Mr. Barlow 's principle might be advantageously applied to the construction of a great refracting telescope to be employed in the observation of nebulae and for certain other astronomical purposes ; but the project seems not to have been further proceeded with .
Besides publishing the memoirs and treatises mentioned above , Mr. Barlow during his active career was a large contributor to the 'Encyclopaedia Metropolitana .
' lie retired from the duties of his Professorship in 1847 .
In May 1823 he was elected into the Royal Society .
He was one of the original Fellows of the Astronomical Society , and a member of several of the leading Societies in Europe and America .
JEAN-BAPTISTE BIOT , the last of that powerful school of science which grew up during the first French revolution , cannot here be the subject of a detailed scientific biography .
The wide extent of his labours would alone render this difficult ; and when it is added that a large part of this extent contains matters in which the position of Biot and of others could not be discriminated in few words , difficulty merges in practical impossibility .
And this is rendered still more obvious when we state that we do not so much refer to actual points of disagreement commenced and continuing , as to matters in which anything short of a minute and cautious handling would probably create new discussions which had better find a natural origin in the statements of professed historians .
Of these matters some are of very old date , and may therefore be said to have passed into history ; while this very circumstance makes it more desirable to dwell especially upon the personal life of one who was born under Louis XV .
and lived to the age of eighty-eight in the full enjoyment of high faculties .
Of this personal life we are able to give some account from documents on which we can rely .
Biot was born at Paris , April 21 , 1774 .
His father , Joseph Biot , was an employ at the Treasury , whose ancestors had been farmers in Lorraine .
The son , after a classical education at the college Louisle-Grand , and some instruction in mathematics from Mauduit , was placed , against his wish , with a merchant at Havre , who employed him in copying letters by the thousand .
Disgusted with this occupation , he volunteered for the army as soon as the legal age of eighteen was attained , and served as an artilleryman in the army of the North at the battle of Hondschoote in 1793 .
Declining the promotion offered on condition of permanently engaging himself , he remained a few months , at the end of which a severe illness made him desirous of returning to his parents .
The military authorities were very slow about the dismissal of volunteers who were likely to be useful , so Biot took his departure for Paris , with nothing but his serjeant 's certificate , in September 1793 .
Walking feebly along the road , he was overtaken by a smartly dressed person in a cabriolet , who invited him into his carriage , and entered into conversation with him .
Finding that he was going to Paris , the stranger pointed out the danger of his purpose , a recent ordinance having made it death for soldiers to approach the capital .
Biot c persisted , and his companion then offered to take him all the way .
This stranger , whoever he was , gained their free passage through military posts , and sent patrols about their business by a mere whisper .
At Compiegne , the young volunteer was summoned before a revolutionary committee , then and there sitting , on the evidence of his uniform .
But his examination had hardly commenced when his companion entered the room in violent anger and addressed strong reproaches to the Committee , which were answered by humble apologies .
When they arrived at Paris , Biot desired to know the name and address of his protector , and was answered St. Just , Rue de la Michodiere , Hotel X. The story , one would suppose , ends here with full explanation of all that had taken place .
But when Biot , after an illness of several weeks , presented himself at the address given , he was told that no such person had ever lived there .
In later years Biot made many efforts to clear up the mystery , but never could get beyond a doubt .
So far the notes from which we write .
We add that it is notorious that the formidable leader of the revolution was on his way to Paris about the time in question , having been commissioner to the army of the North ; and he was the elegant which Biot describes his friend to have been ; but this was , of course , known to Biot .
It may be surmised that the person really was the colleague of Robespierre , who , knowing that the power he had shown would necessitate the inference that he was very high in the state , and render his detection easy , chose to give his real name , but also to hint that further acquaintance would be inconvenient , by giving a wrong address .
He was guillotined in July 1794 , so that Biot , enfeebled by illness , probably had no opportunity of seeing him in public .
Biot was admitted into the school of Ponts et Chaussees , and into the Polytechnic School at its opening .
He formed the acquaintance of Poisson , and the two became the favourite pupils of Monge .
But Biot , Malus , and some others who had smelt powder , took part in the insurrection of October 1795 , the suppression of which by grape-shot was the first very notorious achievement of Napoleon Bonaparte .
Biot found refuge at Melun ; but the names of the insurgent students were known , and they would have been expelled from the Polytechnic School if Monge had not interfered by the declaration that they were among his best pupils , and that if they were dismissed he would retire with them .
Monge was more than once the protector of the school .
The Emperor , when he gained this title , felt strongly that the students were his enemies , and seems to have meditated their dispersion .
" We had work enough , " said Monge to him , " to make them republicans ; give us a little time to form them into monarchists : you yourself must agree that you have turned that corner rather sharply .
" Napoleon did nothing : and he lived to call the school the goose which laid him the golden eggs .
Biot 's next step in life was to a chair of mathematics at Beauvais , At this place he gained the acquaintance and correspondence of Laplace by an offer to correct the sheets of the 'Micanique C6leste .
' He has given , in the Journal des Savans , an anecdote which is very honourable to Laplace .
While at Beauvais he married the sister of his friend Brisson , whose family resided there .
Neither had any money , either in possession or reversion ; so that all except lawyers will share Biot 's wonder when he found that the notary had contrived a contract of marriage twelve pages long .
Madame Biot had been very well educated , and the little stories and dramas which she wrote for her children were celebrated in her circle .
She learnt German in order that her husband , at the desire of Berthollet , might publish a French edition of Fischer 's work on physics ; but the actual translation , watched of course by her husband , was her own .
The first edition was published in 1805 .
In 1799 Biot was appointed an examiner of the Polytechnic School ; in 1800 he was removed to Paris as Professor of Physics at the College de France , and was made an associate of the Institute , of which he became a member in 1803 .
The other dates which we ought to give are as follows .
He was appointed , with Arago , to the continuation of the measure of the meridian , in August 1806 ; with Mathieu , to determine the pendulum at Bordeaux , August 1808 .
He became editor of the Journal des Savants , May 1816 .
IHe went to Scotland and the Shetland Islands for the measurement of the pendulum in 1817 ; to Dunkirk , with Arago , to act in concert with an English commission for the determination of the latitude , in 1818 ; to Illyria and the Balearic Islands , for the pendulum , and to Spain for the repetition of measures connected with the great survey , in 1824-25 .
He was made a Foreign Member of this Society in 1815 , and obtained the Copley Medal in 1840 .
IHe died at Paris , February 3 , 1862 .
The other dates , &c. of his life will be found , given by M. Lefort ( the son of his daughter 's daughter ) , in the ' Nouvelles Annals de Mathematiques , ' 2nd series , vol. i. The list of his writings , associated and separate , is under 477 heads ; and this list , says the collector , is certainly incomplete .
Of his separate works should be especially mentioned the 'Astronomic Physique , ' 1st ed. , 1805 ; 2nd , in 3 vols .
, 1810-11 ; 3rd , in 5 vols .
, 1841-57 ; the 'Traite de Physique Experimentale , ' 4 vols .
, 1816 ; the 'Precis ' of the same , lst ed. , 1817 ; 3rd , in 2 vols .
, 1824 ; 'Recueil d'Observations Geodesiques ' ( vol. iv .
of the 'Base du Syst'me Metrique ' ) , 4to , 1821 ; the edition ( in conjunction with M. Lefort ) .
of the Commercium Epistolicum , ' &c. , with additions , 4to , 1856 .
The works on Indian and Chinese astronomy can hardly be given apart , without the writings on the same subject in the journals .
H. ow completely Biot was devoted to his occupations sufficiently appears .
The indomitable energy of his character was associated with a strong feeling of personal independence .
With the pride of a republican he refused , before his election to the Academy of Sciences , to pay the usual visits of ceremony to his future colleagues .
This he afterwards regretted ; and , as a kind of expiation , he made it a rule , until at last his friends insisted that he should spare his extreme old age the fatigue , to pay a visit to every new member of the Academy , so soon as his election was made certain .
In 1803 , his son Edward was born .
This son , after a respectable career in science and engineering , took a dislike to such pursuits , and applied himself to literature , and especially to the study of Chinese .
He died in 1850 , a member of the Academy of Inscriptions , in which he found himself the colleague of his father ; for it should be noted , as a thing which is , we believe , unique , that Biot died a member of three of the four academies , being also elected to the Acad6mie Frangaise in 1856 .
The mother survived her son two years ; and these losses were the great misfortunes of the father 's life .
The name of Arago will always be associated with that of Biot .
Arago in his early youth ( he was but twenty-four years old when he gained his place at the Institute , after his return from captivity at Algiers ) had distinguished himself to an extent which induced Biot to make it almost a condition that the young man should be appointed his assistant , before he would undertake the conduct of the survey .
When a place in the astronomical section of the Institute became vacant , Poisson was thought of as a successor to Lalande , with every chance of success .
Biot protested , and urged strongly to both Lagrange and Laplace , that the astronomer ought to be a person conversant with astronomy , and that Poisson 's future chair ought to be one of geometry .
Lagrange gave way at once " Vous avez raison , " he said , " c'est la lunette qui fait l'astronome .
" Laplace was harder to convince , but yielded at last .
In 1809 Biot obtained those apartments in the College de France which he occupied with hardly any intermission until his death .
We have heard it said that he never left Paris for one single night during fifty years : this is probably not literally true , but is certainly very near it .
In the same year ( April ) an imperial decree named him professor of astronomy in the new University then founded .
Biot had not been an Imperialist ; and the appointment was a free testimony to his merit .
In 1804 he had endeavoured to prevent the Institute from expressing an opinion in favour of the new regime , on the ground that a scientific body should not meddle with politics : this opinion he always maintained .
The police were well aware that he had assisted Benjamin Constant , Andrieu , and perhaps other frequenters of the house of Madame de Stal , in the composition of a satirical piece which had great success in such private circulation as could be safely given .
Fouche had charged Laplace to tell his young friend to be a little less witty and a little more prudent .
Biot , as might be expected , obtained no very great patronage from the Emperor .
He had a turn for dry satire , which , under very effective restraint , is visible in his controversial writings ; and he had the mode of delivering a sarcasm which tells .
In 1800 , Roederer , then high in the direction of public instruction , paid a visit to the College de France , and , surrounded by the professors , read them a lecture on their functions , recommended practice in preference to theory , and pointed out geometry and algebra as not good for much .
" Cependant , " quietly remarked Biot , " la geomdtrie a du bon pour l'arpentage , " to which the other was unfortunate enough to assent in a manner which showed he did not understand the answer .
The amusement which this excited led Laplace to tell the story to the First Consul , among whose few objects of reverence the mathematics stood very high .
Roederer accordingly had to encounter one of those bourrasques by which Napoleon is so well known .
" You are a pretty ignoramus not to know that mathematics is the root of human knowledge .
The young man served you right when he turned you into ridicule ; and you could not even see what he was at .
" If such anecdotes appear to be unusual in our notices , it may be remembered that these accompaniments would , in most cases , be of too recent a character .
We insert nothing but what is more than half a century old , and we proceed to a few words on Biot 's scientific life .
Over and above separate works , fifteen in number , the scientific life of Biot is recorded in 60 articles of the Journal Philomathique , 119 of the Comptes Rendus , 3 of the Journal of the Polytechnic School , 8 of the Connaissance des Ters , 41 of the Annals de Chimie , &c. , 22 of the Memoirs of the Academy , 1 of the Savans Etrangers , 83 of the Journal des Savans ; and of accounts and criticisms , 37 in the Moniteur Universal , 35 in the]Mercure de France , 1 in the Journal des Debats , 5 in the Journal des Mines , with 23 articles in the Biographie Universelle , 9 in the Memoires , &c. d'Arcueil , 1 in the Academy of Inscriptions , 2 in the Revue Britannique , 6 in the Revue ou decade Philosophique , &c. , and 8 in the Nouvelles Annals du Museum d'Ilistoire Naturelle .
In this large mass of results the author appears as an observer and experimenter , as a critic and historian , and as a teacher and elementary writer .
As an astronomical and geodetical observer , Biot has long had his place in history ; to discuss that place would require the discussion of critics , historians , and subsequent observers .
As an experimenter , we cannot undertake to describe that long train of which Professor Forbes , in his elaborate sixth dissertation of the 'Encyclopaedia Britannica , ' says " the number and variety of his experiments and writings almost baffles enumeration .
" There is no part of physics into which he did not carry his researches ; but of all he was most devoted to optics .
Here the point which has been most signalized by historical writers is the effect of the rotatory action of fluids , to which he attended for forty years .
All acknowledge the sagacity , perseverance , and honesty which are conspicuous in this prominent part of Biot 's life , as in others .
As a critic and historian , Biot 's field of labour was even wider than that of his life as an experimenter and observer .
I-ad he published nothing whatever except his papers on Egyptian , Hindoo , and Chinese astronomy , he would have been known as an inquirer the amount of whose labours was fully equal to that of several whose reputation is entirely founded upon oriental astronomy .
IIad he produced nothing except the long series of articles on contemporary science and history of science which adorns the Journal des Savans , he would have been remarkable as the most continuous and varied scientific critic of his time .
And in all these articles there is a close and discriminating production of the whole subject , relieved by legitimate satire , and by a tone of occasional pleasantry which is the true vehicle of certain parts of good criticism .
Three volumes of 'Melanges Scientifiques et Litteraires ' were published in 1858 ; but it may be hoped that this will be superseded by a more complete reprint .
It is natural that a notice in these pages should make allusion to Biot 's part in a controversy which , more than any other , concerns this Society : we mean the never-ending question of Newton and his opponents .
From the time when the life of Newton appeared in the ' Biographie Universelle , ' its author was what we may here call the chief of the opposite party .
His views were strong , and ably supported ; his mode of opposition was fair and downright .
Biot was one of those disputants who cannot fail to forward sound conclusion , take which side they may .
As an elementary writer , this country is under especial obligations to Biot .
In 1816 , just after the termination of the long struggle which had isolated Great Britain from the continent , he produced those treatises on physics , full and abridged , which laid all the recent physical improvements before those who could not have sought them in scattered organs of announcement .
Very many of those whose youth belongs to this period will remember Biot 's 'Traite ' and especially his ' Precis , ' as the first sources of their acquaintance with modern experimental methods and results .
The treatise on astronomy , not so much known in this country , filled up a void which had been left open in the large mathematical work of Delambre .
It is not often that a death at the age of eighty-eight leaves a blank in the scientific world ; but this must be said of Biot .
To the end of his long life he was in perpetual activity .
A volume on Indian and Chinese astronomy appeared in 1861 , closing the list which began with C Elements of Arithmetic , " prefixed to Clairaut 's 'Algebra , ' in 1797 .
WILLIAM BORRER , Esq. , the eldest of the three sons of William Borrer , Esq. , of Parkyns-manor , Hurstpierpoint , was born at Henfield in Sussex on the 13th of June 1781 .
He passed his long life in the country , discharging the duties incident to a landed proprietor and county magistrate , and earning the respect and attachment of his neighbourhood for his well-considered acts of local beneficence .
Amidst his rural occupations Mr. Borrer found ample scope for the pursuit of botany , to which he was enthusiastically devoted , and earned for himself a considerable reputation among British botanists for his extensive and accurate knowledge of indigenous plants .
To the great repertory of that species of knowledge , the 'Enlglish Botany , ' and especially to the Supplement of that work , he contributed valuable materials ; and , in association with his friend Mr. Dawson Turner , commenced a 'History of British Lichens , ' which , however , was stopped in its progress by the death of the printer and other untoward circumstances .
After lying dormant for a quarter of a century , the fragment of this work actually printed was brought out by Mr. Turner for private circulation , and mainly , as he expresses himself , that it might serve as a monument of Mr. Borrer 's industry , ability , and profound knowledge of the family of plants to which it refers .
Mr. Borrer was elected into the Royal Society in 1835 .
IHe was also a Fellow of the Linnean Society and of the Wernerian Natural History Society of Edinburgh .
He died on the 10th of January 1862 .
The life of our late President , SIR BENJAMIN COLLINS BRODIE , Baronet , Serjeant-Surgeon to the Queen , has not been ended long enough to allow even those who are best acquainted with it , fully or , perhaps , correctly to estimate its precise value .
There is no profession where a man may in his lifetime be so distinguished , and leave behind so slight record of his life , as the profession of Medicine or of Surgery .
With the death of the man there perishes in such case a vast amount of personal skill and observation , which , being unwritten , and indeed not capable of being written , can be amassed again only by the combination of similar talent , opportunity , and industry in another individual .
Nor is even this always possible .
There are epochs in human knowledge as in human affairs ; and a man may so turn to account the peculiar circumstances of his epoch as to attain not only just celebrity , but a certain masterly power which he could not have attained without such a combination of events .
Such considerations must be present to our minds if we would form a correct estimate of Sir Benjamin Brodie .
He furnishes a rare instance of a man who , having in early life had no particular advantages on the one hand , nor any great drawbacks on the other , obtained the highest place in a learned profession , as well as the greatest honour which English Science can bestow on a scientific man the Presidency of the Royal Society .
A brief record of his progress , considered not only as that of an adept in science and a master in the noblest of arts , but as a man , will be well worthy a place in the ' Proceedings ' of the Royal Society -a Society which is not only directly concerned in advancing human knowledge for its own sake , but indirectly also in interesting the most complete minds in the advancement of that knowledge .
It must set a special value on the example of one who proved to demonstration , by a long and admirable career , that devotion to purely scientific pursuits , and a deep interest in all that concerns scientific progress , may coexist with eminent professional skill , with a philanthropic spirit , 'and an enlarged religious mind .
Benjamin Collins Brodie was born in the year 1783 , at Winterslow , in the county of Wilts .
His father was Rector of the parish .
He had three brothers and two sisters , being himself the fourth child .
His father was a man of energy and ability , and brought both to bear on the education of his children , in whose well-being he took the deepest interest .
He instructed them himself ; by his own example he trained up his children in habits of industry ; above all he taught them in many ways from their earliest years to think and act for themselves .
Sir Benjamin would often state the great advantage he had derived from being called upon at the age of sixteen to join in managing a volunteer corps at the period of the first anticipated French invasion in 1798 .
The difficulties of communication , and the whole condition of the country , made such a task more arduous , and therefore more instructive , than a young man would find it at this day .
But this occupation did not distract him from those studies which there has been a tendency of late years to decry .
In after life he often looked back with satisfaction to the labour he had bestowed on committing to memory passages of the Greek and Latin authors , and of our own chief poets ; he would tell how , in long professional journeys , before the days of railroads , he had been cheered by the recital of them ; and he would point out how he believed the imaginative faculty , so essential to any great artist , be his art what it may , had been disciplined as well as fostered by early industry in ordinary classical studies .
Being naturally , or from a sense of duty , a studious boy , he , of his own accord , amassed , in leisure hours spent in his father 's library , a great variety of knowledge ; and he even then acquired a taste for those psychological speculations which shed a genial glow over his later days , when the labour of life was over and when his mind dwelt with serene delight on the contemplation of those higher qualities which are the peculiar property of man , and which are strengthened or impaired according to the use made of them by each possessor .
Thus prepared , in the autumn of 1801 our future President entered such a school of medicine as sixty years ago London afforded .
He had no special predilection for either medicine or physical science .
The arrangements of his family , rather than an active choice , led him to adopt his father 's suggestions as to his future profession .
He had already acquired a taste for work as such , he knew that he had to strive for his own maintenance , and forthwith betook himself with rational zeal to the selected study .
Had his lot engaged him in the study of some other subject-matter than medicine , that other subject would assuredly have been equally mastered by the same steady grasp , and elucidated by the same clear mind .
It is not easy for one conversant only with the existing appliances for medical instruction to appreciate the circumstances of a lad who was sent to walk the hospitals in 1801 .
At present the work of a student is regulated , or over-regulated-is divided into many subjects , so many lectures being assigned to each .
There is the first year 's work and the second year 's work , under an arrangement so systematic that the young student , whatever be his capacities or his previous training , is allowed only to join the stream , and therein is hurried on too fast if slow of apprehension , or wearied by useless attendances if quick beyond the average .
The freest scope was then given to the able and well-disposed-too free by far for the careless or dissolute .
Brodie , nurtured hitherto only by his father 's polished care , the companion of the Rector 's walks , the popular subaltern of a volunteer corps in a county far from the metropolis , reaches London , and is thrown at once upon opportunities so ruinous to some , so good for him .
HIe was not without good advice as to his future course .
Dr. Denman , Dr. Baillie , and Sir Richard Croft , eminent and admirable men , were connected with his family by marriage .
IIe was sent to Abernethy 's lectures on anatomy .
If in these lectures details were absent , the deficiency was compensated for tenfold by the genius and heart of the man .
Abernethy gave to his pupils what the living teacher can best give , a living interest in their work .
The Student was fascinated .
He determined on following the profession recommended by the example of that popular Surgeon ; for he found that he could not be a Physician without a university degree ; and this had not been provided for him .
Brodie 's character and training must have made parts of his early medical studies irksome , and some of his companions distasteful to him-though in this he only shared the lot of other rightminded youths who come from virtuous homes .
Nor can it be doubted that the shock which he must have experienced sixty years ago at the low education and unformed habits of mind of some of his class companions , helped to implant in him that strong , it may be said parental concern in all that affects the best interests of medical students , which characterized him up to the last days of his long and active life .
It is , however , true that , devoted , as his subsequent career proves , to his purely professional studies , he was not dependent on the medical school for his companions .
His literary tastes did not desert him .
He studied in this year the writings of various masters in mental philosophy--of Dugald Stewart , Berkeley , Locke .
He belonged to a literary debating Society , of which Lord Campbell , then young , was also a member ; and as evidence of the subjects there occupying his mind , it may be stated that he read essays on the advantages to be derived from metaphysical inquiries , and on the supposed modern discoveries which are to be found forestalled in Pliny 's 'Natural History .
' This comprehensive view of the subjects , both proper and useful in the formation of a large professional mind , was never altered .
In the most active period of his life he is known to have examined , with care and interest , the scientific papers in the early volumes of the ' Transactions ' of this Society ; and still later to have increased his acquaintance with the older medical and surgical writers .
In this year and the following he dissected at Wilson 's School of Anatomy , worked at pharmacy in the open shop of an apothecary , and did not enter St. George 's Hospital till 1803 .
At the Hospital the youth immediately ripened into the man .
Though he would even then look wistfully at literary pursuits , and kept up constant intercourse with literary men , he here first learned to apply the mental instrument , which hitherto he had only whetted , to the material on which for half a century it was henceforward to work .
He first watched his teachers as they played before him the solemn and weighty game of Therapeutics , " life being the stakes ; " and then , unceasingly in the wards , he studied by himself with avidity the accidents and injuries to the human frame which he had pledged himself henceforward to strive to alleviate or avert .
He wrote full notes of what he observed .
They who know his terse mode of expression , know how clearly he thought , how exactly , how simply he recorded what is essential , and how he discarded everything that is irrelevant .
Though so intent on clinical study , his well-poised mind did not relax its hold on scientific work .
He seized now the opportunity of teaching anatoly , and continued for many years to employ his powers in this manner .
I-e attended few lectures ; there were , happily for him , few to attend .
He read few professional books ; there were not many worth study .
I-e dissected , observed , recorded , taught .
he worked at anatomy for and with Sir Everard Home , not only as it bore on surgical practice , but as a science , pursuing it ( as Hunter had done ) into higher physiological questions , and into the comparison of organ and function throughout the animal series .
Here he received much help from Mr. Clift , the faithful and excellent Conservator of Hunter 's preparations .
It was about 1806 that his connexion with the Fellows of the Royal Society may be said to have begun .
Through Home he made the acquaintance of Sir Joseph Banks , and ( as the few who remember the liberality and kindness of that illustrious and useful man will well understand ) met in his society the galaxy of scientific persons who early in this century flocked daily to his residence in Soho Square .
In after days he used to refer to the advantage he had derived from his early acquaintance with Davy , HIatchett , Wollaston , Brown ( the botanist ) , Dryander , Dr. Young , and others .
He had been always shy , and was still nervous ; modest , yet not without ambition : as he listened to the discourse of these men , and admired the consummate fitness of Sir Joseph Banks for his high station , he probably little thought that he would himself be called upon at a future day to occupy the same distinguished post .
I By these several means he thus early gained a complete appreciation of what was needed to understand the nature of the diseases which oppress mankind , of the relative importance of clinical observation , pure science , and philosophical culture , in procuring alleviation of physical suffering .
One can imagine the sadness , the almost bitterness of spirit which a man so disciplined in youth must have felt when , full of years and rich in vast experience , he felt himself called upon to leave as one of his last legacies to his countrymen his manly answer* to some of the ill-grounded fallacies which fashion supports under the guise of medicine imrproved and reformed .
In 1808 , at the age of not quite twenty-five , he became Assistant Surgeon to St. George 's Hospital ; and he continued in the direct service of the hospital for full thirty years .
The absence of one of his seniors at once threw the charge of many in-patients on his hands .
On these he bestowed the most assiduous care , and lectured on the most important cases .
He had declined on a former occasion to give lectures on surgery , because he could have only given secondhand , or book knowledge .
But he now was able to draw his pictures from the life ; he began not only to lecture in the hospital clinically , but , with Mr. Wilson , in Winldmill Street , to teach systematic surgery ; and he continued to do so for nearly twenty years .
His mode of instruction was then more peculiar than it would be now .
His object was , as Abernethy 's had been , not to gain applause , but to teach the pupils .
IHe found this could not be done by reading out his lectures ; and he soon accustomed himself , as all great teachers do , to pour forth his knowledge , previously arranged and digested it is true , but flowing at the moment spontaneously and unconstrained .
At this time ( 1810 ) his Anatomical Lectures became more frequent ; and he was engaged in preparing his work for the day following till three or four in the morning .
When not so engaged , he sought instruction and recreation with his literary and other friends ; and , strange as it may seem to those who do not see the bearing of scientific study on practical work , he continued his researches on philosophical anatomy with Clift and Home .
He also undertook some original physiologicai investigations , the results of which were communicated to the Royal Society , he having been elected a Fellow in 1810 .
The object of these communications deserves consideration .
It has been remarked that it is an instinct of genius not only to suggest what work can , but what work cannot be attempted with advantage , in other words , that intellectual efforts are not made by great minds except in cases when they will succeed .
Brodie 's physiological researches " On the Influence of the Brain on the Action of the Heart , and on the Generation of Animal Heat , " were made in 1811 , fifty years before his death , His mind was keenly alive , as we have seen , to the value of purely scientific research , without any regard to the immediate utility ( so called ) of the inquiry .
On the other hand , the relief of suffering and the prevention of disease were the cynosure of his life .
The four important essays which appear in our Transactions-viz .
, the one just alluded to , with its sequel ( published in 1812 ) , and two on the " Mode in which Death is produced by certain Poisons " ( one printed in 1811 and the other in 1812)-all give a clue to the large views of the young surgeon .
I-e goes straight to the cardinal points to be noted in the apparatus for the maintenance of life , and inquires into some of the crucial instances in which death is rapidly produced .
The mutual relation between the nervous system , which is the organic differentia of animals , and the circulatory apparatus which gives the basic conditions of nutrition in the higher animals , occupy his mind in the first two Essays .
In the second he was aiming at the solution of one part of the question of questions for physiologists , how poisons operate on vital organs so as to produce death .
These , his first papers , were composed with great clearness , and based on well-devised experiments .
They do not exhaust subjects then only opening ; for they have both been carried forward by various able inquirers in the half century that has now elapsed since he wrote them .
But Brodie proved the correctness of the opinion advanced by Bichat and Cruickshank , that the cessation of the heart 's action depends , not directly on abstraction of the influence of the brain , but on the cessation of respiration ; and he showed that , to some extent ( though to what extent and in what way is not even now certain ) , the maintenance of animal heat is under the influence of the nervous system .
The most important of his experiments on poisons were those which he made with the Woorara .
They showed that the poison is first absorbed through the blood-vessels , and so acts on the nervous system ; that in consequence of the paralysis thence ensuing , the respiratory organs cease to act ; and that the failure of respiration leads to cessation of the heart 's action , and suppression of the circulation .
Accordingly it was further shown that if respiration be artificiallyperformed , the heart will continue to act , and the blood to circulate ; and that if the process be carried on for a sufficient length of time , in some instances the brain will recover , and life will be maintained without perceptible impairment .
Brodie appears also to have been the first to show that the Antiar poison of Java operates by primarily arresting the action of the heart , and that it thus offers a remarkable contrast to the class of poisons to which the Woorara belongs .
The Copley Medal was awarded to Mr. Brodie for the former set of observations in the year 1811 .
It is noteworthy that at this period he was an active member of two small societies , to one of which , the Animal Chemistry Club , Ilumphry Davy belonged , while of the other , the Society for the Promotion of Medical and Chirurgical Knowledge , John Hunter had been one of the original members .
I-e began about this period to be a frequent visitor at Holland House ; and he has often been heard to speak of the benefit he had derived from the society of the great statesmen , literary men , artists , and other eminent persons whom he there met .
In the year 1813 he delivered the Croonian Lecture on the effect of the Nerves on the Heart and on the involuntary Muscles .
With characteristic modesty and his usual thoroughness of purpose , he requested that , as the subject required further inquiry , it might not be printed .
His mind was still bent on the significance of the higher vital phenomena in animals ; for in the following year ( 1814 ) another paper was printed in our Transactions , " On the Influence of the Nerves of the Eighth Pair on the Secretions of the Stomach .
" In 1816 he instituted experiments on animals to determine the effect of the bile on chylification .
His conclusion , that it is essential to that process , has been since disputed ; but it is still probable that the earlier investigator was as near to the truth as his critics .
He afterwards lectured on Comparative Anatomy for four years at the College of Surgeons , from 1819 to 1823 , bringing to bear the stores of knowledge he had previously acquired when working with Mr. Clift and Sir Everard HI-ome .
With these last lectures his active physiological studies must be considered to have closed .
But so trained was he in scientific pursuits , that his eager interest in anatomical and physiological questions , and in the philosophy of his art , never left him .
Henceforward not only his duties at St. George 's Hospital , and to private patients , but also his inclination led him to devote his whole powers of investigation to those alterations in the living body which constitute disease .
The unsatisfactory state of surgical knowledge , and therefore of practice , in regard to affections of the joints , attracted his attention , and he at once hit on a principle which was a guiding maxim to him in after life .
Finding how little could be made out of a disease by dissection of the parts where organic alteration was far advanced , he used to examine the joints of those who had died of other diseases , in order to find the first traces of future injury .
At the end of two years ' assiduous inquiry , for which he had great opportunities , he felt at liberty to communicate to the MedicoChirurgical Society some observations on the question* .
To these he added in the following year t. These papers form the basis of his invaluable work on Diseases of the Joints .
His nice discrimination of the tissues affected , and of the exact value of pain in the joints as evidence of organic disease , has altogether altered the practice in such cases , and has tended greatly to reduce the number of amputations .
What a reflection for a man at the close of life !
To pursue further the details of his active professional life belongs to the purely Medical biographer .
Here it need only be said that he published , besides the work on Diseases of the Joints , three other surgical volumes , and contributed numerous papers to the 'Transactions of the Royal Medical and Chirurgical Society , ' and that he did not cease to lecture on surgery at St. George 's Hospital , with more or less frequency , till 1843 , his instruction being sought with avidity , for it was simple and drawn from the life .
None who heard him can forget the graphic , yet artless , manner in which , sitting at his ease , he used to describe minutely what he had himself seen and done under circumstances of difficulty , and what under like circumstances he would again do , or would avoid .
His instructions were illustrated by valuable pathological dissections which during many years he had amassed , and which he gave during his lifetime to his Hospital .
The threefold character of scientific man , author , and surgeon , thus early formed , was maintained till his sight failed shortly before his death .
A few words must be said on his qualities in each respect .
As a scientific man his several works were marked by distinctness of purpose , adaptation of means to end , and rigid determination to conclude no more than observation completely justified .
Iis relations to other scientific men may be best understood by recalling the just , courteous , and candid manner in which he conducted the business of the various societies whenever he was called upon to preside , and the lucidity with which he kept the main points before a meeting .
He always advocated and supported open discussion , and in this way did good service to the Royal Society .
As an author , he was not voluminous ; nor did he speak much in public .
He discarded all arts of style , aiming solely at precision and brevity : he wrote as he spoke , only when duty called , or when there was something which he believed he could write or say well .
He was well versed in the literature of his profession and of those sciences which interested him ; but he had not much love for books as instructors in his calling , because he knew that observation and d reflection were of more service than reading for the formation of the scientific mind , and original knowledge more valuable than that which is secondhand .
Ile himself used books and so advised younger men to use them rather to gain the knowledge of what had been done , and as an aid towards actual observation and reflection , than thereby to educate themselves .
His belief that observation , practice , and thought are the chiefest means for self-training in science partly accounts for the brevity of his published works , and greatly enhances their value .
As a surgeon , he was remarkable from early life for the scrupulous care which he bestowed on the investigation of the cases entrusted to him .
This obtained for him in a few years rare quickness as well as precision in the formation of his opinion .
VWhen Sir Astley Cooper 's practice declined , he was for many years extensively called upon to act as an operator .
He excelled in that department of his art ; for he had every requisite for success-knowledge , coolness , and the quick imagination which prepares for almost all possible emergencies that can occur , and suggests at once expedients when any come unforeseen .
He did not , however , give the highest place to this part of his professional duties ; for , in an occupation in which intellectual power and practical skill are combined , he valued those parts the most in which the most intellectual power is evoked .
At the same time he was ready and ingenious in mechanical contrivances , and had the neatness and the method so requisite for a good surgeon .
It was characteristic of his mind , that , among a few valuable lectures on some important subjects which he collected into a volume , he has given a place to one on Corns and Bunions-showing that in his judgment a small evil which can produce great annoyance requires as much consideration in its turn as more serious disorders .
In truth , as the great aim of his life was to prevent or to cure disease , that which was curable , though trifling , would in one sense attract his notice more than that which was already irremediable .
At the same time his difficulty in coming to the conclusion that there was nothing to be done , in even the gravest case , was a marked feature in his hopeful mind .
But the character of Brodie can be only properly considered as a whole .
Neither as scientific man , nor as surgeon , nor as author was he so remarkable as he appears when viewed as he was-a complete man necessarily engaged in various callings .
It was impossible to see him acting in any capacity without instinctively feeling that there he would do his duty , and do it well .
Nor could he be imagined in a false position .
A gentleman , according to his own definition of that word , " he did to others that which he would desire to be done to him , respecting them as he respected himself .
" Simple in his manners , he gained confidence at once ; accustomed to mix with the poorest in the hospital and with the noblest in their private abodes , he sympathized with the better qualities of each-valued all , and despised nothing but moral meanness .
Though as a boy he was retiring and modest , he was happy in the company of older persons , and , as he grew older , loved in his turn to help the young .
" I hear you are ill , " he wrote once in the zenith of his life to a hospital student of whom he did not then know much ; " no one will take better care of you than I ; come to my country house till you are well ; " and the student stayed there two months .
le was thought by some reserved-he was modest ; by others hasty-he valued time , and could not give to trifles that which belonged to real suffering ; he was sometimes thought impatient , when his quick glance had already told him more than the patient could either describe or understand .
Unconscious of self , of strong common sense , confident of his ground or not entering thereon , seeing in every direction , modest , just , sympathetic , he lived for one great end the lessening of disease .
For this object no labour was too great , no patience too long , no science too difficult .
He felt indeed ( to use his own words on the day of his election as President ) " his happiness to be in a life of Exertion .
" As a professional man he valued science because it so often points the way to that which is practically useful to man ; but as a scientific man his one object was the Truth , which he pursued for its own sake wholly irrespective of any other reward which might or might not follow on discovery .
He had not the common faults of common men , for he had not their objects , nor their instinct for ease , nor their prejudices : though he became rich , he had not unduly sought riches ; though he was greatly distinguished , he had not desired fame ; he was beloved , not having courted popularity .
What he was himself , that he allowed other men to be , till he found them otherwise .
He saw weak points in his profession , but he saw them as the debris from the mountains of knowledge and of wisdom , of benevolence and of self-denial , of old traditional skill ever growing and always purifying , -those eternal structures on which are founded true Surgery and Medicine .
If ever he was bitter in society , it was when they were undervalued ; if ever sarcastic , it was when the ignorant dared assume to judge them .
A light is thus thrown on his even career of uniform progress .
Training his powers from youth upwards , by linguistic and literary studies , by scientific pursuits , by the diligent practice of his art , by mixing with men , he brought to bear on the multifarious questions which come before a great master of healing , a mind alike accustomed to acquire and to communicate , a temper made gentle by considerate kindness , a tact that became all but unerring from his perfect integrity .
He saw that every material science conduces to the well-being of man ; he would countenance all , and yet be distracted by none .
He knew the value of worldly influence , of rank , of station when rightly used ; he sought none , deferred excessively to none ; but he respected all who , having them , used them wisely , and accepted what came to himself unasked , gave his own freely to all who needed , and sought help from no one but for public ends .
A few words only may be added on the inner life of his later days .
Those who knew him only as a man of business would little suspect the playful humour which sparkled by his fireside the fund of anecdote , the harmless wit the simple pleasures of his country walk .
Some , who knew these , might not have imagined another and deeper current which flowed unheard when neither the care of his patients nor his literary pursuits or memories engaged his mind .
He who from his early professional life sat down every night , his work ended , his notes entered , his next day ordered , to ask what could have been better done today and what case otherwise managed , was not one to reach threescore years and ten without a keen onward gaze on the entire destiny of man .
Yet he who realized in his profession the answer of Trophilus the Ephesian to the question , Who is a perfect physician ?
-"he who distinguishes between what can and what cannot be done " -such a man would not dogmatize on what cannot be known , nor would he , so humble , attempt to scan the Infinite .
But his nature yearned for some better thing to come ; and yearning , it became satisfied .
HIe had for many years thought and conversed among his friends on facts he had noted in relation to our mental organization .
In the year 1854 , he published anonymously a volume on Psychological Inquiries .
This was followed by a second , with his name , in 1862 .
These volumes contain little that is actually new to professed psychologists ; but they are the conclusions of one who had thought and workedvariously , consistently , practically .
Living not in the closet , but hearing the opinions of every party and of every kind of menliberal in all his views-without prejudice , and ever open to conviction , yet tinged with a general dislike to change as such , -he tells in these volumes what he had concluded concerning the mind of man -its laws , its discipline , its future state .
They therefore who value such a character will prize these writings for qualities other than the novelties they may contain .
It will be remembered that the scientific inquiries of his early life related to the influence of the nervous system on certain parts of the animal economy .
To the ordinary physiologist this may be a purely material question ; to him it was not so .
In middle life he said to a friend , speaking of his lectures on the Comparative Anatomy of the Brain , " the complexity of the mechanism of the higher brains is enough to make one giddy to think of it .
" A fortnight before his death he talked to the same person of this mysterious link between our consciousness and our visible material organization , descanting with keen interest on the relations between mind and body , and the mutual reactions of one on the other .
As he then lay on his sofa almost for the last time , in great pain , having scarce for many months seen the outer world which had been so much to him , and to which he had been so much , he spoke freely of our ignorance as to many things which it would be a joy to know-of the existence of evil-of the too little attention which philosophers had paid to the terrible nature of physical painof the future state .
So gathering up the teachings of his useful life , and still , as ever , looking forward , he waited its close .
Not many days after this he breathed his last , at Broom Park , on October 21 , 1862 , in possession of the full calm power of his disciplined mind to within a few hours of his death .
Such was our late President .
They who knew and honoured him may excuse , while they accept , a delineation too feeble for so complete a man .
In the quality of his mind he was not unlike the most eminent of his contemporaries , Arthur Duke of Wellington .
Those who did not know him , and who do not appreciate the power requisite to make such a master in medicine as he was , may be surprised at the comparison .
Yet our great soldier might have accepted the illustration without dissatisfaction .
Whatever art Brodie undertook , if he has been correctly drawn , he would have entirely mastered .
The self-discipline of the strongest man can effect no more .
The care with which the two men compassed every detail and surveyed every bearing of a large question , the quiet good sense , the steadiness of purpose , the readiness of wide professional knowledge in critical emergencies , were in each mind alike .
The public and his profession esteemed Brodie as the first in his art .
lie advised three successive Sovereigns , and from one had the only other mark of esteem which a Sovereign can bestow-a Title .
He was made a Corresponding Member of the French Institute in 1844 , and received the Honorary Diploma in Civil Law from the University of Oxford in 1855 .
IIe was elected the President of the Royal Society in 1858 , and became the first President of the Medical Council under the Act for regulating the Education and Registration of the Medical Profession ; but he resigned both offices in two years , on account of the advancing failure of his eyes .
It remains to be recorded that in 1816 Mr. Brodie married the daughter of Serjeant Sellon , and survived her two years .
By her he had issue two sons and a daughter .
Of these , the eldest , the present possessor of the Baronetcy , like his father , received early in life one of the Medals of the Royal Society , and is now the distinguished Professor of Chemistry in the University of Oxford .
FRANCESCO CARLINI was born in Milan on the 7th of January 1783 .
His father , Carlo Giuseppe Carlini , a native of Cremona , was one of the librarians of the Brera , and was eminent as a Bibliographer .
He died in 1789 .
His ancestors came , it is said , from Linz in Austria .
At an early age Francesco Carlini manifested a taste for astronomy , and was in the habit of making calculations for Oriani , Ilggio , and Cesaris , the astronomers of the Brera .
In 1 799 he was admitted to the Observatory as a pupil , was appointed one of the commissioners of weights and weasures for the kingdom of Italy soon afterwards , and in 1804 was promoted to the rank of supernumerary astronomer .
In 1803 he made observations of Pallas in opposition , and continued his observations of this and the other small planets up to 1816 .
Between 1814 and 1818 he constructed tables of the equation of the centre , and the reduction to the ecliptic , of all the small planets then discovered .
In 1804 he undertook the sole charge of calculating the Effemeridi Astronomiche , pronounced by Lindenau and Bohnenberger~ in 1816 , to be the best ephemeris in existence at that time .
From 1802 to 1807 he took a share in the geodesic operations required for the construction of a map of Lombardy .
These were carried on from 1788 to 1807 by the astronomers of the Brera , and afterwards by the French engineers .
A careful examination of the solar tables of Delambre , made in order to ascertain their fitness for use in calculating the Effemeridi , having revealed some serious errors , Carlini was induced to undertake a revision of them .
Retainilg the constants which Delambre had deduced from the observations of Bradley and Maskelyne , he recalculated the tables by a method of his own .
In 1832 he published a new edition of the tables , based upon newer and more accurate elements .
These tables were used till very recently for .
the calculation of the sun 's place in the most celebrated Ephemerides .
Laplace , dissatisfied with the semiempirical basis on which the lunar theory rested , even after the publication of the ' Mecanique Celeste , ' suggested to the Institute , as the subject of the prize for 1820 , the formation of lunar tables , by theory alone , as exact as those which up to that time had been constructed by theory and observation combined .
As far back as in 1813 Plana and Carlini had resolved to construct a complete theory of the moon , subjecting all the inequalities to the laws of geometry , and had made considerable progress in their task , when the announcement of the programme of the Institute induced them to compete for the prize by sending in the results they had already obtained .
By the decision of a commission , consisting of Laplace , Burkhardt , and Poisson , the prize was divided between Plana and Carlini , and Damoiseau .
The principle on which their joint memoir rested , and which rendered it superior to all researches of earlier and many of later date , was this : -never to take from observation any constants that were not indispensably necessary for the solution of the problem .
They adhered most rigorously to this condition , without which the analytical solution cannot be perfect .
In the development of the various expressions in series , they retained the literal notation , giving an algebraical , not a numerical solution .
This memoir was not published at the time : afterwards Plana resumed it alone , developed it more completely , and published it in 1832 , under the title " c Thorie du Mouvement -de la Lune , " in three volumes quarto , a work which forms an epoch in the history of astronomy .
In 1820 they published a joint memoir in reply to some objections to their theory raised by Laplace-and another on the lunar equation , having for its argument twice the difference between the longitude of the node and that of the perigee .
Carlini next undertook the construction of lunar tables .
These have been used up to the present time in computing the places of the moon for the Effemeridi di Milano .
He afterwards investigated various points of the lunar theory , especially the remarkable inequality of the moon 's mean motion , indicated by a comparison of ancient and modern observations , and produced , as Hansen proved in 1847 , by the disturbing action of Venus .
Of his " Algoritmo del calcolo dell perturbazioni lunari , " intended as the commencement of a complete lunar theory , only the first chapter appeared in the 5th volume of the memoirs of the Istituto Lombardo .
Carlini 's principal contributions to practical astronomy are:"Tables of astronomical refraction " ( 1807 ) ; " Computation of occuitation of stars by the moon " ( 1808 ) ; " Tables for the reduction of circummeridian altitudes , " ' ( 1809 ) ; " Tables for calculating the coefficient of the square of the time in the precession of stars " ( 1819 ) .
He invented a method of finding the time and latitude by means of a telescope provided with a level and a micrometer , and applied it in Spain , where he went by order of the Government to observe the eclipse of the sun on the 18th of July , 1860 .
Between 1821 and 1827 Carlini assisted in the measurement of the Italian portion of an arc of longitude extending from Bordeaux to the Adriatic .
He made the requisite astronomical observations on the summit of Mont Colombier ; determined the length of the seconds ' pendulum on Mont Cenis ; observed from Parma the gunpowder signals fired on Monte Cimone , and from Milan those fired on the summit of Monte Baldo .
He also determined anew , with the aid of better instruments and improved methods of calculation , the latitudes of Mondovi and Andrate , the extremities of the arc measured by Beccaria .
He found the sum of the deviations of the plumb-line to be about 48 " , and thus confirmed the accuracy of Beccaria 's observations .
On the death of Angelo de Cesaris in 1832 , Carlini was appointed Director of the Observatory of the Brera .
He was a good analyst , understood five modern languages , was the author of various scientific biographies , and was one of the editors of the ' Biblioteca Italiana ' from 1826 to 1840 .
The list of his writings appended to the notice of his life read before the Istituto Lombardo contains one hundred and forty-four titles .
Most of these , exclusive of separate works , are to be found in the appendices to the Effemeridi astronomiche di Milano ' from 1805 to 1863 , the 'Memorie dell ' Istituto Lombardo-Veneto , ' the Memory , Atti , and Giornale dell ' Istituto Lombardo , the 'Biblioteca Italiana , ' the 'Memorie della Societa Italiana , ' the 'WMonatliche Correspondenz ' and 'Correspondance Astronomique ' of von Zach , and the 'Zeitschrift fiir Astronomie ' of von Lindenau and Bohnenberger .
Carlini presided for many years over the Istituto LombardoVeneto , afterwards the Istituto Lombardo , and was a member of the principal Italian Academies .
Ie was foreign member of the Institute , of the Astronomical Society , and of the Academies of Vienna , Gottingen , and Berlin .
The date of his election as foreign member of the Royal Society is 1832 .
In 1832 Carlini married Gabriella Sabatelli , the daughter of an eminent artist .
She survives him .
He was amiable in private life , and of spotless character .
lIe remained free from infirmity , either bodily or mental , up to the age of nearly eighty years , and was able to compute the elements of the second comet of 1862 only a month before his death , which occurred , after a short but painful illness , at Crodo in Ossola , on the 29th of August 1862 .
The foregoing particulars of his life and labours are extracted from a biographical notice read before the R. Istituto Lombardo , on the 8th December 1862 , by his successor as Director of the Observatory of the Brera , G. V. Schiaparelli .
JAMES ORMISTON M'WILLIAM , M.D. , was a native of Dalkeith in Scotland , and was educated in Edinburgh , where he obtained his medical degree from the University , and the diploma of Licentiate from the Royal College of Surgeons .
In 1829 he entered the Navy , and , after serving for a time on a foreign station , attained the rank of Surgeon , and was appointed to I.M.S. 'Scout , ' stationed on the west coast of Africa .
On that unhealthy station , so trying to young naval surgeons , he devoted himself most earnestly to his duties , and obtained the distinction of the Gold Medal instituted by the late Sir Gilbert Blanc for special merit in the medical service of the navy .
On returning to England , after the ship 's term of service had expired , Dr. M'William took advantage of his temporary liberation from duty to improve himself in professional and scientific knowledge , and more especially to make himself well acquainted with the principles and practical methods of ventilation , heating , and other arrangements for the preservation of health .
This species of knowledge , together with the information he had acquired on the coast of Africa , peculiarly qualified him to superintend the fitting up of the three ships which were destined to proceed on a voyage up the Niger .
His sound judgment , intrepid character , and medical experience of a tropical African climate , had already led to his being appointed chief medical officer of the Expedition .
This Expedition was undertaken by benevolent individuals , supported by a considerable Government grant , to plant an English colony in Central Africa , and to promote agriculture and honest trade among the natives , in the hope thereby to reclaim them from trafficking in slaves .
The chief incidents of the ill-fated voyage are well known .
In the summer of 1841 the three ships proceeded to the African coast , under the command of Captain Trotter , and , ascending one of the mouths of the Niger , reached the confluence of that river with the Chadda , 270 miles from the sea ; but in the mean time malignant fever had broken out in the ships , and in a short time had prostrated both officers and crews to such an extent that first one of the vessels , and soon afterwards another , had to be sent back freighted with the sick of the expedition .
The remaining ship , the 'Albert , ' of which Dr. Ma'William was surgeon , continued her voyage fifty or sixty miles higher up the river , in the hope of reaching some less unhealthy region ; but the sickness did not abate , some of the ship 's company had died , and many more , including the commander and most of the officers , were lying helpless under the malady ; so that Captain Trotter , confirmed as he was in his judgment by Dr. M'William , determined to abandon the enterprise , and the 'Albert ' followed her consorts back to the sea .
By this time only two officers , Dr. M'William and Dr. Stanger , and one of the European seamen were left able for service .
In this plight the return voyage was commenced , and , the one remaining sailor having also fallen ill , the navigation of the ship was left to the two medical officers , Stanger acting as engineer and M'William as steersman ; and by their good management and gallant perseverance she reached the sea in safety .
After his return home , in 1842 , Dr. M'William published the 'Medical History of the Niger Expedition , ' which was well received ; and some time afterwards he was sent on a special mission to the Cape de Verde Islands , to inquire into the origin of the yellow fever which had broken out at Boa Vista soon after the arrival of the 'Eclair .
' After a most laborious investigation , Dr. M'William gave in to the authorities an able Report , in which he clearly established that the disease was communicable by infection , and had been imported by the 'Eclair .
' This report was printed by order of Parliament .
In rather tardy recognition of his public services , Dr. M'William was in 1846 appointed Medical Officer to the Custom House , and in 1858 was made a Companion of the Civil Order of the Bath .
He was elected a Fellow of the Royal Society in 1848 , and a Fellow of the Royal College of Physicians in 1861 .
I-e was a most active member and promoter of the Epidemiological Society , of which he was Secretary , and to which he contributed many valuable papers .
As a naval medical officer he was highly esteemed by his brethren , not only for his professional merit , but for his unceasing efforts to secure for them , and particularly for the junior members of the service , a rank and position more in accordance with the social standing of the medical profession in civil life .
Dr. M'William 's active and useful career was terminated on the 4th of May 1862 , in consequence of an injury of the brain , caused by a fall down a steep stair a few days before .
Reay-Admiral SIR JAMES CLARK Ross was born in 1800 , and died in April 1862 .
The incidents in the life of this great navigator and excellent man would doubtless fulrnish abundant matter for an interesting narrative ; but here we must be contented with little more than a bare indication of dates .
In 1812 James Ross entered as a midshipman on board the 'Briseis , ' commanded by his uncle , Captain ( afterwards Sir John ) Ross .
In 1818 he accompanied his uncle in his first polar voyage , and between 1819 and 1827 he returned four times to the same seas under Parry .
Again he accompanied his uncle in his Arctic voyages performed between 1829 and 1833 .
He conducted the scientific observations in these last-named expeditions ; and it was while thus employed that he determined the situation of the North Magnetic Pole , in latitude 70 ? ?
5 ' 17 " and west longitude 96 ? ?
45 ' 48 " .
In 1834 he was raised to the rank of Captain , and in 1835 was sent out to Baffin 's Bay to succour icebound whalers .
Captain James Ross 's skill and experience as a magnetic observer led to his being employed , between 1836 and 1838 , in a series of determinations of the magnetic declination and dip , and the intensity of the magnetic force over Great Britain and Ireland .
In 1839 he set out on his memorable Antarctic Expedition ; and after making three voyages within the Antarctic Circle , reaching 78 ? ?
10 ' of south latitude , greatly widening the known geography of the south polar regions , and gathering a rich harvest of observations in magnetism and other branches of terrestrial physics , he returned home after an absence of four years .
In 1848 he sailed on the last of his many arduous voyages .
It is well known that the direct purpose of this voyage the discovery and relief of Franklin and his fellow sufferers-was unhappily not accomplished , but its Commander did not fail to render it profitable to science .
Sir James Ross received his knighthood in 1844 .
King Louis Philippe nominated him to the Legion of Honour .
He was elected a Fellow of the Linnean Society in 1824 , and of the Royal Society in 1848 .
He was also a Corresponding Member of the French Academy of Sciences , and belonged to various other foreign societies of note .
To this brief notice of the leading events of Sir James Ross 's professional life , it will be incumbent on us to add a larger comment on his labours and achievements as a man of science ; but as these have not yet been fully made known in their proper place , it is deemed advisable that such reference to them as it will be requisite to make should be postponed for the present .
The great work which especially deserves to have its merits prominently set forth is his magnetic survey of the Antarctic regions .
This is justly held to be the greatest work of the kind ever performed , and it was undertaken at the special desire of the Royal Society and the British Association .
An account of the magnetic observations made by Sir James Ross in the first and second of the three Antarctic voyages was published in the 'Philosophical Transactions ' by his friend General Sabine ; and it is hoped that the labours of the third voyage and the coordination of the three years ' work will be laid before the Society in the next session .
The completeness with which the great and hazardous enterprise was carried out renders a full exposition of what was accomplished all the more requisite for a just appreciation of the merits of its gallant and skilful conductor ; and the propriety of waiting until this has been given will , it is conceived , be generally recognized .
EDWARD STANLEY , Esq. , Surgeon Extraordinary to the Queen , and Surgeon to St. Bartholomew 's Hospital , died suddenly , in one of the wards of that Institution , on the 24th of May 1862 , at the age of seventy .
Mr. Stanley , after receiving his general education at Merchant Taylors ' School , was , in 1808 , apprenticed to Mr. Ramsden , at that time one of the Surgeons of St. Bartholomew 's Hospital , on whose death he was transferred to Mr. Abernethy .
To this great master the pupil soon recommended himself by his earnestness in study , and especially by his devotion to anatomy and pathology ; and through their joint labours was created the Hospital Museum of Morbid Anatomy , to which Mr. Stanley especially contributed many preparations illustrative of diseases of the bones and joints .
This important collection they afterwards liberally presented , as a gift , to the Hospital .
Mr. Stanley 's acquirements in anatomy , and his well-directed zeal in its pursuit , led to his appointment as Demonstrator , and , after holding that office for some years , he joined Mr. Abernethy in 1826 in lecturing on anatomy and physiology , and continued to discharge this duty after the death of his eminent colleague , until 1843 .
In the mean time he had been , in 1816 , elected Assistant Surgeon , and twenty-two years later , Surgeon to the Hospital ; and he continued in that office until 1861 , when , although in good health and full possession of his faculties , he considerately retired to make way for his juniors , and accepted the title of I-onorary Consulting Surgeon offered him as an acknowlegment of his past services and a mark of respect for his honourable motives in resigning his duties .
In 1858 he was appointed Surgeon Extraordinary to the Queen .
Mr. Stanley entered the Royal College of Surgeons in 1816 ; he became an active and industrious member of the Council and Court of Examiners , served the office of Hunterian Lecturer , and was twice elected President .
IIe was of old standing among the Fellows of the Royal Medical and Chirurgical Society , and successively filled the offices of Secretary , Treasurer , and President .
I-is election into the Royal Society was in 1840 .
Mr. Stanley 's principal work is his ' Treatise on Diseases of the Bones , ' which appeared in 1849 .
While Demonstrator of Anatomy lie published a 'Manual of Practical Anatomy , ' which in its time was extensively used in the Anatomical Schools of this country ; and in 1829 an 'Account of the Mode of performing the Lateral Operation of Lithotomy .
' He also contributed twelve papers to the ' Medico-Chirurgical Transactions .
' MR. JAMES WALKER was born in 1781 , at Falkirk , where he passed his childhood and received the rudiments of his education .
He was afterwards sent to Glasgow , where he studied at the University and obtained distinction in Natural Philosophy and Mathematics .
From that University he , in later years , received the honorary degree of Doctor of Laws .
In the year 1800 he came to London , and commenced the profession of Civil Engineer , under his uncle , Mr. Ralph Walker , at that time engaged in the construction of the West India Docks .
He continued assistant to his uncle during the progress of that undertaking and during the completion of the East India Docks .
In 1803 he was appointed Engineer of the Commercial and East India Roads , undertaken in order to open a more direct communication with the Docks and the eastern parts of London .
These works were successfully carried out r1nder his direction , and now form the great route to the extensive suburbs which have risen between London and Blackwall .
The successful completion of the East and West India Docks , and of the communications leading to these important d6pots , obtained for Mr. Walker the appointment of Engineer for the Commercial Docks , which , with all improvements and enlargements up to the present time , have been executed from the designs and under the direction of himself and his partner , Mr. Burges .
The satisfactory manner in which these works were accomplished led to other appointments under the public Boards , who , from that time to the day of his death , consulted Mr. Walker on every engineering work of importance .
His numerous and important labours as a Civil Engineer , for the last forty years , are well known .
Among the great works with which he was connected , we may indicate , as especially worthy of note , Vauxhall Bridge , the Victoria Bridge over the Clyde at Glasgow , the improvements of the river Clyde ( which from the death of Mr. Telford up to a recent date were under Mr. Walker 's direction ) , the great repairs of the Caledonian and Crinan Canals , the drainage of the Middle Level by a cut of thirty miles in length , the coffer-dams and river-wall of the new Houses of Parliament , the Netherton Tunnel and other important works carried out by the Birmingham Canal Navigation Company , the Pier and Harbour of Granton , the improvements of the Harbour at Belfast , and the Harbour works at Dover .
All these and many others , such as the designs and execution of the Harbours of Refuge at Alderney , Dover , and Harwich , the Tyne Piers , and the completion of the Plymouth Breakwater , were under the direction and superintendence of Mr. Walker .
To them may be added , what is perhaps the most lasting monument of his skill , the various Lighthouses of the Corporation of the Trinity House .
The Bishop Rock Lighthouse , on the Scilly Islands , the erection of which was attended with peculiar difficulties successfully overcome by Mr. Walker , will rank with the foremost of the great structures of that class reared by Smeaton and by Stevenson .
Mr. Walker 's sound judgment and high character as an Engineer caused him to be frequently consulted by the Corporation of the City of London on the vi ious engineering works under their jurisdiction ; among which may be named the City Sewers , the Navigation of the Thames , and the Thames Embankment .
The last-mentioned work was laid out by Mr. Walker , and his design has now been adopted under the designation of " Walker 's line .
" Thus , for more than half a century , did Mr. Walker indefatigably exercise his professional skill in works of public utility in all parts of the kingdom-works which have had no mean influence on the social and commercial progress of the country .
Mr. Walker was elected into the Royal Society in 1828 ; he cooperated with Mr. Telford in establishing the Institution of Civil Engineers , and succeeded him as President ; and on the institution of the University of London , he was nominated in the Charter among the original members of the Senate .
In private life he was much respected ; he died on the 8th of October 1862 .
|
112349 | 3701662 | On the Physical Constitution of the Sun and Stars | 1 | 57 | 1,868 | 17 | Proceedings of the Royal Society of London | G. Johnstone Stoney | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1868.0001 | null | proceedings | 1,860 | 1,850 | 1,800 | 56 | 997 | 31,364 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112349 | 10.1098/rspl.1868.0001 | http://www.jstor.org/stable/112349 | 112,463 | null | Astronomy | 18.087002 | Atomic Physics | 17.370836 | Astronomy | [
14.641529083251953,
-33.03754806518555
] | " On the Physical Constitution of the Sun and Stars"* .
By G. JOENSTONE STONY , M.A. , F.R.S. , F.R.A.S. , Secretary to the Queen 's University in Ireland .
Received May 15 , 1867 .
PART I. Of the Sun .
Sect. page Sect. page 6 .
Of the Distribution and Periodicity I. Iiitroductory ... ... ... ... I of the Spots ... ... . .
, .
, .
, .
42 2 .
Collateral Inquiries ... ... ... ... ... 11 3 .
Of the OuterAtmosphere of the Sun 17 PART II .
Of other Stars .
4 .
Of the Photosphere and the Subjacent Parts ... ... .
34 1 .
Of Solitary Stars ... ... ... ... ... ... .47 5 .
Of Clouds in the Outer Atmosphere 39 2 .
Of Multiple Systems.51 PART I.-OF , THE1 SUN .
Section I.-Introductory .
1 .
THE true surface of the suin is the outer boundary of his enormous atmosphere ; but the principal escape of heat takes place from a concentric layer at a vast depth beneath the surface .
Withinl this luminious film there is a dark body , glimpses of which are occasionally seen as the unmbrie of spots .
2 .
The part of the atmosphere above the photosphere , which may be conveniently called the Outer Atmosphere , is emineintly transparent to most of the rays which emanate from the shell of clouds , or from beneath them .
But this is not the case in reference to others .
The atmosphere absorbs rays of those refrangibilities which correspond to the dark rays visible in the solar spectrum , and multitudes of others of a like kinid beyond the limits of the visible spectrum .
The depth of the atmosphere is so enormous that we must conclude it to be many times more than sufficient to act as an opake screen in reference to the great majority *t Read Jtune 20 , 1867 : see Abstract , vol. xvi .
p. 25 .
A part of the second section of the MS .
sent to the Royal Society has been pLLblished in the Phil. Mag. for Aug. 1868 ; and the suLbstance of an Appendix suggesting observations to be made on the occasion of the Solar Eclipse of Aug. 1868 , which also forms part of the MS .
, was published in the 'vMonthlly Notices ' of the Astronomical Society for Dec. 1867 , and reprinted in the Pllil .
Al:ag .
, vol. xxxiv .
1 ) .
502 ( 1867 ) , The rest of the paper is printedl here .
of such rays .
That there are darh lines in the solar spectrum reveals to us the fact that the suirface of the atmosphere is cooler than the luminous region beneath .
But we may go further than this .
Most gases are colourless ; in other words , they do not scatter rays incident on them .
Neither do they reflect light from their surface .
It follows , then , from the laws which regulate the exchange of heat , that where such a gas is of sufficient thickness to be opake in reference to any particular ray , it will send forth the most intense ray of that particular refrangibility which it is possible for a body of the temperature of the gas to emit .
Hence that there are lines in the solar spectrum of very different intensities is an evidence to us that the surfaces of the atmospheres from which they have their source are at different tenperatures .
It thus appears , upon a rough view , that the upper layers of the atmospheres of sodium , magnesium , and hydrogen are cooler than those of iron and calcium , and that these again are cooler than the upper layers of the atmospheres of nlickel , cobalt , copper , and zinlc .
In this , them , we have evidence both that the atmospheres of the several gases extend to different heights , and that the temperature increases from the surface of the solar atmosphere downwards .
Again , such facts as that some of the iron lines are less dark than others in their neighbourhood , that some of the copper lines are not noticeable , prove that even before deseending suficiently far to have passed through a stratum of these gases thick enough to be opake to these rays , we have already arrived at a sensibly higher temperature .
This temperature , in the case of some of the lines of cobalt , copper , and zinc , appears to approacb , if it does not pass beyond , the temperature of the luminous clouds .
3 .
Let us now direct our attention to the darker nucleus which lies within the photosphere .
It is known that a body , when surrounded on all sides by an opaque enlvelope of others at its own temperature , will reflect some of the incident light , if its surface be in any degree polished , and if the body be not wholly transparent or wholly black .
It will scatter others of the incident rays if .
either its surface or its substance be suLch as would not be wholly invisible if exposed to light brighter than that corresponding to its temperature .
And , lastly , it will emit rays in virtue of its own temperature of such kinds and in such quantities that , aloaig with those transmitted , reflected , and scattered , they will make up a total which is definite for each temperature .
This is one of the established laws of the exchange of heat .
It follows from this that a body thick enough to be opaque which emits much more feebly than others at a given temperature must reflect incident rays better , or scatter them-a more copiously .
It caiiot in an eminent degree do both .
Unless the dark body of the sun is cooler than the photosphere it is therefore , at least in those places which are exposed to us as spots , either such that it scatters incident light abundanitly , or it has a highly reflecting surface .
4 Before pursuinrg further our inquiry into the iature , of the central body of the sun , it will be convenient to enter upon the discuission of the phenomena of the luminous clouds ; and it wlli avoid confusion in this part of our investigation to adopt provisionially the definite hypothesis that the central body of the sun is all opake ocean with a highly reflecting surfacesuch a surface as an uiitarnished white molteni alloy would present .
We shall run no risk of error in doing this if we afterwards carefully reexamine such parts of our inquiry inlto the pllenoimena of the clouds as would be affected by substituting for this hypothesis any other that is admissible .
5 .
[ We shall also assume that the photosphere is not itself the origin of the heat which it disperses abroad , but draaws it from the adjoining regions .
No doubt if chemical action coul(d be the source of ' solar heat , the photosPhere might be its seat , and resemble the luminous part of a candleflame .
In this case the opaque regionis withini might be cooler than the photosphere , provided the photosphere were so translucent as to allow a sufficient radiationi throughi it from the parts within to the open sky .
But the photosphere to be thus translucent shiould of necessity be at a far higher temiperature than an equally bright body with a perfectly radiating surface .
And almost to this intense heat it would raise a great extent of the outer atmosplhere , which , being eminiently transparent , is but imperfectly fitted to moderate the heat it receives from contact with the photosphere .
Helnce we slhould expect to see conspicuous bright lines in the solar spectrum , which , however , we do not find .
Moreover , the amount of the sun 's radiation appears to be decisive against our attributing it to chnemical action.-September 1868 .
] 6 .
Let us consider what would happen if the pbotosphere were away , and nothing but an atmosphere of fixed gases in contact with an intensely heated molten splhere .
To simplify our conceptions , let us coniceive the molten mass to have a core which is maintained at a constant temperature , to have a surface reflecting perf'ectly , and to be enveloped by an extensive atmosphere of one fixed gas , wlvich , for fnrther simplicity , we shall suppose gives a spectruim of irnvariable lines .
The atmosphere is supposed to le extensive enough to render the change of temperature throughout it so gradual that there are nlo currents of convection .
The under surface of this atmosplhere would be raised by direct conitact to the same temperature as the polished surface of the dark body within .
The temperature would very slowly decrease in passing outwards from the core , first through the molten ocean , and then throughll the atmosphere , until that upper layer of the atmosphere was reached which alone can emit heat into space .
Through the thickness of this outer stratum the temperature would rapidly fall , the whole escape of heat fro-m the system taking place excltusively from it , in the form of undulations of the ether of those particular wave-lengths which the gas constituting the atmosphere cani excite .
Such is a picture of what would ultimately become the permanent state of such a system as we have imagined .
7 .
Let us niow suppose the surface of the ocean to lose part of its refleeting-power , and to become such an imperfect mirror as is possible with the bodies we lknow to exist .
The surface of the ocean will at once begin 13 moderately to radiate heat , most of which will escape into space .
It will thus become a surface of minimum temperature , cooler than the depths of the ocean within , and also for a time than the adjoining parts of the atmosphere without-just as the surface of the grounid becomes a surface of minimum temperatuire while dew is falling .
This surface of minimum temperature will draw heat from the warmer bodies on both sides of it , and will thus tend to cool both the atmosphere above and the ocean beneath .
8 .
Let us next conceive a particle with a highly emitting surface , and of the same temperature as the surrouniding medium , situated in the atmosphere a short distance above the ocean .
Such a body , owing to its lavish radiation , would quiickly fall in temperature far below the bodies around it .
If , however , these latter can supply it with heat so fast as to prevent its reduced temperature sinking below the temperature of brilliant incandescence , it will continue a imagnificent spectacle amid the comparative darkness around .
Let us now suppose that we have in the neighbourhood of this particle a vapour such that it is gaseous at the ardent temperature of the surrounding medium , but that it is precipitated either as a smoke or mist by the coolness of the radiating particle ; it will , the instant it is so precipitated , begin itself to radiate copiouslv , and so will tend to maintain the reduced temperature which is the condition of its continuing to blaze forth .
The process is the in-verse of what takes place in setting a flame alight , and is strictly analogous to it * .
If the vapour be of great depth , the upper parts , whenl precipitated in luminous cloud , will protect the rest of the vapour from that free radiation towards the sky which is the necessary condition of the phenomenon .
If the blaze had been first communicated to a part below the outer layer , it would at first form a cloud in that situation- the radiation from the upper side of this cloud would be least obstructed the blaze would therefore tend to spread outwards , and would no doubt do so much more swiftly than the cloud could subside .
The blaze would therefore soon fly to the upper-l[ surface of the vapour , where alone it could establish itself permanilenitly .
Such , them , appear to be the luminous clouds .
9 .
Since the great escape of heat takes place from the photosphere , it must be cooler than the contiguous parts of the regions within or of the atmosphere withouit .
And the lowest temperature to which either of these could possibly fall is evideintly the reduced temIperature of the clouds , a mi* It seems not improbable that as there are substances which will take fire spontaneously and , when tley have done so , will maintain a temperature of ignlition-a far higher temperature than they had before-so perhaps there may be vapours in the solar atmosplhere capable of spontaneously forming a molecule of liquid or of solid at their own high temperature , which would have but a momentary existence were it not that its instantly beginning to radiate both renders its new state fixed and sets the whole aieighbourhood ablaze .
t It will be shown further on , that a IrcGce of the vapour which forms the clouds may , and probably does , extend far beyonld them .
But the cloulds are at the boundary of the region in which there are !
Iruqe quantities of the vapouir .
nimum which would only be possible under the condition that the lumtninous stratum was anl absolute screen stopping every ray of heat coming from beyond it , and also reducing the entire of the intermingled atmosphere of fixed gases quite to its own low temperature .
The former of these conditions , especially , seems improbable when we bear in mind that the film in which cloud can form must be so transparent as to admit of the abundant radiation towards the sky which we have found to be essential .
We shall be able to treat this subject further on with more precision ; but , in the meantime , we are clearly entitled provisionally to regard the film of clouds as colder than the regions on either side of it .
10 .
Let us now consider more attentively the thermal conditions of the photosphere and of the subjacentregions .
In doing this it isnecessary to distinguish that part of the condensed vapour from which there is so abundant a radiation outwards as would enable vapour in that region to pass inito cloud , from such other parts of the conidensed vapours as are too much screened from the sky to allow any more cloud to form .
It will accordingly be convenient henceforth to restrict the word cloud to the former , and to use such words as mist or rain when we have occasion to speak of condensed vapour in a lower situation .
Now , in the first place , if from any cause a part of the vapour fitted to produce luminous clouds rose above the general level and became detached , it wouldform a cloud , which by its own weight , and by the coolness it would impart to the fixed gases interspersed through it , would gradually settle down till it became merged in the general luminous stratum .
This behaviour would be hastened by a suidden change of the density of the solar atmosphere , which , as we shall find hereafter , takes place at the boundary of the photosphere .
11 .
The clouds , thougn of a thickness small when compared with the enormous extent of the atmosphere of the sun , may nevertheless be of considerable depth ; but they can in no place be of such a density and thickness as to be opaque , since ino part of the stratum can come into existence from which there is not a sufficiently free radiation towards parts already cooled down or towards the open sky .
This , then , will put a limit to the density of the clouds .
If , from any cause , heat is supplied unequally to different parts of the stratum , the delnsity of the clouds must be correspondingly unequal , inasmuch as , in the more heated regions , even the lowest part of the stratum , which is the worst-situated , must be sufficiently exposed to the sky to enable it , under these adverse circumstances , to maintain the low temperature which is essential to the formation of cloud .
The clouds will accordingly be rarest where most heated .
As , then , the clouds are translucent in all parts , and in some parts more so than in others , it becomes of importance to study the intensity of the heat and light which reach us from beyond them .
12 .
The clouds must either brood like a fog over the surface of the subjacent ocean , or they are separated from it by an interval .
I will deal with the latter hypothesis first .
Assuming , then , that there is such an interval , we may suppose that the part of the atmosphere which occupies it is either nearly saturated with the vapour from which clouds are formed , or but sparingly supplied with it .
If it be very moist , the clouds as thsey descend , either through convection or by subsidence , will pass into th form of mnist , which will collect into a rain that will fall towards the oceal beneath .
If , on the other hand , the interval between the clouds and ocean be far from being charged with vapou , the cloud as it descends will dissolve away among the hot and dry gases below , while the ascending currents , as they rise into the situation from which they can freely radiate , restore the same quantity of a thin gauLze-like cloud .
The possible alternatives , then , are , 1st , that the interval between the clouds and ocean is transparent , or , 2nd , that it is rendered in a considerable degree opake by mist and rain , or , 3rd , that the clouds reach to the ocean .
13 .
Let us examine these hypotheses , beginning with that of a clear atmosphere under the clouds .
If there be such a transparent space , it is easy to see that the intensity of the rays which strike the under surface of the clouds is greater than that part of the solar radiation which emanates directly from the clouds ; for a portion of the rays which flow downwards directly from the clouds will be reflected by the body of the suni beneath ; another portioni will be scattered at the same surface .
These two portions will fall short of the ciitire quanitity of rays in the first instance radiated downwards from the donLds .
But as the body of the sun is hotter than the clouds , what is here wanting will , according to a known law regarding the exchange of heat , be more than made up by w hat the body of the su'n will itself emit* .
Thus we have already a quantity of heat radiated upwards against the clouds greater than that emritted by them downwards .
But fLrther , the clouds must scatter a part of the rays that strike their under surface .
Some of the rays so scattered will be afterwards reflected or scattered by the body of the sun , and will augment still further the heat striking the under surface of the clouds over that which they radiated downwards .
This excess will be great if the clouds be of a material that scatters light copiously ; for in this case we shall not only have a laroe supply of rays that had beeni so scattered added to the stock , but also , if the clouds scatter incidentrays abundanttly , they will , in obedience to the laws of the exchanige of heat , be at the same time such as will emit more feebly ; and accordingly the brightness which shines upon them from the background will be relatively more coiispin cions .
But , however this may be , whether the excess be more or less , it at all events exists , if the space under the clouds be clear ; and the clouds are in the position of a luminous and partially transparent body , with a still brighter body beyond .
If the average condition of the nearer body , the screen of clouds , be such that it is in a considerable degree opaque , then will a small spot in it which is thinner and co isequently more transparent than the neighbouring parts appear brighter than they ; whereas , if the average conditioni of the nearer body allow rays to pass pretty freely through it , then will a thin spot appear but little brighter than the parts around , and the circumstances might even be such as to render it darker than them .
We find both these appearances on the sun 's disk .
In the middle of the sun 's disk we find it to be most luminous ; and here the clouds would intercept least of the greater brightness beyond .
In the marginal parts of the disk the spectator looks obliquely through the stratum of clouds , which is therefore more opaque to his view , so that , in approaching the edge of the disk , the less initense light emitted by the clouds would be progressively less and less fortified by the splendour within .
The brightness of the disk would be accordingly shaded off towards the edge .
At the same time thininer parts of the filrrm , if not too extensive , would be seen conspicuously as faculee near the edge of the disk , while towards the centre their brightness would be merged in the genieral illuminiation around .
14 .
But , further , as the shell of clouds is at a much lower temperature than the adjoining layer of the atmosphere beneath it , while it is subjected to but little less pressure , it is evident that there must be a violent motion of convection between the two , the chilled portions descending , while the hot vapours from below boil upwards .
Cloud will form in the rising vapours , but it will be less dense than that of the parts more effectually cooled .
The appearance will be very much like what we see when looking from above upon water in the act of boiling , , the smooth tops of the columns of ascending water being represented on the sun by the brighter patches due to the thinness of that cloud which cani mainitaini its existence in the hotter vapouirs , while the turmoil which is seem in the water between these columns corresponds to the darker interstitial spaces which give to the sun 's surface a minutely granulated appearance ( rice-grains , willow-leaves , &c. ) , and in which the cloud at times becomes so opaque that those flakes which by prolonged emission become the most dusky seem to show like black or , at least , very dark pores .
This honeycormbed structure of the stratum of clouds will umodify the erect of obliquity in .
rendering the marginal parts of the sun 's disk less bright than the centre .
It will cause the effect to be perceived further from the border than it otherwise would be .
15 .
So far , then , the hypothesis of a clear space between the clouds and the ocearL seem , s to square with the phenomena ; but upon a further scrutiay we are forced to resign it as untenable .
For , as has been explained , the light which has suoered but one reflection , or been but once scattered , by the body of the sun , falls short of that which emaanates directly from the clouds , and the greater brightness of the background is due to the additions made ( 1 ) by the rays emiitted by the oceaii in virtue of its higher temperature , and ( 2 ) by the light which has suffered more than one reflection or been more than once scattered at the surface of the ocean .
Now the umbrae of spots exhibit to us the bocly of the sull so dark when compared with the lumninous clouds , that the great brightness of the faculke cannot be due to the light emSitted by the ocean .
It must therefore be due to the seconid cause , which , as we know , can only produce any considerable effect if the clouds are of such a nature that they scatter light abundantly .
But , again , we kinow from the proximity in which the umbrae of spots have been seem to the edge of the disk , that the interval between the clouds and the ocean is trifling as compared with the superficial dimensions of many faculve .
1I-ence , if the illumination of the background be due to the second cause , to light reflected or scattered from the body of the suin , the parts under extensive thin portions of the clouds would be sensibly less illuminated , and would give rise to an appearance more like that of penumbrme than of faculue .
The hypothesis would therefore fail to account for large faculhe .
Its rejection is also demanded by the appearance of the spectrum .
For if the clouds had the property of scattering light in the degree which would account for the granulated aspect of the photosphere , they would in the same proportion emit light feebly ; and the whole light reaching us , whether from or through them , would fall very perceptibly short of the maximum corresponding to their temperature .
Alnd as , on the other hand , a gas is a perfect emitter of the rays of which its spectrum consists , there could not fail to be coIlspicuous bright lines from those gases which extend only to the hotter strata of the solar atmosphere .
Now it is certain that no such lines are conwpicuous .
16 .
The same objections lie with still more force against the hypothesis that the clouds are in contact with a polished oceani .
We may therefore summarily dismiss this hypothesis .
17 .
Let us then tuirn to the alternative of an interval with mist and rain .
The mist beneath the clouds , as it is found in a hotter region , would emit more light , though the mist were no iuore dense than the cloud .
But the mist is probably much more dense ; and it is nlatural to suppose that it is dense enough to be opake , in which case , if it be formed of a material which is a good radiator , it will emit light of almost the maximum intensity which can be emitted by a body of its temperature .
Indeed this effect would be produced if the mist and r'ain were in a quantity much less than that which would be opake , in consequence of the assistance renldered by the body of the sun beneath , and that without any hypothesis as to the state of the latter , except only that it is opake and at as high a temlperature as the mist .
Now as it is likely that the average quantity of mist and rain is much more than this , its density may undergo very considerable fluctuations without its ceasing to pour forth its full torrenit of light and heat .
Such , then , appears to be the brighter background which shines through the clouds .
As in the last case , the currents of convection which prevail generally over the suin produce the gradation of light fading towarcls the edge of the disk , and the finely granulated structure of his surface , with its little bright patches , its dusky intervals , and its dark pores .
Where circumstanrces render the cloud thinner over any considerable extent while the raini continues , we hae a facula which is visible ( if it be not lost in the equal brightness of all around ) when it is near the centre of the diskc .
Where such thin parts occur in numerous small patches , they produce that ordinary mottled appearance of the sun 's surface which is visible in telescopes of moderate power .
If the rain stop , we have penumbra .
If the cloud also vanish , we have the umbra of a spot .
18 .
We have thus arrived at an hypothesis which in a veiry satisfactory manner agrees with several of the phenomena .
Before , however , we trust ourselves to this or any other particular hypothesis , we must retrace our steps and go over the whole ground with care , retaining at each step all the alternatives which up to that point are possible , and reducing the number by eliminating from the list every hypothesis which we find to be inconsistent with any known fact .
19 .
Now , in the first place , the gradation of brightness from the margin to the centre of the sun 's disk has usually been attributed to the action of an absorbing atmosphere telling with most effect upon the edges of the disk .
3But of course factula canlnot be referred to any action of our earth ; and it is incredible , therefore , that they exist only near the edge of the disk .
Heince the cause of the gradation of light , whatever it is , must be such as will leave the facuhe of uiiumpaired lustre as they move from the centre to the edge of the disk , while it renders other parts more dusky .
We may therefore discard the hypothesis that an absorbing atmosphere is the cause , since it would not act in this way .
It is therefore due in some way to the nature of the photosphere itself .
The telescope informs us that the photosphere coinsists of two parts which may be distinguished:-a brighter part , seen in the centre of the disk , in the faculee , in smaller bright patches , and in its purest form in the brighter specks of those parts of the surface which are granulated ; and a dusky part , seen towards the margin of the disk and in the interstices between the bright specks of the granulation .
Now , inicandeseeiit bodies radiate equally in all directions , and therefore , if the light of the sun enmanated from a muere mathematical surface , the disk would not be brightest at the centre .
Hence the photosphere is a stratum , not a surface .
A gain , the brighter parts cannot be at the top of this stratum , since in that case the margin of the sun 's disk would be the brightest .
Hence the bright and dusky parts are either iintermingled , or the dusky parts form the outer layer ; and if they are intermiingled , the brighter parts must be the more transparent , to render this hypothesis consistent with the gradation of light we find on the disk .
Again , the observationis show the whole granulated surface of the sun to be in a state of incessant chainge , although not by any means so inmpetuous as the earlier observers supposed ; hence at least the outer layer of the photosphere is mobile .
It is accordingly either a gas , a liquid , or a cloud .
The nature of its spectruti forbids otur admitting it to be a layer of gas * of moderate depth ; and if the layer of gas were so profounid as to be opake , it would radiate the maximum amount of light belonging to its temperatire at great depths , and so obliterate the mottled appearance which exists .
Again , an opaque liquid would be luminouss only at its surface , which we have found to be inadmissible .
Nor is an ocean of transparent liquid sufficienit .
Little light gets through 20 nietres of sea-water , and probably a few hundred metres of the most trai sparenit liquid would be practically opaque .
This trifling depth therefore vould render the incaildeseniit ocean luminous to almost the full extenit which is possible for a body of its temperature .
Such an ocean , th-refore , if tranquil at the surface , would reduce the whole sun 's disk to an uninterrupted gradation f of brightness .
If , .
to account for the granulationi , we suippose the oceani to be every here and there fretted with storms , the foam , being endowed with the property of scattering light abundantly , would no douibt be a bad emitter , and would therefore form dusky spots ; but these spots would be most conspicuous at the centre of the disk .
We must therefore reject the hypothesis of a transparenit ocean .
The hypothesis of a cloud , then , is the only one which remains .
20 .
Of clouds , there are two well-marked varieties-clouLds precipitated from a state of vapour , like the clouds in our atmosphere , and clouds of fixed solids or fixed liquids , such as smoke , a cloud of dust , the mad ill turbid water , oil in an emnulsion .
The sun attracts with so much more force than the earth that everything on his surface presses down with a force twenty-eight times as great a ; s that with which it would press downwards on the earth 's surface .
From this , and fro the amazing extent of his outer atmosphiere , it is 'natural to suppose that the pressure in its lower strata must be enormous .
This must occasion the lower strata to be very dense , unless the effect of the pressure be couLnteracted by the terrific heat .
OnX the other hand , the average density of the whole suni being only about one-fourth of that of the earth , the solids and liquids on his surt'aCe are probably much less dense than withi us .
If it should happen that the lower strata of the atmosphere were imAore denise than some e of the solid or liquid substances on the sun , these latter would rise ulntil they reached that part of the atmosphere which is of the same denisity as theimselves , and woulid float there ; and if in a state like dust , they would doibtless be maintained in violent agitation by currenits of convection , those on the outside being most cooled by radiation and siniking , to be replaced by others from the hot regions beneath .
The dust in the ascending currents would be the warmest , and therefore the brightest , and if the currents of convectionl were on a sufficiently extensive scale , we might expect as a result such a granulated appearance as the sun presents .
But it would be one which would be inlcomyipatible with the gradation of brightness which extends from the centre to the margin of the sun 's disk .
The stratum in which these convection-currents exist could affect the light coming from beyond merely as a partial screen , sinice there would be no marked* difference in point of transparency betweeni the ascending and the descending currents , so that the peculiar action which the honey-combed structure of the stratum would otherwise produce is not developed .
There would accordingly be scarcely any diminution of brightness till quite close to the edge of the disk ; and there it should fall off very rapidly .
As these are not at all the appearances which present themselves , we must give up the hypothesis of a clotud of fixed solid or liquid matter .
The hypothesis of clouds precipitated from vapour is therefore the only one not excluded ; and we have found that it appears consistent with all the phenomena that have been yet discussed .
Section II.-Collateral Inquiries .
21 .
The only class of bodies about the mnolecular constitution of which we have any satisfactory t information is gases .
These appear to consist [ The increase of tra'nsparency of the heat ; ed portions would be due to the separaion of the particles of dust caused by the expansion of the intermingled air .
Now at these high temperatures an addition to the temperature produces anl immense alteration in the quantity of heat and light radiated ( see ? ?
68 ) .
Hence the elevation of temperature cannot be great ; and accordingly the volume of the air , whichlvaries as the temperature measured from the absolute zero , is but little increased .
Such a change would determine great cuLrrents of convection , but would not materially separate interspersed particles of dust.-September 1868 .
] 1 The dynamical theory of the molecular constitution of gases , which , if I mistake not , may be ranked in point both of importance and probability along with the wave theory of light , does not appear to have yet miet with that general attention and acceptance which it seems to deserve .
It may , not be out of place , therefore , to add to the nliTnberless proofs which have been drawn from its interpreting the phenomnena of gases , by many writers , butt especially by Clauisius , the following negative proof , which demonstrates that no statical theory , whether on the hypothesis of a continuous substance or of distinct particles , is possible .
A gas is sLLsceptible of enormous dilatation and compression without any abrupt change in the laws upon which its pressure depends ; hence , if it consist of particles at rest , the force which acts in any directioni on any one , must be the result of forces emanating from many others , no one contributing more than a share which may be regarded as infinitesimal .
Hence it is easy to see that if the density be changed , the pressure will vary as the square of the density ; for the force in any direction on any one particle will increase as the ntumber of the particles on that or the opposite side ( according as the elementary forces are attractive or repulsive ) near enough to act on it , i. e. will increase as the density ; and the number of particles subjected to this augmented force which are found within each element of volumiie will also have increased in the same proportion .
Hence the pressure per square mnillimetre across any surface within the gas will increase as thf square of the density : and as this is a law which does not exist in of molecules moving about actively and irregularly in all directions , the path of any one being for the most part rectilinear , or , in other words , most of its motion being executed at a sufficient distance from the neighbouring molecules to be beyonid the reach of sensible inifluence from them .
Every now and then , however , each molecule comes sufficiently near some other molecule to have its course bent , on which occasions it darts off in a new direction .
Moreover miiany facts in physics and chemistry lead irresistibly to the conclusion that the molecules are resolvable into simpler elements ; and the probability distinctly is that each in most gases is a highly complex system .
When a body so constituted is enclosed , the molecules by flinging themselves againist the walls of the containing vessel produce the pressure of the gas .
If the enclosure be at the same temperature as the gas , they do so without gain or loss of vis viva .
But Iif the wall be at a higher temperature , the activity of those molecules which strike it is increased , and vice versed .
The altered activity is shared with the rest of the gas by conduction and convection-or mtiore slowly by coniduction only , if the circumstances do not admit of convection ; and so the temnpe ratuLre of the whole becomes changed .
22 .
When we compare different gases , we find that their molecules differ both in mass and in the motions that prevail within * them .
That the internal motions differ is abundantly testified by the amazing variety in the grouping of the spectral linzes to which the various gases give rise t. Again , the number of molecules per cuLbic millimiietre is known to be the same in all perfect gases , when taken at the same temperature and pressure .
Hence the masses of the molecules are in most simple gases proportional to what chemists have called their atomic weights ; and in those instances in which this is not the case they stanid in the same simple relation to these atomic weights as the densities of the gases nearly do .
Thus the masses of the gaseous molecules of hydrogen , nitrogen , oxygen , chlorine ) seleniium , bromine , iodine , and tellurium bear to one another the ratios of the numbers 1 , 14 , 16 , 35 5 , 79 5 , 80 , 127 , 129-which are the atomic weights of these substances , and nearly in the ratios of their vapour-densities .
But to represent the mass of molecules of phosphorus on the same scale , we must double the number used as its atolic weight , and take 62 instead of gases , it follows that nio gas conisists of distinct particles at rest .
The same proof applies , by the priniciples of the differential calculus , to the hypothesis of a contiDuouis and homogeneous substance .
For this proof given more at large , sec Proceedings of the Royal Irish AcademBy , vol. vii .
( 1858 ) , p. 37 .
31 , since its atomic vapour-volume is half that of the foregoing gases .
Similarly in arsenic we must take 150 instead of 75 ; on the other hanid , in .
cadmium and mercutry we must halve the atomic weights , and take 56 and 100 inistead of 112 and 200 .
In the case of sulphur , each molecule of its vapour has a mass represented on the same scale by the atomic weight of sulphur , viz. 32 , if the vapour be observed at temperatures above 1000 ' Centigrade ; but at some lower temperature it seems to contract to one-third of its former volume , since at a500 Centigrade , and under , it is found to be thus shrunk .
The mass of each molecule has become three times what it had been before , and is therefore represented at low temperatures by 96 .
23 .
Let us now consider what it is that puts a limit to the atmosphere .
Let us first suppose that it consists of but one gas , and let us conceive a layer of this gas between two horizontal surfaces of indefinite extent , so close that the interval between them is small compared with the mean distance to which molecules dart between their collisions , but yet thick enough to have , at any momeent , several molecules within it .
Molecules are constantly flying in all directionis across this thin stratum .
Som-e of them come withini the sphere of one another 's attraction while within the layer , and therefore pass out of it with altered direction and speed .
Let us call these the molecules emnitted by the layer .
If the same density and pressure prevail above and below the layer , the molecules which strike down into it will , on account of gravity , arrive with somewhat more speed on the average than those which rise into it .
Hence those molecules which suffer collision within the stratum will not scatter equally in all directions , but will have a preponiderating downward motion , so that of the molecuiles emitted by the stratumll more will pass downwards than upward : .
This state of things is unstable , and will not arrive at an equilibrium until either the density or the temperature is greater on the underside of the layer .
If the density be greater , more molecules will fly into the stratum from beneath than from above ; and if the temperature be greater the molecules will strike up into it , both more frequently and with greater speed .
In the earth 's atmosphere it is by a combiniation of both these that the equilibrium is maintained : both the temperature and the density decrease from the surface of the earth upwards .
24 .
We have hitherto takeni into account only those molecules which , after a collision , have arrived at the stratum from the side on which the collision took place .
But beside these there will be a certain number of molecules which , having passed through the stratum from beneath , fall back into it without having met withi other molecules , either by reason of the nearly horizontal direction of their motion , or because of its low speed .
The number of molecules that will thus fall back into the stratum will be a very inconsiderable proportion of the whole number passing through the stratum , so long as the temperature and density are at all like what they are at the surface of the earth .
In the lower strata of the atmosphere , therefore , the law by which the temperature and density decrease will not be appreciably affected by molecules thus falling back .
But in those regions where the atmosphere is both very cold and very attenuated , where accordingly the distance between the molecules is great and the speed with which they move feeble , the number of cases in which ascending molecules become descending without having encountered others will begin to be sensible .
From this point upwards the density of the atmosphere will decrease by a much more rapid law , which will within.a short space bring the atmosphere to an end .
Not , however , before the denisity has sunk immeasurably below what can be reached in our laboratories .
If there be a unit-eighteen * of molecules in every cubic m1illimnetre of the air about us , there will remain about a unit-fifteen in every cubic nillimetre of the best vacuuims of our air-purnp.s .
The molecules are still closely packed , within about an eighth-metre of one another ; i. e. there are about 60 of them in a row as long as a wave of orange light .
This accounts for our atmosphere 's spreading to the height at which meteors betray its presenice , which is far beyond the height at which we cani detect it by any ordinaryT means .
25 .
If an atmosphere consist of a mixture of gases ( for example , of uncombined nitrogen and hydrogen ) , the bounldary of each gas will be at a different height .
Where the nitrogeni is no longer able to maintain itself , the molecules of hydrogen , with a velocity v/ 14 ( or nearly 4 ) times as great , can still spread far beyond it .
It is also to be observed that the nitrogen will reach a greater height in conisequence of the presence of the hydrogen than it could alone , since an ascending molecule of nitrogen has more chance of escaping the fate of falling back without having encouintered another molecule if there be molecules of hydrogen to be met with as well as molecules of nitrogen .
In this way a substance of which there is but little in the atmosplhere may aseend nearly to the full height to which it would rise if present in abundarnt quantity .
Thus the vapour of socihum , which , as we shall find , is present in the SUn 's atmosphere as a mere trace , seems nevertheless to reach nearly the full height assigned to it by the mass of its molecules , through the assistance afforded to it by the abundanit atmosphere of hydrogen , which extenids much further .
In the saime way the vapoIur of water is probably borne to the linits of the earth 's atmosphere , although but a miinzor constituen t ; and the trace of carbonic acid which terrestrial air also contains , is p-robably supported to a height niearly as great as it would reach if present in much greater quanltity .
Where , then , as in the sun 's atmosphere , the lightest constituent is abundant , all the other gases which enter into its composition , will raing , e to heiohts which stand in the order of the masses of their molecules , whether they be present in large or in small qu-antities .
And where , as in the earth 's atmosphere , there is but a trace of the lightest constituent , viz. the vapour of water , it will form an exceptioni to the rule , inasmuch as it will be unable to mainitain its footing more than a little beyond the limits of the lightest of the abundant constituents , which in the case of the earth 's atmosphere is nitrogen .
26 .
It becomes of importance , then , to arrange the constituents of the solar atmosphere in .
the order of the masses of the miolecules , as this will be the order in which the surfaces of their successive atmosplheres will succeed one aniother .
A provisional attemipt is made in the followinog table to arrange on this principle the better-known of the elementary substances , including all the bodies whose spectra have yet been compared with the spectrum of the sun , or with those of other celestial bodies .
The positioIn in the list of those substances whose names are printed in ordiniary type has been ascertained by direct observations on three vapour-densities , al-cl nday be depended on ; but all the rest , which are printed in italics , are placed on the provisional suppositioni that the miiasses of their molecules when in the state of vapour are proportional to their generally received atomic weights .
It is probable that in some of these inistances the mass is proportional to some simple mnultiple or submultiple of the atomic weight , and that the position in the list ought to be altered accordingly .
We shall find grounds for concluding that this is the case with Barium , and that it ought to be placed in the list probably betweenl zinc and seleniuim , perhaps between calcium and titanium , or between sulphur and chlorine .
TABLE II .
Table of Elementary Substances arranged in the order of their Vapour-densities where these are known , and in the order of the Atomic weights where the Vapour-densities are not known .
i Observe +ed Observed vapourdvapourPresumi-ed masses of Wliether Elements .
( lensity , th , the gaseouts moleprcsent in the that of air hydrof cules , that of biysun 's atmtobeing the 1 rogogen egen being the uniit .
being the uinit .
sphere or not .
Hydrogeni ... ..069 ... ... OG '32 11 which is 1H presenit .
Lithium ... ... ... ... ... ... ... ... ... ... ... ... ... .
7 , , i ot .
Glteinumn ... .
9O G Boron ... ... ... ... ... ... ... ... ... ... ... ... ... . .
109 , , B Carbon ... ... ... ... ... ... ... ... ... . .
12 , , C Nitrogen ... ... ... ... ... ... ... 713 14(04 14 , , N not .
Oxygen..11056 15-98 16 , , 0 not .
F'luorinie ... ... ... ... ... ... ... ... ... ... ... . .
19 , , F Sodinm ... ... ... ... ... ... ... ... ... ... ... .
23 , , Na present .
M1-1-agnesium ... ... ... ... ... ... ... ... ... ... ... 243 , , Mg pr esent .
Alumin-um ... ... ... ... ... ... ... ... ... ... ... . .
275 , , Al dotubtful .
Silicon ... ... ... ... ... ... ... ... .
28 , , Si doubtftl .
Suilplhur above 10000 C 223 3223 32 , , S Chlorine ... ... .
247 35-6G9 35 , , C Potassiu ... ... ... ... ... ... ... ... ... ... ... ... 39-1 , , K doubtful .
Calciumn ... 40 , , Ca preseiit .
Titanium ... ... ... ... ... ... ... ... ... ... ... ... 50 , Ti TAB3LE I. ( continued ) .
ObevdObserved vapour-ve vapourPresuimed masses of vpu-density the gaseous moleWite Elemeno'ts .
esst that of cuils , that of byh rsnti h that of air Is-'satio bei ng the h-ydlrogeni drogen bein-g tohe sun'soo aitmo uniit , being the uiiiit .
shr rnt unit .
Vconmdienn* ... ... ... ... ... ... .
51-2which isV Chromnium ... ... ... ... ... .52-5 , ,Cr present , Manzganese ... ... ... ... ... ... ... .
, , Mnpresent .
Iron ... ... ... I ... ... ... ... ... .
50 Fe present .
Cadmium ... ... ... .3.94 50-94 5G , ,id not .
Nickel. .
~~~~~~~~~~~~ ... .
59 , ,Ni presenat .
Co balt ... ... ... ... ... ... o9 C Co present .
Phosphorus.450 ... ... 05 03 62 , 2P COPper ... ... ... ... ... ... ... .
0635 , Cu prese n't .
Yttrium ... ... ... ... ... . .
06430 , , Ziinc ... ... ... ... ... ... ... ... .
65 , Zni present .
Seleniunm ... ... ... . .
0-8 80-40 79 5 , So Bromine ... ... ... ... 5-54 80-00 80 , ,Br Ru ... ... ..d ... ... ..n ... .
85.4 , ,Rbt not ... .tron ... ... ..ium ... ... 875 S , p8 doubtfLil .
Zirconium ... ... ... ... ... ... ... 895 , ,Zr ceriutm ... ... ... ... ... ... ... .
92 , ,Ce not .
Lanthanum ... ... ... ... . .
92 , ,La not .
Sulphur under 5990 C 6017 95062 90 , 3.8 _Did~ymium ... ... ... ... ... ... . .
90 , Di not .
Mvotrbdenusn ... ... ... ... . .
90 , Mo Niobiumn ... ... ... ... ... ... 97 , , Nb Mercury ... ... ... ... .6976 0 100 , , Iig not .
Rhodium ... ... ... ... ... ... . .
104-2 , Ro Rutheniumfz ... ... ... ... ... ... ... 104-2 , ,Ru not .
Palladium ... ... ... ... ... I ... . .
100.5 , Pd not- .
Silver ... ... ... ... ... ... ... . .
108 , Ag n-ot .
Tin ... ... ... ... ... ... I ... . .
118 " , , n n-ot .
Thorinum ... ... ... ... ... ... ... 119 , ,Tb Uranlium ... ... ... ... ... ... ... 120 , ,U Antimiony ... ... ... ... ... ... ... 122 , , b not .
Iodin-e ... ... ... ... 8-710 125-95 127 , ,I Telluriumn ... ... ... .8-913 128-80 129 , ,To Cesium ... ... n ... ... ... ... ... 133 , ,Cs Barium ... ... ... ... ... ... ... . .
137 , ,Ba present .
Tantalum ... ... ... ... ..1370 6 Ta Arsenic ... ... ... ... 100 1531 150 , ,2.As Tungqsten ... ... ... ... ... ... ... 184 , ,W Gold ... ... ... ... ... ... ... ... 1900 , Au .
not .
Iridium ... ... ... ... ... ... ... .
1972 , ,Ir not .
Platinum ... ... ... ... ... ... ... 1972 , ,Pt not .
OsmWium ... ... ... ... ... ... 199 , ,Os Th11allim ... .o ... ..n ... ... ... . .
204 , ,TI Leaid ... ... ... ... ... ... ... ... 207 , ,Pb not .
Bismnuth ... ... ... ... ... ... ... .
210 , , Bi a[The position of vanadium has been alteredl from that assigned to it in the MS .
of this memoir , in accordance with Rioscoo 's recenit investigations regardin'g this substance .
I-f the vapour-density of van-adlium-i be ever determined , it is presumable that .
its molecular mass will prove to be 2 V , i. e. 1-02 4 , in analogy to those of phosphorus and arsenic , in wh-ich case its positionin the Table will nieedl to be alteredl again.-September 1808.1 Section III.--Of the Outer Atmosphere of the Sun .
27 .
Such , them , is the order in which we should expect to find that those of the elements which exist in the sun 's atmosphere succeedl oil inother , the atmosphere of hydrogen far overlapping all the rest ; thieni , at a profound depth , sodium and magnesium , reaching nearly to the same height , since the masses of their molecules are near-ly equal ; next , at a great distance further down , calcium ; then , in a grou ) reaching niearly to the same height , ehromium , maniganese , iron , n-ickel , and cobalt ; then , within a moderate distance of these , copper and zinic ; and lastly , after a vast interval , barium .
These are all the elements as yet known to exist in the sun 's atmosphere .
Let us now compare with the observationis this anlticipation founded on the molecular constitution of the elements , bearilig in minid that the order is likely to be in some few cases incoirect , owing to our having occasionally erred in assigning the foregoing " masses to the vapour-molecules .
To make this comparison most effectually , Table II .
, opposite to p. 32 , of the intensities of the solar lines observed by Kirchhoff will be of use .
In this Table the lines of each known constituent of the solar atmosphere are placed in the order in which they occur in the parts of the spectrum mapped by Kirchhoff , which extend between wave-lengths 43 and 77 eighth-metres , that is from the indigo about G to the extreme crimson beyond A* .
Each spectral line is represented by a nuttmbere , 1 , 2 , 3 , 4 , 5 or 6 , which also indicates its strength in the solar spectrum , 6 meaning the darkest and 1 the faintest recorded by Kirchhoff .
28 .
The study of this Table is particularly instructive .
It will be convenient to begin by studying the iron lines , since they are numerous , extend over a great range of the spectrum , and above all because there appear to be no bright lines in the iron spectrum to which dark lines in the solar spectruim do not correspond .
This was invariably the case with those observed by Kirchhoff , who has mapped upwards of 70 of them TABLE ( coitiziued ) .
Wave-lengths Wave-lengths in in eighth-metres , Kirchhoff 's eighth-metres , Kirchhoff 's i. e. metres diarbitrary i. e. metres diarbitrary vided by 108 .
scale .
vided by 108 .
scale .
49 30 corresponds to 1998-0 55 corresponds to 1309-0 49 40 , , 1986-1 55-70 , , 1248-4 49-50 , , 1974 3 55-80 , , 1240 2 49-60 , , 1962-5 55-90 , , 1232-0 49-70 , , 1950-8 56 , 1223 8 50 , , 1913-0 ? ?
56-10 , , 1215.6 51 , , 1762 0 ? ?
56-20 , , 1207-4 5160 , , 1673-0 56-30 , , 1199 3 51-70 , , 1658-3 57 , , 1144-0 ? ?
51-80 , , 1644-3 58 , , 1070-0 ? ?
51-90 , , 1630-8 58-90 , , 1009-7 52 , , 1617-5 59 , , 1003 0 52-10 , , 1604-3 60 , , 948-0 ? ?
52-20 , , 1591-2 61 , , 897 2 52 30 , , 1578-3 61-10 , , 891-9 52-40 , , 1565-5 61-20 , , 886-6 52-50 , , 1552-8 61-30 , , 881-3 52-60 , , 1540-2 61-40 , , 876-1 52-70 , , 1527-9 61-50 , , 870-9 52-80 , , 1516-1 61-60 , , 865-7 52-90 , , 1504-8 61-70 , , 860-6 53 , , 1494-1 61-80 , , 855-5 53-10 , , 1483-8 61-90 , , 850-5 53-20 , , 1473-7 62 , , 845-5 53-30 , , 1464-0 63 , , 800.0 ? ?
53-40 , , 1454-4 64 , , 758-5 ? ?
53-50 , , 1445-6 65 , , 719 ? ?
53-60 , , 1436-1 66 , , 682-3 53-70 , , 1426-6 67 , , 648-3 ? ?
53-80 , , 1417-2 68 , , 615-9 ? ?
53-90 , , 1407-7 69 , 584-8 54 , , 1398-3 70 , , 555-8 ? ?
54-10 , , 1389-0 71 , 528-4 ? ?
5)4-20 , , 1379-7 72 , , 502-4 ? ?
54-30 , , 1370-5 73 , , 477-7 ? ?
54-40 , , 1361-2 74 , , 453-8 ? ?
54-50 , , 1352-1 75 , , 430-3 ? ?
54-60 , , 1343-3 76 , , 406-9 54-70 , , 1334-7 77 , , 383 ?
The following Table contains the original determninations expressed in metrical icasores on the supposition that a Paris inch=27-07 illiimetres .
The signl + is added where the omitted decimals lay between -0016 ' aznd 1005 , andwhere they lahy betweei -005 that ( given betweeni iron electrodes from a battery of S0 cells , which gives a far greater number* of iron linles , and with this apparatus he has beeii able to observe the enormous number of 460 coincidences .
TABLE ( conlinued). .
t_cB Remarks .
53 LB9 2.+ 19 o *74 o 1430 5e *10 1+ 138-4 c CZ 5369+ 25+ 1428-2 S Fe .
*71+ 2 1425-4 5b Fe .
'74+ 3 1423-0 Sb Fe .
'761+ 142115 6c Fe .
5408 ? ?
3313909 5 5d Fe .
5101 ?
7 138944 6c Fe .
*28+ 19137236 b Fe .
'345+ 1367-0 6d Fe .
'49-f 161352-7 Sb Fe .
'51 1+ 13S1'1 Sb Fe .
54-609 1343'5 6c0 Fe .
55'77117 1242-6 6c Fe .
'91 14 ? ?
1231-3 Sd Fe .
*99 8 1.2247 5d Ca. 56 0341221-6 S5 d Ca..07 4+ 1217-8 r ) d Fe ; Ca. '20 13 1207.3 5 , q Fe .
D2 5894+ 274+ 1006 8 6b Nal Initerval betweenD , and D , DI 59 00+ 6 1002-8 ( ) b Na j =G603Xth-met'es .
6105S204+ 8949 2e Ca. '2419 8849 4b Ca. Co. '3915 877-0 4c Fe .
'43+ 5874'3 4b Ba .
'63+ 20 863'39 iSb Ca. '71 8860 2 3d Ca. '9221849 73c Fe .
a 62 59 67+A strong linle canLsed by the earth 's C 6568 309 6941 C ) ; IL ; winged .
jatmosphere .
B 68'7S 307 S92-7 I6c Winged on en side .
A 76112 737 404-1 6 Winged .
In this list two of Angstr6ni 's rays have beeii omitted-those to which he assigns the wave-lengthfs 19034 and 19364 VIlIth-inhelies , which correspond to 51-53- , and 52-42 VIIIth-metres ; since there arc no conspicuous linies in the solar spect.ruim corresponding to them-i , andic since , in the ease of the latter at least , there is plainly soimle , mlliisprint .
If we might conjecture that they ought to haave beein entered as 1900(4 and 1932 4 eighthl-inchles , they wouldl corresponid to 51-44+ and 52 31 eighth-miietres , and belong to two strong iron rays .
29 .
The first thing that strikes the eye in the part of the table appropriated to the ironl lines is a continuous gradation of intensity from the indigo to the red .
The most refrangible iron lines mapped by Kirchhoff are those in the indigo , all of which he found of the deepest black , which he represents by the number 6 .
Then follow the lines in the blue , in which there appears to be a struggle between this intense blackness , and the darkest shade short of blackness recorded by Kirchhoff , and to which he assigns the number 5 .
In this part of the spectrum lines of the intensity 6 are still predominant .
In the next region , the bluish-green , this struggle is continued , but now with a predominance of lines of the intensity 5 .
About the middle of the green we for the first time meet with an unexceptionable linle of intensity 4 , corresponding to the wavelength 53-87 VIIIth ; metres .
The last line of intensity 6 presents itself at wave-length 55 77 , after which , in .
the yellow , orange , and red , the inteDsity of iron lines has for the most part sunk to 4 or 3 .
30 .
Now the iron lines seen in the solar spectrum originate in the upper part of the iron atmosphere , each ray coming from a stratum of such a thickness that it is opake for that particular ray .
This thickness differs from ray to ray , being greater for those rays which are caused by atomic motions of feeble intensity .
Such rays therefore will in part originate from a greater depth in the solar atmosphere , and therefore from a region of greater heat .
They will therefore be brighter , or in other words less conlittle informed on these subjects to speculate with any confidence on the cause , and perhaps the following conjecture is the best that can yet be made .
The effect may perhaps be due to the brief duration of the , sparks .
The enormous temperature caused by each spark lasts for a very short time , and is not renewed until after the lapse of an interval long in comparison .
The electricity , when it passes , probably produces its direct effect in accelerating and controlling the directions of the motions of translation of the molecules of the gas ; and only indirectly , through the resulting violence of the molecular collisions , excites those more subtle atomic motions which give out the light .
Those of the atomic motions therefore which are most influenced by each collision will be the first to reveal themselves , and the rest not until after very many collisions shall have taken place , so that before they have had time to culminate , the duration of the spark may be over : whereas when they have time fully to unfold themselves , as they can in a continuous current , they may attain in some cases a higher intenisity , and consequently emit a greater brightness .
In support of this explanation , we have the fact that the lines seem with Ruhmkorff 's coil have been observed to correspond to the most conspicuous lines in the solar spectrum .
Now those atomic motions which are most developed by a few collisions will usually be those of which the periodic time is most subject to perturbation ( see Phil. Mag. 1868 , vol. xxxvi .
p. 132 ) .
They will therefore in such cases give rise to dilacded lines in the solar spectrum , and if the circumstances be such as to cause much of the breadth of the line to appear quite black , as for example in many of the iron lines , it will in consequence of its breadth appear much more intense .
On the other hand it should be remiiembered as against our conjecture , that if the Ruhmkorff 's sparks last as lolng as the measures Wheatstone made of the durat ; ion of the spark of a Leyden Jar , viz. four Vth-seconds , the number of collisionis which take place during the continualnce of a spark must be so great as to take away much from the probability of the explanation .
spicuouis as dark rays .
These same rays , sinice they are duie to feeble atomic motionis , will , in the iron spectrumn produced by artificial meanls , appear the faintest .
Now in all regions of the iron spectrum artificially produced , rays present themselves of every possible degree of intensity ; whereas of those observed by Kirchhoff in the solar spectrum , the fluctuation of intensity in any orne region of the spectrum seldom exceeds onre degree of his numerical scale , and but once exceeds two degrees .
This is coniclusive evidence that iron is so very abundant in the solar atmosphere as to be opaque for the feeblest of these rays before a depth is reached which is very much hotter than the outer surface of the iron atmosphere .
It also shows that the gradationi of brightness in the iron lines from the more to the less refranigible parts of the spectrum is not due to the less refranigible lines coming from profound depths , and being on this accouint brighter .
But the cause is sufficiently obvious .
If a body of such a kind that it emits the maximum light corresponding to its temperature , be gradually heated , it will first begill to glow with scarlet , orange , yellow , and green rays ; and according as its temperature rises its spectrum will expand in both directions towards the extreme red , and still more towards the violet .
If , then , a body heated in a furnace be compared with one at a much higher temperature , the spectrum of the former will evervwhere be fainter than that of the latter , but not equally so .
It may have a considerable brightness in the red and orange rays , and show sensible light in the green , and at the same time appear in the comparison absolutely black at higher refra-igibilities .
And the same general appearanice* would doubtless be founid if the maximum spectrum of any one temperature were compared with the maximum spectrum of a higher temperaturet .
Now the upper layer of the iron atmosphere , from which comes all the light that reaches us in the iron lines of the sun 's spectrnm , is at a vastly lower temperature than the photosphere , but not so cool as to be of insensible brightness through the whole range of the spectrum .
It begins to glow sensibly in the green , even in comparisonl with the intenise light of the sun , and renders the iron lines of the green short of absolute blackiness .
And this effect goes on increasing until it reaches its climax in the oranlge and red .
31 .
As molecules of calcium vapour are of a mass less than that of irlon molecules , in the ratio of 40 to 56 , calcium vapour must reach a far cooler regioni of the solar atmosphere than iron .
Nevertheless none* of the calcium lines observed by Kirchhoff appear to be as intense as many of the iron lines .
This is no doubt due to calcium vapour being a much smaller constitueut of the sun 's atmosphere than iron , just as oxygen is less abundant in our atmosphere than nitrogen , and carbonic acid much less abundant than either .
Judging from the indigo and green calcium lines , which are all less intelnse than the iron lines in their neighbourhood , it would appear that some light reaches us from a hotter region than any light that reaches us from iron lines , and accordingly that calcium gas is so rare , and in consequence the stratum which can intercept and therefore is employed in emitting these rays is so thick that , though its upper surface soars far above the upper surface of the iron atmosphere , its under surface stretches further down than the under surface of the corresponding , and comparatively shallow , active stratum of iron gas .
This appears to be the case too with most of the rest of the calcium lines observed by Kirchhoff ; but the lines 50599 and 56-03 in the yellowish-greenl , and the lines 61 63 , 64-32 , and 64.55 in the red , all of which are of intensity 5 , are probably exceptions , and owe their strength to calcium gas being much more opake in reference to them , so that they are emitted by a stratum shallow enough to reach but little beyond the extreme verge of the iron atmosphere .
These are some of the lines that give the calcium light , when seen undispersed , its beautiful purple colour .
Calcium is no doubt very opake also in reference to the other lines of the same class , such as the lines Hll , H-2 and g , beyond the limit of Kirchhoff 's maps .
In taking a general review of the calcium spectrum , these lines should be left out of consideration as not being comparable with the rest ; and if this be done , the remaining lines will exhibit the same gradation of intensity from the red to the blue which we found in the iron lines .
32 .
But in the immense extent of atmosphere which spreads upward from the surface of the calcium , in the vast elevation to the boundary of the atmospheres of magnesiunm and sodium , and in the far greater heights to which hydrogen alone can soar , the temperature has fallen too low to produce light visible in comparison with solar light in any part of the spectrum .
And accordingly all the linles referable to magnesium , sodium , or hydrogen , in whatever part of the spectrum they may lie , are intensely black .
But before proceeding to examine these lines in detail , it will be convenient to inquire into the state of the regions further clown .
33 .
The sun 's atmosphere is heated beneath by contact with the scorchiuig body of the sun , and it would throughout its whole extent attaini this l The lines 4883 and 5274 of intensity 6 , the latter of which is the less refrangible of the lines constituting the close double line E , are left out of account ; as they are also iron lines , and no doubt owe their intensity to this circumstance .
The lino b6-07 of intensity 5 , which is also a line common to the two spectra , is probably a stronger line on this account than it would be either as a calcium or as an iron line .
enornmous temperature were it not for the escape of heat from it , which is perpetually going on .
The first and principal escape of heat takes place from the photosphere , but it is also going on in the form of spectral lines , whether visible or beyond the range of refrangibility that the eye can see , from the upper layer of each gas that is successively left behind in asceniding through the atmosphere .
The last escape of heat is from the hydrogen linies .
The stream of heat which passes per seconld through any spherical shell concentric with the suLn into those parts of the atmosphere that lie outside it , is equal to what escapes per second from the latter into space .
This stream therefore rema-ins constant wherever an interval exists between the outer boundary of one gas and the bottom of that uipper layer of the next which is thick enough to be opake for the faintest of its spectral lines ; but throughout the depth of each such upper stratum the stream of heat is on the decrease.34 .
We shall better uniderstand what takes place by considering the agency by which the heat is carried outwards through the solar atmosphere .
It is partly by conduction , but principally by what may be called internal radiation , to which are probably to be added in some situationis convectioni and irregular motions such as would result from storms .
By conduction I mean that conduction which is effected by the rectilinear motionis of the molecules .
It is the only conduction to which experimentalists have founid it necessary to attend , since the quantities of transparent gas upon which they ' operate are not such as to be , in the cool state in which they have examined them , perceptibly opake to any of the incident rays .
But whei the gas is incandescent and present in enormous quantity , the chief transference of heat through it will be in consequence of what I have called internal radiation , which comes into play whenever the spectral rays emitted by onie part of the gas are absorbed by the surrounding parts before they can reach the outer bounidary and escape .
If the gas be highly opake for any particular ray , which is in general the case of those rays that appear very bright in spectroscope experiments , it will travel but a short distance before it is effectually absorbed ; but the rays which are faint in spectroscope experiments will wanider further , and will contribute the most to the rapid carriage of the heat to great distanices .
It should also be borne in mind that if an extenisive gas have a uniform temperature throughout , the rays which at profound depths are dashing about , are all of the maximum brightness corresponding to that temperature ; but that if the temperature of the gas be shaded off in one direction , as it is in the solar atmosphere , the rays of internal radiation wh2ich are directed outwards at any particular spot are brighter than the maximum brightness corresponding to the temperature of that situation , since they come from warmer regiols ; and that those rays will be the brightest which in our experimenits would be faint , since they come from the most remote , and , therefore , from the hottest of the parts from which any of the rays arrive .
35 .
It will not now appear strange that the region immediately otutside the photosphere should attain an enormous temperature .
It is in conitact with the luminous clouds , and would on this accouint alone be brought to as high a temperature as theirs ; but , beside this , rays of every refrangibility are emitted from the hotter region beneath the clouds of anl intensity corresponding to the far muore consuming heat which there prevails .
And if out of this terrific heat all the rays be selected which correspond to all the spectral lines of every gas in the solar atmosphere , they will constitate a body of heat , a small part of which is no doubt spent upon the gauzelike luminous clouds , or absorbed by the intermingled atmosphere .
, but the bulk of which is poured into the atmosphere overhead .
On the other hand the only heat which escapes outwards from this upper atmosphere is the quantity , small in comparison , which is emitted by these same spectral rays at the reduced temperatures which correspond to the duisky lines visible in the solar spectrum , or to similar lines lying beyond the limits we can see *. .
All the rest of the heat received by the superincumbent atmosphere is returned by it downwards , and is the measure of the fervid temperature which its lowest stratum attains .
Thus the atmosphere above the luminous clouds will begin by waXing in temperatuire , and contillues to grow hotter through .
that interval to which the heat emnitted from beneath can in any abundance directly penetrate .
At the limit of this space there will be a surface of maximum temperature , after which the heat will very gradually fade off by reason of the conduction , convection , and internal radiation which feed the escape outwards from the upper layers of the successive atmospheres .
36 .
It is of importance to observe that if the boundary of any one of the gases that constitute the sun 's atmosphere fall within the stratum which is hotter than the luminous clouds , or very close above it , that gas can only exist in a state of such utter attenuation within the stratum that we can scarce expect to detect any lines in the spectrum corresponding to it .
The stratum in question rests upon the , luminious clouds benieath , and its upper limit is to be defined as that situation in which the temperature has again fallen to the same point at which it stands in the shell of clouds .
At all intermediate stations the temperature is higher , or , in other words , the motions of the molecules of the gases are more active. .
At the upper and under boundaries of the stratum they are equal ; but the pressure , and consequently the density , is somewhat less at the upper station , or , in other words , the molecules of the gases constituting the atmosphere are there a little more separated .
Now any gas which comes to an end withiin the stratum must be unable to maintain itself at the upper surface of the layer , while in the stratum of luminous clouds it is able to hold its ground with equal molecular motions , solely because the molecules are there somewhat niearer together .
It must therefore at the lower station be in a state of almost inconceivable rarefaction ; and , from the laws of diffusion , its density at any higher point can nowhere go beyond this .
It appears , therefore , almost in vain to expect to see bright lines in the solar spectrum .
If , however , any such exist* , they will probably be most readily detected in light taken from near the margin of the sun 's disk , where the brightness of the region behind the luminous clouds is cut off , and where the thickness of the stratum of attenuated gas which forms the bright lines is increased by the oblique position 6f the spectator .
37 .
This rarefaction ( which would be carried to an extreme in the case of a gas , if any such exist , which extends into , but not beyonid , the stratum that is hotter than the luminous clouds ) will also affect in a very considerable degree those gases which do not spread far beyond it .
Accordingly the fainter lines in the solar spectrum either arise from such lowlying gases in a state of great tenuity , in which case those lines only can be visible in reference to which these gases are most opake , which will therefore be the brightest of their artificial spectra ; or they arise from constituents of the solar atmosphere which spread into the colder regionis above , in which case they caln only be those lines in reference to which these gases are highly transparent-such as are lines 50A48 and 53d52 of the Calcium spectrum , and the lines 49-21 and 51 81 of the Nickel spectrum .
It may perhaps be found that faint lines of this latter class will be seen about equally distinctly in spectra formed of light taken from the centre of the sun 's disk , and in spectra formed of light taken from near its margin .
When the light is taken from the centre these lines have the advantage of a brighter background to set them off ; when it is taken from the margin they have in their favour the greater depth of Calcium or of Nickel atmosphere which is looked through .
But in the case of those faint lines of the other class which originate in the lower strata of the sun 's atmosphere , the effect of obliquity will be very much greater ; so that we may expect to find these rays most conspicuous in spectra of light from very near the edge of the disk .
This appears to accoun-t for observations* lately made by Angstrom .
38 .
Let us now consider the information given to us by the lines of the spectrum which are due to hydrogen , sodiurn , and magnesium .
In the first place the sodium lines are narrow and sharply defined .
In both respects they differ from the lines of hydrogen and magnesium , which are broad and winged , that is , shaded off on one or both sides into dusky bands less dark than themselves .
Now at and up to the temperature of the flame of a spirit-lamp sodium vapour can give rise to such lines ; but at the temperature of a Bunsen 's burnier the sodium lines have begun to expand and be ill defined .
HLence we learn that in those upper regions of the sun 's sodium atmosphere in which these lines originate , the temperatur e is lower than that of the flame of a Bunsen 's burner .
Nor need we be astonished that this or a much lower temperature can prevail so close to the fierce heat of the photosphere , when we take into account how effecttually the outer parts of the sun 's atmosphere are screened from the glare beneath by the stoppage in the intermiediate regions of almost every ray that could act upon them .
39 .
The absence of wings to the linies D indicatest to us that there is not in the sun 's atmosphere enough of sodium vapour of temperatures intermediate between the temperature of a Bunsen 's burner and the temperature of the photosphere to be in a sensible degree opake to the wings of the rays which it emits .
This both shows what a mere trace of sodium is diffused through the solar atmosphere , and also to what a vast height it rises as compared with the thickness of that part of the solar atmosphere which ranges in temperature between a temperature below that of a Bunsen 's flame , and a temperature comparable with the intense heat of the photosphere .
In fact , the atmosphere of sodium , owing to the small mass of its molecules , which is less than half the mass of inolecules of iron , must spread to a vast distance beyond the iron atmosphere ; and through this immense space the temperature appears to vary very slowly , and to be nowbere high .
40 .
The outward stream of heat which reaches the upper layer of the iron atmosphere for the most part escapes into space from that neighbourhood through the numberless lines of iron , calciumn , chronium , manganese , and through the darker of the lines of niickel and cobalt , all of which drain off heat from this region .
No heat passes beyond , except the small quantity necessary to keep up the feeble escape from the lines of hydrogen , sodium , and magnesium , and others of the same class , such as B , A , &c. , which are not only of a lower temperature , but are also few in number , if we may deem those that fall within the visible part of the spectrum a sufficient sample of the whole .
Since , then , there is so much greater any escape of heat from the upper layer of the iron atmosphere than from the regions outside , there will exist a surface of minimum temperature near the limit of the iron , beyolnd which there will be first a very slight recovery and then a gradual fading off of the temperature .
The observations of the sodium lines indicate that this surface of minimum temperature which lies near the outer boundary of the layer from which iron lines originate , cannot be as hot as the flame of a Bunsen 's burner .
41 .
Within the iron atmosphere , on the other hand , there is a rapid stream of heat directed outwards to supply the outpourings from near the boundary of the irorn atmosphere , as well as what is feebly dispersed by lines such as those of hydrogen , sodium , and magnesium .
Still further downi the stream becomes a torrent , as it has there to supply also the lavish expenditure of heat by the multitude of lines more faint than the iron lines , which are not only more numerous than lines of any initensity comparable with the iron lines , but also each one of which discharges into space a flood of heat proportioned to its exalted temperature , or , in other words , to its faintness as a linle in the spectrum .
All this leads us to coInclude not only that the temperature increases very rapidly within the iron atmosphere , but that the rate of this increase becomes more and more precipitate as we descend .
And this is in exact accordance with the iintelligence brought to us by the sodium lines , which , from being winigless , indicate that the interval from the surface of the iron to the region where the temperature first becomes comparable with that of the .
photosphere , is both intensely hotter , and of trifling extent wheln compared with the vast expanse from the surface of the iron up to the surface of the sodiumn atmosphere .
42 .
Molecules of magnesiuim have very nearly the same mass as molecules of sodium .
The two gases therefore rise to nearly the same hieight in the solar atmosphere .
Nevertheless the lines in the spectrum due to magnesium present a very different aspect from those of sodium , into which we must now inquire .
The lines of sodium are narrow and sharp ; those of magnesium broad and friniged , the borders being of the intensity that Kirchhoff represents by the number 4 .
Now , the iron lines in their neighbourhood are of intenisities 5 and 6 , which shows that the upper layer of iron in which the iron linles take their rise may be distinguished into two strata , the outer of which produces in that part of the spectrum linaes of intensity 6 , while both together produce lines of intensity 5 .
To produce a line of intensity 4 , a third stratum below the layer in which iron lin.es originiate must be in action .
Light reaches us from this third stratum in the wings of the magnesium lines ; and in fact the black part of the manesium lines is due exclusively to the magnesium vapours between the top of the magnesium atmosphere and the plane of demarcation between the two strata into which we have distinguished the active layer of iron , while the wings are caused , at least in part , by the magnesium vapour which exists in the lower section of the active layer of iron and in the stratum which immediately adjoins it beneath .
Thus the layer of magnesium which gives rise to the lines of the group b may convenientlv be distinguished into two parts , the outer of which extends from the remote boundary of the magnesium atmosphere to the middle of the layer from which iron lines originate , and the second from this latter station through a hotter layer which lies further down .
If magnesium vapour existed in the situation of this lower moiety only , the magnesium lines would be bands of their present breadth , but nowhere attaining the intensity 6 : the superposition of the central black stripe is the work of the magnesium vapour in the vast outer section .
43 .
When we take into account how much higher a specific opacity sodiuim and magnesium vapour have than iron for the principal rays which they respectively emit , we are led to conclude that while magnesium vapour is abundant when compared with the attenuated vestige of sodium in the sun 's atmosphere , it may be but sparingly present when compared with such a constituent as iron ; and that this is so is established by the abselnce from the sun 's spectrum of any lines corresponding to the rays of magriesium , in reference to which the specific opacity of magnesiutm is low , such as the magnesium lines 44-92 and 46 06 .
44 .
We have found that there is but the merest trace of sodium in the sun 's atmosphere , and that this trace mounts to an immense height above the iron .
To render this possible there must be some abundant gas which extends as far as or beyond the sodium , in which it may diffuse itself , and so be borne to the full height corresponding to the small mass of its molecules .
The gas which does it this service appears to be hydrogen , which , having a molecular mass only one twenity-third of that of sodium , must soar to an almost inconceivably greater height .
Hydrogen seems to be a very large constituent of the sun 's atmosphere .
There are three considerable rays in the spectrum of incandescent hydrogen , and a fourth faint one has been lately pointed out by Angstr6m .
To these four rays , even to the faintest , there correspond intensely black lines in the solar spectrum .
This indicates an abundance of hydrogen .
The wave-lengths of the four lines are 41 04 , the new hydrogen line , Angstr6m 's h , in the violet ; 43*43 , in the indigo , which is the second of the six very conspicuous lines seen in the sun 's spectrum on the less refrangible side of G ; 48'65 in the blue , which is Fraunhofer 's F ; and 65 68 in the red , which is Fraunhofer 's C. All these lines are wing , ed : the black stripe in the more refrangible lines is very broad , and in the others it is of considerable width .
These circumstances also indicate an abundance of hydrogen .
The te-mperature of the sun 's atmosphere above the surface of the iron is too low to dilate hydrogen lines .
The breadth , therefore , of the black part of the hydrogen lines must be due to the quantity of this element which is to be found in the interval between the outer boundary of the iron and -that situation in which the temperature first becomes too high to appear black when projected against the brightness of the photosphere .
This interval is small in the part of the spectrum where the line C occurs ; at the line F it extends through a considerable part of the thickness of the layer that gives out iron lines ; at the hydrogen line near G it extends quite through this layer ; and in the situation of the fourth hydrogen line it extends much further down .
But even in the least of these intervals there is ugh of hydrogeni to give a very sensible breadth to the lilne C. This quantity must be very considerable ; as also mutst the quantity which can produce , in the hotter regions below , the fringes which border all the hydrogen lines .
To recapitulate , the width of the hydrogen lines , the wings that fringe them , the intense line in the sun 's spectrum which corresponds to a faint hydrogen ray , and the height to which hydrogen can support traces of other gases , and more especially the vestige of sodium in the solar atmosphere , all testify to the abundance of this element .
45 .
The sodium lines D are an open channel through which heat is pcured from a very hot region into that imimense upper expanse of the sun 's atmosphere which is tenanted by sodium , magnesium , and hydrogen alone .
This is not the case with the magnesium lines of the group 6 , nor with the four hydrogen lines .
These all stop heat before it has travelled to any great distance , by reason of the great abundance of hydrogen , and by reason of the specific opacity of magnesium for the rays 6 , and its quantity , which , though small , is immeasurably greater than the quantity of sodium .
And on a different account , the same may be truLe of the faint rays of the spectra of sodium and magniesium .
Two such magnesium rays were observed by Kirchhoff of wave-lengths 44 92 and 46-06 ; and Huggins has recorded three faint pairs of sodium lines , of wave-lengths 51F6 , 56-9 , and 616 , and a nebulous band at 49 9 .
It is not yet fuLlly ascertained whether there are iines in the solar spectruim answering to any of these rays .
If there are such lines , they are fainit .
Now , if it shall prove that no such lines can be detected , it will indicate that heat from beneath of these wave-lengths passes without sensible diminution through the cool parts of the sun 's atmosphere and therefore does not heat them ; and if it be fouind that they give rise to faint lines , this faintness is to be attributed to but little of the heat despatched from hot regions being entangled in its passage ouitwards .
Similarly the hieat which is so transmitted through the wings of conspicuous lines crosses with little obstructioni the colder regions above ; since at the temperatures that there prevail few of the periodic times of the atomic orbits deviate sufficienitly from those celntral periodic times which corresponid to the mniddles of the liines .
46 .
But of whatever kind these or other vehicles for the conveyanice of heat beyond the atmospheres of calcium and iron may be , it is certain that nto sodium or magnesium rays can carry heat beyond the limnits of the sodium atmosphere .
It is also certain that the heat borne outwards is unlable to maintain beyond the iron atmosphere a temperature as high as that of a Bunsen 's burner , and that , after passing a situation but little outside the iron , the temperature alls off from this maximulim .
It must have sunk very low where the next considerable escape of heat takes place -at the boundaries of the atmospheres of magnesium and sodium .
Accordingly , we must regard the hydrogen in that still higher dreary waste which is tenanted by hydrogen alone , as a feebly conducting body , of imnmense depth , warmed but mederately beneath , and exposed on : the outside to a chilling radiation towards the open sky .
Its outer strata must be intensely cold .
47 .
The case of a comet consisting of a gas * not found in the solar atmlosphere is altogether different .
As it approaches the sun it is exposed to the full unveiled glare of the photosphere , and absorbs the heat of those wave-lengths which correspond to the lines of its spectrum .
However small a part of the incident heat this may be , it may make the comet nearly as hot as an opake body would become ; since the comet can lose by radiation no heat except through these same spectral rays .
48 .
Having now examined in detail the lines of hydrogen , sodium , magnesium , calcium , and iron , Nve may treat in a more cursory manner the other elements that have been observed in the sun 's atmosphere .
Chromium , nickel , cobalt , copper , and zinc enter in small quantities into the composition of the sun 's atmosphere .
Probably nickel is the most abundant of them .
Of the others no lines appear in the suni 's spectrum , except those in reference to which they have a high specific opacity , in many cases higher than that which iron has for any of its rays .
There are , therefore , but traces of them present ; and the appearance of the lines agrees well with the situiation in the sun 's atmosphere assigned to them by the masses of their molecules : chromium , projecting quite through the iron atmosphere , produces a few lines of an intensity comparable with that of the iron lines in their neighbourhood ; and the boundaries of cobalt , nickel , copper , and zinc , appear to lie within that upper layer of iron which sends forth iron lines .
49 .
The appearance of the zinc lines is not incompatible with this element 's having the vapour-density usually supposed by chemists , viz. , 32-5 instead of 65 ; but the evidence of the sunl 's spectrum , such as it is , for it is scanty , owing to the paucity of the lines , seems to lean against this hypothesis , unless a similar reduction is to be made in the case of all the other metals of the atmosphere .
But whatever uncertainty may rest on this point , there is at least no doubt that barium cannot have a vapourdensity anything like so high as 137 .
At most it cannot exceed half that number , which would barely raise the boundary of the barium atmosphere within the lower part of the layer from which iron lines proceed ; and , if it were not for objections on chemical grounds , the strength of such lines as the barium lines 45 66 , 49 37 , and 61-43 would prompt us to suspect for the vapour of barium even a lower density .
But the strength of these lines is probably due to the remarkably high specific opacity of the vapour of barium in reference to them .
There is plainly only a small amount of barium in the sun 's atmosphere .
50 .
It will readily be perceived that it is vain to look for the cause of any conspicuous line mapped by Kirchhoff , in any substance with a vapourdensity more than 70 times that of hydrogen .
This narrows very muci the field in which to search for the origin of the darker of the lines enumerated in Table III .
, opposite , the table of unappropriated lines .
Many of these , as , for example , three of the five lines of the group at 60'3 , are probably due to manganiese , and may be remnoved from this table , as soon as a list of the thirty manganese lines , lately identified by Angstr6m , shall have been published .
Others of them are probably some of the 460 iron lines , produced by a continuous electrical current , or among the additional lines which may be produced under like circumstances in others of the elements which we have been heretofore examining .
When all these are eliminated it does not seem likely that many conspicuous lines between G and B will remain to be traced to their source .
Carbon is probably as devoid of volatility as it is infusible ; or at all events the one probably bears some proportionl to the extraordiniary eninence of the other .
If this be so , it cainnot be a gas at the temperature of the situations from which dark lines come , or at least not in sufficient quantity to produce visible effect .
B-ut it is very much to be wished that a comparison shiould be made of the spectra of boron , fluorine , sulphur , chlorine , titanium , and plhosphorus , with the sun 's spectrum , and especially of chlorine , if any weigDht is to be attached to the suspicion , fournded on very insufficient grounds , that the solar lines 43 40- , 43 55- , 66 38 , 66 50 , 66t68 , and 70 00 , the grouip of three lines at 45 1 , and several others , are to referred to this element .
51 .
The absence from the sun 's atmosphere of such gases as nitrogen and oxygen , and of hydrogenl from the atmospheres of some other stars , and the fact that while some active chemical agents lose , like sulphuric acid , their energy under such increasing temperatures as our laboratories can provide , others , like boracic acid , become practically more powerful , give a considerable amount of colour to the presumption that compound bodies exist in the sun .
The masses of the molecules of these compound bodies will in most cases be too-high to permit them , however volatile , to reach the cool parts of the sun 's atmosphere , so as to reveal themselves in conspicuous solar lirnes .
But the probability of their so appearing is very much greater in the class of ruddy stars , as we shall find in the sequel ; and , perhaps it is not impossible that the line B of the solar spectrum , or some of the lines less refrangible than B , may result from some compound of low vapour-density , such as hydrochloric acid* .
It is certainly very remarkable that neither B nor any lille less refrangible has up to the present been identified with a ray of any simple substance .
52 .
Upon a general view of all the lines of the solar spectrum it appears that their intensity continuously diminishes from the violet end of the spectrum up to the line B. At this point , owing to the sudden introduction of an entirely new set of lines , their intensity abruiptly and very much increases .
These new lines either have a terrestrial origin or come from substances which stand high in the solar atmosphere .
The linles , however , which originate further down , do not attain their minimum of intensity until they reach a point further to the right than B. This appears both from the progressive diminution of their intensity up to B , and from the total , or almost total , absence of linses further on , wherever a vacuity is left between the lines which we must attribute to a different origin , as at wavelengths 71'1 , 73-8 , and in the wide spaces between the prominent lines from this situation up to the line A. 53 .
When this is considered in connexion with the cause to which the diminution of intensity is to be referred , it indicates that if two perfectly radiating bodies were gradually heated while the difference of their temperatures was kept constantly the same , the point of the spectrum at which the difference of their brightness is least would advance with increasing temperatures towards the red end of the spectrum .
When the body of lower temperature has but just begun to glow , we know that this situation of minimum difference of brightness is found in the orange ; at temperatures approaching that of the photosphere it has removed at all events as far as the line A , that is nearly to the extreme verge of the visible spectrum , and it has , perhaps , advanced beyond it .
This , as we shall find further on , explains how some solitary stars can attain a depth of colour that approaches crimson .
54 .
It appears from the analysis which has been made that none other of the gases in the solar atmosphere that extend as far as the stratum from which iron lines come , can compare in quantity with hydrogen and iron ; and from what has been stated in ? ?
36 , we may be sure that there is no very abundant gas which comes to its limit in the hot regions that intervene between this stratum and the photosphere .
Hydrogen and iron are accordingly the principal ingredients of the parts of the sun 's atmosphere which extend beyond the photosphere .
Section IV.-Of the Photoslphere and the subjacent parts .
55 .
In interpreting phenomena of solar spots we should never forget the disadvalntages under which we attempt the enterprise .
Our theory may be true , but it is incomparably more tneagre than our knowledge of the causes of terrestrial weather .
Our observations may be correct , but they give us only outside glimpses , and from such a distance that France or Spain would be specks too small to make out whether they are round or square .
We must not imitate the peasant who saw from afar the smoke of a great city , and persuaded himself he had a very good idea of the kind of place a city is .
If our explanations of the phenomena of terrestrial weather are dim and unsatisfying , we cannot reasonably ask from a theory of the corresponding phenomena of the sun , even though it were beyond a doubt the true theory , more than the first hazy and rude sketch of an interpretation .
56 .
Many fixed gases which are too heavy to extend at all , or in any abundance , through the stratum of minimum temperature , must wax in density very rapidly within it .
Hence the density of the solar atmosphere becomes almost suddenly greater at the shell of luminous clouds .
This may be the cause of an appearance not unfrequent in spots near the margin of the sun 's disk , in which situation the further side of the umbra of a spot is often bordered by a bright crescent , giving to the umbra the appearance of a hole punched through a plate .
This appears to be because there is , in these cases , in reality a depression of the dense strata at the umbra , shallow , perhaps , but yet with sides sufficiently iniclined to enable light coming so obliquely as to suffer total reflection* against the flatter surface of the penumbra , to escape through it .
A similar cause may , perhaps , and probably does , enable light to escape from patches of the penumbra when the surface of the penumbra is irregularly undulating in a sufficient degree .
t Such as that which produices Fata Morgana .
Local showers are in other cases the cause of b)rightness in the umbra and penumbra .
The sudden increase of density of the sun 's atmosphere at the photosphere must serve to keep the lumninous stratum in a nearly spherical form .
The surfaces of the gases above the photosphere may be violently tossed about by the storms of the solar atmosphere , but the suirface of the photosphere is never carried further than to the top of a facula or the bottom of the umbra of a spot .
57 .
The winds which affect the photosphere may be distinguished into two classes , those of the sun 's outer atmosphere , and those of the regions within the photosphere .
Both classes may coexist in different parts of the same storm .
The former class sweeping through the open space above the photosphere , and through rarefied air , will often come from far , and as a general rule be the swiftest .
Those below , moving in the dense part of the atmosphere , and perbaps within a confined space , can but seldom attain the same high velocity .
58 .
Both classes of wiind tenid to obliterate the cool filmn in which clouids usually exist , and to replace it by hotter air .
But the hotter air substituted by winds from below , will be equally charged with moisture ; while winds from above will tenid to dilute with dry air both the cool film and the adjoining strata immediately under it .
In both cases new and more transparent clouds will form ; but in the former case the rain will not cease , and we have only facula ; in the latter it may and often does , in fact , whenever the film of clouds and the subjacent stratumn with which it is mixed by convection , have been rendered sufficienitly dry .
When by proloniged convection this state of things is passing away , there will be a struggle betweeni dry weather and wet , which we shall see in the patched appearance of the penumbra .
59 .
Anr umbra presents itself when the cloud , too , is removed , and the dusky body of the sun seen through the opening .
It does not seem likely that this can take place so loing as there is any of the moist stratum at a temperature below its boiling-point and exposed to radiation .
If this view be correct , the umbra can only occur either when the depression caused by a rotatory storm , or by winds impinging from above , has obliterated the dense stratum and brought the air into contact with the ocean ; or when , by the influx of hot air from above or the upheaving of the hot strata beneath , it has come to pass that throughout the whole of .
a vertical column there is no place where the vapour which forms cloud is at a temperature below its boiling-point .
If this happen through the rise of subjacent strata , we should have an umbra without penumbra ; and it does not seem impossible that the same appearance may sometimes present itself where a depression is caused by a wind impinging from above which has not exerted much horizontal friction against the surrounding parts of the photosphere .
60 .
It must often happen that a hot current sweeping over the surface of the penumbra dissolves away part of the cloud , diluting the vapour D with dry air pip to the poiint of being but just unlable to precipitate itself while exposed underneath to the heat of the penumbra .
If a current so charged with vapour happen to cross the umbra , it will receive less heat from below , and some of the vapour in it will now be able by radiation to maintairm itself as cloud .
This cloud will be pecuiliarly circumstanced .
It is formed from ans isolated body of vapour , and on-ce formed will continue in existence , sinice the hot currenits which will rise at intervals through it when convection sets in , will consist of dry air uniable to generate the cloudl overhead , which would otherwise screen it from the open sky .
It will accordingly often find itself unider circumstances to become by reason of this prolonged existence progressively cooler ; and as the temperature falls , more of the vapour is able to precipitate itself , unitil at length the cloud becomes so dense that rain sets in .
The rain is probably caught and dissolved in the dry air below , long before it can reach the body of the sun ; but if it last through a space of even a few thousand metres , it will give to the bridge of vapour the brightness of a facula .
In other cases the vapour either carried into the umbra from around , or perhaps rising into it from a steaming ocean beneath , appears to form mere pellicles of cloud that mottle its deep shadow .
When the storm is of the nature of a whirlwind , a current of dry outer air which has not lapped up moisture from the photosphere , usually seems also sucked in , and manifests its presence in the dark spot which AMr .
Dawes has called the nucleus of the umbra .
61 .
It appears more reasonable to suppose that the phenomena which have hitherto beeni explained by the transference of ponderable matter over immense distances in inieredibly short tim-les , the filling , up of gulfs , and the like , are phenomena of the rapicl formation or dissolution of cloud , and lose inuch of their marvellous character .
Terrestrial cloud may be seen to form within a very few miniutes over the whole of the visible heavens , and often when there is no winyd , or apparently advancing against the wiild .
62 .
If there be a substanice in the sun of low vapour-density , but nCot capable of existing in .
a state of vapour in the coolness of the height to which it would otherwise rise , and if this refractory substance is volatile at the temperature and pressure which exist lower down , it will behave in a very peculiar manner .
In the lower strata of the sun 's atinosphere it will exist as a vapour ; and ffromii this situation it will keep continually making its way upward in its effort to find its natural level .
Before it reaches its destination , Lowever , the gas incessantly streaming upward will as incessantly be precipitated .
If the particles of the cloud so formed are heavier than the survounding atmosphere , they will begin to subside .
Not only so , but the chill caused by their radiation in their new solid or liqlaid state , will make the inverse flame spoken of in ? ?
8 burrn downwards , until it sinks to that level at which the upward supply of vapour , owing to its tendeney to diffuse itself upwards , or caused by currents of convection , exactly balances the downward motion of the fiery cloud from subsidence or the desecndiDg currents of convection.:Here , then , if this substance be in sufficient aburndance , we have all the conditions niecessary for the sun 's luminious clouds .
And we are led almost irresistibly to colnjecture that in carbon* we have such a substance .
The mass of its molecules is very low , either six , or twelve , or twenty-four times the mass of a molecule of hydrogen .
It appears to have just the requisite degree of fixedness ; it shows ino sign of volatility at any ordinary high temperature , but has been driven into vapour by one hundred elements of Bunsen 's battery , each element consisting of six ordinary cells coupled side by side ; that is at a temperature which may , quite consistently with everything we know , be that of the strata adjoining the sun 's photosphere .
There is enough of carbon in the sun to produce the lumiiinous clouds , if carbon be as large a constituent of the sun as it is of the earth ; and most of the carbon in the sun is probably uncombined , as carboll does not seem apt to form compounds likely to be abundant which can stand intense heat .
It is , moreover , precipitated from its vapour as a black body with the most perfect power of emission of any known substance ; and we are assured that the lumirious clouds consist of some such material by the absence of bright lilnes from the solar spectrum .
It would probably be impossible , in the present state of our knowledge , to put forward on behalf of any other substance , simple or compound , anything like the same claim to be deemed the material of which the luminous clouds consist .
And I know ' of but one consideration to be set on the other side , viz. that if the luminious clouds be a smoke of carbon , and if the rain beneath is more properly to be described as a fall of soot , in flakes like snow , and if these flakes come to rest upon the surface of an ocean beneath , they must by their high radiating power render this surface eminently luminous , which we know from the phenomena of spots that it is not .
63 .
As , then , there are strong reasons for surmising that the luminous clouds consist of carboni , we are led to enquire what may exist to remove the one difficulty in which this hypothesis involves us .
Now , in the first place , it would disappear if the heat in the space beneath the clouds melts the falling flakes , so that they reach the ocean like rain , and mix with the other liquids constituting it .
And it would disappear if the heat and dryness of the space beneath the clouds enable it to evaporate the flakes ere they reach the ocean .
And , finally , it would disappear if there be ino suich ocean , but only a continuation of the atmosphere becoming denser and hotter .
It will be lnecessary to examine this last hypothesis with some care to see that it is compatible with the known phenomena of spots .
64 .
It is not likely that carboln is the only substanice in the sun that possesses the properties which are the conditions for the formation of cloud , although it is probable that carbon is , of such substances , that one which has by far the lowest vapouir-density , It is , at all events , presumable that among such aburndanit elemenits as nitrogen , oxygell , silicium , and altininium , or such of their compoulds of low vapour-density as ca-n exist in the sun , there may be some which , like carb-on , are solid or liquid at the temperatures and pressures of the greatest heights to which they would , if gaseous , rise .
And if the atmosphere of the sun extend to any great distance below the photosphere , there must be in the sun such a substance to account for the dusky backgrounid we see in the penumbrm and umbrme of spots .
There must in this case be a seconld layer of clouds , formed not far beyond the photosphere , in the comparatively short space through which the temperature aug ments rapidly between the luminous clouds and the central parts of the sun .
These clouds must , moreover , be of some transparent material to possess in a sufficient degree that property of scattering light which would render them as devoid of emissive power as we see them to be .
For the saml-i reasoni we must conclude that the sooty shower from above caninot reach them , as it would inevitably soil them , so as to deprive them of these essential qualities .
We learn from this , that the point at which carbon boils must fall withini the short interval betweel the two layers of clouds .
This is not at all unlikely , inasmuch as the advance downwards of the inverse flanie , of which mention has been so often made , would probably be arrested only by its close approach , either to the bottormi of the atmosphere , or to the situation in which carbon boils , so as to be entirely dissipated in vapour .
Aned the secornd layer of clouds would quickly follow , since its position depends on that taken up by the carbon clouds , as it must lie within the layer of rapidly varying temperature immediately under them .
If this hypothesis , then , be the true account of what takes place on the sun , the penuimbrre of spots are caused by our seeing the clouds beneath through a gauze-like film of carbon cloud which has ceased to senid down rain ; and the umbrte of spots are formed when a very shallow saucer-like depressioni of the photosphere has carried a part of its outer surface so far that it has reached the region in which carbon will boil .
Here the filmy clouid of carbon , which nowhere else can entirely disappear , will be completely dissolved away .
65 .
In this branch of our enquiry we are often obliged to deal with hypothetical matter , and cannot in such cases look for conclusions which command our assent .
We must 'be satisfied if we may hope that they will prove of use in guiding future inlvestigations .
Nevertheless , I am disposed to think that we should give the preference , as a provisional hypothesis , to the supposition of a layer of cloud lying under the photosphere , rather than to the only other alternative which seems in any considerable degree admissible , namely , a highlly reflecting ocean .
It is perhaps , on the whole , and in our present state of ignoranee , enicuimbered with fewer difficulties .
Section V.-Of Clouds in the Outer Atmosphere .
66 .
But to return to what is more to be relied on , we may be suire that some small part of the carbon , or whatever else the luminous clouds mainly consist of , and similar traces of any other ingredients that enter in less quantities into their composition , must escape precipitation , and will diffuse themselves upwards , and the more freely as they come first to a region where they are raised to a higher temperature as well as subjected to less pressure .
Through this hot stratum they will continiue gaseous , but a short distalnce above it they will meet with a temperature low enough to condense them .
Here , then , separated from the photosphere by the whole depth of the hot stratum , they will form a second film of luminous clouds , one , however , which is so attenuated as to be visible only during an eclipse , when it constitutes the lowest of the clouds that then present themselves .
They may be traced in Dr. De La Rue 's photographs of the eclipse of July 1860* as continuous arcs of cloud extending about 350 on either side of the points of first and last contact .
Hence , and from the apparent magnitudes of the sun and moon on that occasion , we may conclude that this upper shell of clouds was at an apparent distance of about 11 " of space from the edge of the sun 's disk , which corresponds to an absolute height above the photosphere of 8 metre-sixes , or 14 time the earth 's radius .
And as the clouds of which we are now speaking are a little outside the hot stratumn that lies immediately over the photosphere , we sball not be far wrong in concluding this stratum to be about as thick as the earth 's radius is long .
The clouds outside it probably form a nearly contilnuous shell round the sun .
They are everywhere of extreme tenuity , but may nevertheless be very variable in density ; and it is probably owing to this that the concave sides of the two arcs shown in the phiotographs exhliibit such a ruggedness that , as Dr. DDe La Rue has pointed out , it cannot be accounted for by the mountainous edge of the moon .
In fact the film of cloud seems to be so excessively thin that even during an eclipse it can only be seen where it is presented very nearly edgewise at the extremiie margin of its disk , or for a short distanice inside it , a distance which varies with the local density of the film , and so gives rise to the appearance in questioni .
67 .
This second shell of clouds , as they consist of the same materials as the clouds of the photosphere , and are higher in the atmosphere , and therefore subjected to less pressure , will evidently not form urntil they can do so at a somewhat lower temperature .
But the difference may be so slight that in their normal position these clouds lose more heat by radiation towards the sky than they receive by absorption from the photosphere , which would cause them to imitate , but with a languor proportional to their flimsiness , all the phenomeila of convection , &c. which we have traced in the prinicipal layer of clouds .
68 .
But this behaviour would be altogether changed if by any cause a part of the film were borne upwards into the cool regions above .
At whatever part of the atmosphere a cloud may find itself , it will be exposed to the unmitigated glare of the photosphere , and will be raised by it to a temperature bordering upon that of the photosphere itself* .
A cloud in this situation will therefore warm , instead of cooling , the air in which it is dispersed , and will tend to float violently upwards until it gets to a part of the atmosphere so rare , that the particles of condensed vapour tend to sink in it from their specific gravity as fast as they are carried upwards by the body of heated air entangled with them .
This may be the cause of the columnar clouds with overhanging tops which have been observed during eclipses .
As they spread out at the top and become diffused , they will not as effectually heat the intermingled air , and will therefore begin to subside .
Between clouds that are carried so violently upwards and those that repose in the luminous shells , any intermediate descriptions may exist , and were perhaps the cause of the mountainous projections from the upper shell that have been seen , and of several of the detached clouds .
69 .
But besides the materials that enter into the composition of the clouds of the photosphere , we must renmember that there may exist other substances in the sun or in some other stars ca-pable of giving rise to clouds .
If there be materials of sufficiently low vapour-density , and in a sufficient degree more volatile than carbon , though not volatile enough to stand the cold of the height to which their vapour-density would otherwise lift them , they will be precipitated in cloud .
Or gases in the solar atmosphere which are kept asunder by the temperatures of its lower strata , may be able to combine in the cooler regions above .
If the new body be a solid or liquid , it will constitute a cloud .
Even if it be gaseous , it will in general have other spectral lines than those of any lower-lying gas in the atmosphere , and will therefore be subjected to the direct radiations of the photosphere ; it will accordingly become intensely heated , and in many respects behave like a cloud .
Its density , too , will in most cases be greater than that of either of its constituents .
And , finIally , a gas which in the lower parts of the sun 's atmosphere emits only rays of a spectrum of the second order , may in the upper regions find itself urnder circumstances to produce a spectrum of the first order .
If this should happeni , the gas in its new condition would be exposed to the full heat of the photosphere , and would conduct itself like a cloud .
70 .
From the exceeding transparency of the solar clouds , they are entirely without that abundanlce of internal reflections and refractions which are what give to a cloud of steam dense enough to be opake , or a sheet of paper , or a piece of white marble , their lustre when illuminated .
It is accordingly by their inhereilt splendour given to them by their being made intensely hot by the photosphere , not by borrowed light , that they shine .
A cloud of dark opake materials is therefore , cWteris paribus , the brightest .
Those which Mr. De la Rue found impressed on the photographs , though not visible to the eye , must have been of substances transparent in regard to most visible vibrationis , but opake for some of higher refrangibility .
71 .
It is very likely that there may be substances in the sun 's atmosphere , or in those of some of the stars , which reach a height at which they are unable to remain in the state of gas by reason of the surrounding cold , or to assume permanently the form of cloud because of the heat of the photosphlere to which they would thereupon immediately become exposed .
In such cases there will be a struggle between the two conditions , the vapour continiually condensing and redissolving until it has by this process imported much heat into its nieighbourhood .
Wherever such a state of things exists , it must inevitably have the effect of raising some of the isothermal surfaces above the position in the atmosphere they would otherwise occupy .
Similar consequences would ensue if two gases became so cool that they could no loniger continue uncombined , and were so heated through their new spectral lines the instant they united that the new substance was at once resolved back into its constituents ; or where a gas reaches a situation too cold for its existence in the state in which it sends out spectral rays of the second order , and no sooner changes its condition than it absorbs through its new spectral lines heat to such an extent that it must fall back again .
Such struggles may be the prolific source of stormns when they are local , and perhaps of an appreciable variation in the brightness of stars when they are on a great scale .
Section VI.-Of the Distribution and Periodicity of the Spots .
72 .
We may catch a glimpse from the foregoing investigations of what appears at least a possible explanationi of several pheniomenia of the solar spots , which we do not seem yet in a position to refer to their causes with confidence , such phenomena as the local distribution of spots and their periodicity .
If from any cause a portion of the lower strata of the outer atmosphere is thrown upwards , it will carry a part of the second stratum of clouds above its natural level .
The intermingled air will dilate and tend to cool down as it ascen-ds ; but its temperature will be restored by the heat absorbed and communicated to it by the cloud carried with it .
Its thus remaining hot will convert what was perhaps at first only a gentle upheaval into a violent upward current , which will , from the operation of cauises familiar upon the earth 's surface , occasion a cyclonie in the lower strata of the outer atmosphere .
The inner atmosphere ( that is , the dense atmosphere from the surface of the photosphere downwards ) canrnot be readily drawn into the vortex , by reason of its great specific gravity ; but it will be swept round and round by the violence of the hurricane above , and a kind of whirlpool will result which will depress the cenitral parts into the peniumbra and umbra of a spot and lift its borders into faculue .
The for mation of this whirlpool will be greatly assisted if , as we shall presently see we have reason to suspect , there are preexisting currents in the inner atmosphere setting in opposite directions along the zones of spots .
73 .
If , then , we are right in attributing a large proportioni of the spots to ascending currents in the outer atmosphere , we must next seek some cause which can determine the existence of such upward currenits in two bands parallel to the equator .
It is natural to look for this in some phenomenon analogous to our trade-winds ; and , as Sir Johnl 1-herschel has observed , such a phenomnenon may arise if the ellipticity of the suni bring about an unequal escape of heat from his poles and from his equator .
The elliptic strata of the atmosphere could be in equilibrio only on the supposition that they are of precisely the same density throughout : but this they cannot be ; for as the outer atmosphere is an imperfectly conducting plate , heated on the one side by the photosphere , cooled on the other by radiation towards the sky , at the poles , where the plate is thinnest , its outer strata will be sensibly hotter than their average temperature over the whole sun , and their inner strata very slightly cooler ; and at the equator , where the plate is thickest , its inner strata will be hotter than the average , and its outer strata cooler .
Helnce at the poles , where the temperature of the outer parts of the atmosphere is higher than the average , t hey will diffuse themselves upwards and overflow ; at the equator , where the temperature is less than the average , they will subside and tend to escape laterally at the bottom .
Moreover , the lower strata being subjected at the equator to more pressure than the average , by reason of the coolness of the superincumbent strata , and to less pressure at the poles , will also contribute to produce an under-current in the outer atmosphere from the equator towards the poles .
Hence if it were not that the rotation of the sun modifies the result , we should have a constant wind blowing steadily from the equator to the poles over the surface of the photosphere , and a counter-current in the upper regions.of the atmosphere .
74 .
The effect upon the inner atmosphere is directly the reverse .
heat will escape from the photosphere very slightly more freely at the poles , less freely at the equator , than the average .
The upper strata of the inner atmosphere will therefore be a little lighter at the equator , and will overflow towards the poles , tending to produce a feeble surface-current in the photosphere in the same direction as the wind which blows above it from the equator towards the poles .
75 .
But the suni 's surface is all the time being carried round by his rotation from east to west .
This will impart a strong westerly direction to the descending current where it reaches the phiotosphere at the equator* , and will further render it where it spreads out over the photosphere towards the poles , a south-east wind in the northern hemisphere , and a north-east wind in the southern .
Thus these winds blow in such directions as to rotate more rapidly than the general body of the sun , and they therefore seek to raise themselves above the photospheret .
At the eciuator the upward tendency expenlds itself in somewhat retarding the descending current , but a few degrees on either side , where this obstacle has become sufficiently feeble , it determines extensive upheavals of the lower strata S. Polar calms and l/ ascending curreiits.\ / one of variable winds produced by descending currents.\ Southern zone of variable winds produced by currents about to asceid .
Northern zone of variable winds produced by currents about to ascend.\ / // /#f Zone of vrianble winds produced by descendiig currents .
Polar calms and ascending cur ents .
_ N. Diagram of the winds supposed to blow over the , photosphere of the sun .
of the outer atmosphere , which , however gently they may begiD , we have seen will terminate in a cyclonie .
Hence the two belts of spots on either side of the equator .
In somewhat higher latitudes , the equatorial current having ascended , and , as it were , split the polar eurrent into two sheets , has diverted one of them along the surface of the photosphere .
In these regions , therefore , there is a constant wind blowing over the photosphere from the north-west in the norther hemisphere , and from the south-west in the southern .
Accordingly , in the two zones of spots there are probably variable winds blowing over the photosphere , the polar and equatorial currents threading their way through each other , and both tending upwards , like the fin gers of the two harnds interlaced into one another .
MvTearnwhile the equatorial current which had risen into the middle of the atm-osphere over the zone of spots exchan , ges , in the northern hemnisphere , its north-westerly direction , first for one due nortb , and then for one towards the north-east , as it ascends still higher .
But this temporary effect of its vertical miotion will be lost , and it will again , when it ceases to ascend and advances only horizontally , direct its course to the north-west , until , in higher latitudes , the swifter rotation which its westward direction imparts to it nlo longer offers any sensible impediment to its sinking in the atmosphere * .
And here it will be iniduiced to do so by meeting in greater conicentration the upper polar current , coming too from regions of slower rotatory motion , and therefore with a tendency to descend .
-lere , then , will end the space throughout which it has split the polar current into two sheets .
It descenids to the surface of the photosphere producing a zone of variable winds-in this case , however , caused by polar and equatorial currents which are both deseending , and so unable to give rise to cyclones .
Between this and the pole the equatorial current seems to be next the photosphere , and blows somewhat towards the pole , but chiefly from the east .
There will be ascending currents about the poles ; but they will breath upwards so gently , and over so great a space , that they are probably unequal to the .
task of heaving up the upper stratum of clouds in the vigorous way that leads to cyclones .
Our conclusions may now be collected .
The annexed diagramn shows in one view the directions of the variouis trade-winds that seem to blow over the surface of the photosphere , and the prevailing character of the zones that separate them .
The diagram is in the position in which the sun 's disk is usually seen in a telescope .
76 .
We found that there is in the ininer atmosphere a slight tendency to produce surface-currents from the equator towards the poles , owing to the greater escape of heat at the poles .
But the inifluence of the winds in determining currents in the photosphere over which they sweep is probably so predominant , that both between and bevonid the belts of spots they are able to determine the currenits in the photosphere , those of middle latitudes being , accordingly currents towards the east , whilst the equatorial and polar currents set in the opposite direction .
Such currenits would evidently conspire with the winds that blow over them to produce agitations in the photosphere .
They would also contribute to that proper motion of the spots in longitude which has beenl observed .
77 .
We appear to be compelled to resort to some external cauise to account for the periodicity of the spots .
Among causes known to exist , that wlicil seems to offer itself with most plausibility for our acceptance is a swarm of meteorites like those which visit us in November three times in a cerntury , and those which visit us in other months every yeart .
To accoiunt for the periodicity of the spots , we must suppose the meteorites to describe their orbit in 11 11 years , the period of mutations of the spots .
Henice the semiaxis major is 4 98 times that of the earth 's orbit .
The perihelion distance must be very small ( say , 0 01 ) to admit of the swarmn 's grazing the sun 's atmosphere at each perihelion passage .
This would assign 9 95 to the aphelion distance , a quantity from which it cannot much deviate .
Now the mean distance of Saturn is 9 54 ; so that we may safely conclude , if the explanation which is now offered is the correct one , that the meteorites in questionl were diverted into the solar system , by either Jupiter or Saturn , at no enormously remote period ; just as the November meteors seem to have been brought in by the attractionl of the planet Uranus in A.D. 126 .
At each perihelion passage some of the outlying members of the streamn become entangled in the upper parts of the suIn 's atmosphere , dashing through it at a rate of about 414 kilometres per second * .
The enormous friction they must undergo before they are brought to a state of relative rest will convert their immense vis viva into heat , which will be expended in raising the temperature of the upper strata of the part of the sun 's atmosphere upon which they act .
This part is of necessity more equatorial than polar , and is very much more equatorial than polar , except on the peculiar supposition , which we have no reason to select , that the plane in which the meteors move is very niearly perpendicular to the plane of the sun 's equator .
The heat imparted by the meteors to the sin 's atmosphere therefore tends to diminish that defect of temperature in the upper parts at the equator which occasions the trade-winds of the sun .
The influx of meteors , therefore , into the sun 's atmosphere mitigates the violence of the trade-winds , and in this wav enfeebles the cause of cyclones and of spots .
Furthermore , except on the very improbable hypothesis that the axis-major of the orbit of the meteors lies exactly along the line of irntersection of its plane with that of the sun 's equator , the meteors must act more on one side of the equator than the other , and thus soften the trade-winds , and render the spots less frequent and extensive in one hemisphere than in the other .
So that the hypothesis of a stream of meteors has the following points in its favour:-it is a vera causa ; it accounts for two wholly distinct phenomena , the periodicity of the spots and their prevalence in one hemisphere more than in the other ; and it leads to such an aphelion disX The velocity of the sun 's equator is about 2 kilometres per second .
f [ It also accounts for the approach of the zones of spots to the equator during the periods of minimum spot-frequency ; inasmuch as when the current descending at the equator from great altitudes is enfeebled , the surface winds of middle latituldes , which have a tendency to cling to the photosphere , owing to their having a less rotationi , will encroach further upon the equatorial current and will thus bring the junction between them , along which the spots lie , nearer to the equator .
If the decennial mutations of the spots be due to a current of meteors , this hypothesis ought to offer some indication of the cause of fluctuations of longer period , such as that of fifty-six years .
This is perhaps to be sought in the great perturbation which the motion of the members of the stream must suffer from the attraction of Jupiter .
This planet must act upon them with intense effect , sinlce the planet and the meteors have niearly the same periodic time.-July 1868.1 taiice of the orbit of meteors as assigns to them a position into which either Jupiter or Saturn could have brought them .
78 .
If these solar meteorites exist , they would seem to have had time to extend themselves round the greater part of their orbit , and leave the vacant space smaller at present than that which is occupied , so as to render the phenomenon depending upon their absence , viz. the increase in the number and size of spots , that which develops itself in the most marked manner .
We may , then , perhaps presume that the epoch at which they came into the solar system was long before the year 126 , though , cosmically speaking , a recent occurrence .
79 .
This appears the proper place to observe that the heat which is so lavishly dispersed by the sun cannot be kept up , as has sometimes been supposed , by the continual falling in of meteorites moving in orbits round him ; since if that were so , the outer parts of the solar atmosphere would be kept intensely heated , which is contradicted by all the phenomena .
In the next part of this memoir , which will treat of other stars , I will offer what appears to me a possible account of the proximate source of solar heat .
PART II .
OF OTHER STARS .
Section I.-Of Solitary Stars .
80 .
Observations with the spectroscope having apprised us of the presence in the suni and other stars of several of the elementary bodies with which we are familiar on the earth , we are bound to assume provisionally and until something offers to warrant a different belief , that those which are abundant on the earth and in the sun are abundant elsewhere also .
Let us then consider how such differences as we must presume to exist between star and star would affect a body like the sun .
81 .
Star manifestly differs from star in mass ; they probably also differ in temperature .
Let us therefore inquire how a great change in the sun 's mass or in his average temperature would operate .
Strange to say , an increase of his temperature would produce many of the same effects as a diminLution of his mass .
This is because the dilatation of the sun 's bulk , and the consequent removal of the outer parts of his atmosphere to a greater distance from the centre would lessen the force of gravity upon them .
In either case , therefore , the effect upon the atmosphere would be the same as if the gases constituting it became specifically lighter .
They would all be able to maintain their footing with feebler molecular motions .
In other words , each gas would rise in the atmosphere until the distance between its outer layer exposed by radiation to the intense cold of the sky , and the inner layer heated by the photosphere , interposes a space of such thickness as will , in obedience to the laws of conduction , reduce the temperature on the outside to the lower miniimum which the gas can now endure .
Accordingly , the spectral lines of a star , either hotter or less massive than our suin , should be all of them more intenise than the corresponding lines of the sun 's spectrum .
MIoreover , maniy substances which by reason of the large mass of their molecuiles are uinable to stanid in the sun the low temiiperature * of the clouds of the photosphere , and are therefore confined to the regions within , are able , on a starwhich attracts with less force orwhose centre is farremoved , to pass through this obstacle and show themselves in the atmosphere above .
Finally , such stars will be ruddy .
The sun himself is a somewhat ruddv star , as may be seen by a glance at Tables II .
and III .
Both ends of his spectrum are subdued by lines .
The yellow , orange , and scarlet are nearly as bright as they came from the photosphere ; the green is sensibly shaded over by lines ; the blue suffers somewhat more ; the indigo about G and the crimson beyond B , very much ; and the violet from G to H to such an extent , that it is difficult to find a spot where the full light of the photosphere appears to penetrate .
The chemical rays beyond the violet are progressively more and more enfeebled as their wave-lengths shorten ; so much so , that the fluorescent spectrum from several artificial sources is longer , and from some much longer , than the sun 's .
A similar defnciency seems to exist at the other end in that prolongation of the solar spectrum beyond A , which Sir David Brewster has dimly seen and succeded in figuring .
Now every encroachment upon the spectrum will be more marked when very dark lilnes become numerous , that is , in stars hotter , or of smaller mass ; and if the lines themselves are pretty evenly distributed , it will subdue the different colours in proportion to their refrangibilitiest .
Ruddy stars , therefore , either have a less mass than our sun , or are more dilated by heat throughout the regions beneath the photosphere .
82 .
The consequences of the two other alternatives , of a star 's mass being greater than the sun 's , or of the temperatture within the photosphere being less fierce , so that these regionis are of less bulk , will be plain inow .
In such stars , some of the substances which range through the part of the sun 's atmosphere above the photosphere are imprisoned within that luminous shell .
Others of them , such as iron , calcium , and those of a like vapour-density , can only hold their ground while at a higher temrperature , alncl would show faint though numerous lines in the spectrum .
A few , such as sodium , magniesium , the substance that causes the line B ( if this ray be of solar origin ) , and above all , hydrogen , would perhaps still continue dark .
The lines of hydrogen , from its incomparably small vapourdensity , would be so much the last to yield , that there is probably no star with gravity so intense as to produce any sensible impression upon them .
And accordingly , in all very white stars which have been examined , these four lines stand out in extraordiiiay prominience .
83 .
It is now no longer a mystery why solitary stars are either white or of a red or yellow tinge .
In all those cases in which the dilatation of the central parts by heat is so proportioned to the mass of the star as to render the force of gravity upon the outer atmosphere the samue as it is upon the suin , the star will be equally white .
The class of more brilliantly white stars with an almost violet gleamn , such as Sirius and a Lyrae , are those with masses too great in proportion to their temperatures for this adjustment .
And , on the other haiid , those whose masses fall short of what the foregoing condition assigns , or , on the other side , whose temperatures are in excess , will , in proportion as they deviate from its fulfilment , have spectra more and more closed in upon that palt in which the spectra of two incandescent bodies differ least in brightness when the luminous bodies are at nearly , but not quite , the same temperature-that is , upon the greetn , yellow , orange , and red rays , uniting inito a tint which always inclines to either yellow , orange , scarlet , or crimson .
The minute crimson stars which are met with here and there in the sky seem to be either very small stars , or stars enormously distenlded by heat .
It is very desirable that the proper motion and parallax of these bodies should be inquired into when practicable , on the chance that some of them may be found to owe their colour to being very small , and therefore very close to us .
84 .
I need not say with what fidelity these maniy consequences of a change in the force of gravity in passing from star to star reproduce them .
selves in Mr. Huggins 's observations .
But before making the comparison , it will be well to consider rapidly what interfering causes may have to be taken into account .
85 .
We have hitherto spoken of the effects of the initensity of gravity in a star upon substances giving the same liines as we see in the sun .
Our results are therefore subject to modificationl wherever the system of lines is itself changed .
If , for example , the elements which give rise to the more prominent linles of the sun 's spectrum are wanting in the stars , other lines , which perlhaps are not , like those of the sun , pretty evenly spread over the whole spectruim , may take their place .
If this should happen , some colours will be more absorbed by them tfian others ; and this will tenid to give to the star the complementary tint .
In such cases the resultant effect will be mixed ; the effect of the cause just mentioned being blended with that strengthening of the lines at the blue end of the spectrumn which operates most when gravity on a star is weak .
We shall presently find that this state of things , which would be improbable in solitary stars , may have been brought about in the case of the companiions of some double stars .
Or , again , elements which in the sun are free may in the stars be found only in a state of combination , and be either absent from the star 's atmosphere or give rise in it to an entirely new set of lines .
This * has perhaps been the fate of hydrogen in a Orionis , P3 Pegasi , and the other stars in which theie are no lines corresponding to the solar lines C and F. If , however , the lines that are in this way withdrawn be as few as the lines of hydrogen , their absence will not sensibly affect the colouir of the star .
Anld finally , such conditions may prevail upon particular stars as will enable a spectrum of the first order to present itself , -that kind of spectrum in which the usual scattered linies of a spectrum of the second order are replaced by a multitude of fine closely ruled lines arranged in groups of regularly shaded bands , so as to give to the spectrum of the gas the appearance of a fluted pillar .
The bands in the spectra of a Orionis , P Pegasi , and some others probably arise in this way , and perhaps from some compound of hydrogen * .
The lines constituting such bands will be affected by differences of the force of gravity in the same way as other linles , and will therefore , if distributed with tolerable impartiality over the spectru m , cooperate with them in producing that tendency towards a ruddy hue which belongs to stars that exercise a feeble attraction at their surfaces .
It may be noted that in none of the figures which Mr. Huggins has given of the spectra of solitary stars with shaded bands , do they seem crowded abnormally over the yellow , orange , and red , but rather the reverse .
86 .
*We are now in a position to appreciate the significance of the phenomenia which the spectral examination of stars has brought to light .
We can easily see why in the class of bluish-white stars of which Sirius and a Lyrme are types , stars at whose surfaces the force of gravity is greater than on otur sun , " the dark lines they presenit in great number are all , with one exception , very thin and faint , and too feeble to modify the original whiteness of the light , " and why " the one exception consists of four very strong single lines , one line corresponding to Fraunhofer 's C , one to F , and another near G"t .
There can be little doubt that the multitude of faint lines will prove to be due almost exclusively to iron and the substances near it in vapouir-denisity , such as calcium , clirdmnium , manganese , nickel , and cobalt , with of course sodium and magnesium .
These , with the exception of sodiium and magnesium , can produce only linies which are faint through the whole extent of the spectrum , sinice when attracted downl with so much force as they are by the stars they canniot exist beyond regions of elevated temperature .
And substances a little higher ia .
vapour-density will be ulnable to endure even the chill of the photosphere , and therefore shrink within it .
The violet and indigo rays being , in these stars not subclued by lines in the same way as they are in the suni , gives to the whiteness of the stars a somewhat coloured tilnge in eyes , like ours , accustomed to adjudge the sun 's light to be white .
87 .
On the other hand , Aldebaran is a good sample of a star which exerts less attraction at his surface than the sun , but which in other respects differs little from him .
All the gases which cause solar lines can rise in the atmosphere of Aldebaran to colder heights than they can on the suin , and , as a consequence , they encroach more upon the violet end of his spectrum , and thus give to his light its rose-like tint .
Another consequence is , that substances present themselves in the star 's outer atmosphere with vapour-densities so high that the sun 's superior attraction keeps them imprisoned within his photosphere .
Mercury , mass of molecules 100 ; antimony , 122 ( ?
) ; tellurium , 129 ; bismuth* ' , 210 ( ?
) .
88 .
All the foregoing appearances present themselves in ciOrionis , which is therefore also a star on which the force of gravity is less than on the suin .
They are found in a Orionis with the addition of a spectrum of the first order , one of whose bands has been observed to fluctuate in distinctness .
We have reason to suspect , therefore , that the changes of brightness of this star , which is slightly variable , arise from some cause which alters periodically the temperature of the upper layer of that gas in its atmosphere from which the spectrum of the first order comnes .
Section HI.-Qf Multiple Systemst .
89 .
Hitherto we have considered only the case of stars uninfluenlced by one another .
If , however , two stars should be brought by their proper motions very close , one of three things would happen .
Either they would pass quite clear of one another , in which case they would recede to the same immensity of distance asunder from which they had come ; or they would become so entangled with one aniother as to emerge from the frightful conflagration which would ensue as one star ; or , thirdly , they would tbrush against one another , but not to the extent of preventing the stars from getting clear again .
It is this last cause which we muust now closely examine .
After the stars disengage themselves they will be found moving in new orbits , which , if their motions before contact had been parabolic , will become elliptic .
They will therefore return againi and again , and at each perilhelion passage will become engaged .
If we take into account only the tangential resistance which the atmosphere of each presents to the motioni of the other , we shall findl that the mean distance of the stars would he reduced .
If the resistance acted only at the apse of the orbit , the diminution of the meani distance would be effected by a shorteniino of the aphelion distance exclusively , the perihelioa distance remaining ulnaltered .
But since the resistance is not confined to this spot , but acts also for some space oil either side of it , the perihelion distance will at each passage undergo a slight decrease , which would inevitably cause the stars in the end to fall inlto one another , if the tanlgential resistance were the only force disturbing the orbits .
But there will be normal forces also .
The resistance to which each star is subjected in passing through the atmosphere of the other is a force neither directed through its centre , nor parallel to the tarngent of its orbit , sinee an atmosphere is not a thing of uniform denlsity .
Since these forces are not parallel to the tangents of the orbits , they will produce normal components , which will be directed outwards ; and sinice they are not directed through the centres of the stars , they will cause the stars to rotate , and these motionis of rotation , which will take place in the same direction in which the stars are revolving in their orbits , will in the subsequent perihelioni passages cause each star to sweep the atmosphere that opposes it downwards towards the other star wnile bursting through it .
It will accordingly itself suffer an equal reaction , which will be arnother force normal to its orbit and directed outwards .
Suich forces will lengtheni the perihelion distance , while they leave the mean distance undisturbed* .
Accordingly the combined where / 3 is the perihelioni distance , and the other letters have their usual significations .
A tangential resistance acting at any point of the orbit diminiishes v , and therefore by equation ( 1 ) diminishes a , the mean distanice .
To find its effect on G , the perihelion distaince , transform the second equation by putting -pG x 1 ) ; ... ... ... ... ... ... ... ... ... ... e ... ..6 ... .v..v vt t0 00 * .
( 2 ) whence , neglecting the higher powers of xr , since we only seek the effect of a reslstance acting in the neighbourhood of the perihelion where x is small , ' .
( .
1 ) ... ... ... ... ... ... ... .(3 ) p r , From equation ( 3 ) it appears that if v is diminished while p and r continue unchalnged , x must increase , and therefore by equation ( 2 ) / , or the perihelion distance , is reduced .
; This appears from the foregoing equations by supposing p to receive an increment , while v and r remnain unchanged .
Equation ( 1 ) is not disturbed ; in other words , the mnean distance is unaffected .
Equation ( 3 ) shows that x becomes less ; and equation ( 2 ) that / 3 , or the perihelion distance , is increased both by the increase of p and the diminution of x. The reverse effect upon 3 is produced by a decrease of p. Nowp is increased by the normal forces from the time the stars touich up to the moment of the perihelion passage , and decreased during the second half of the transit .
Accordingly 3 , the perihelion distance , is first increased and then diminished .
If the stars behaved to one another like perfectly elastic bodies , these chanlges would be equal , and would cancel one aniother .
But at each transit vis viva is converted into heat , in other words the stars do not behave like perfectly elastic bodies , and the mechanical forces elicited during the seconid half of the transit are feebler than those during the first .
Hence there will on the whole be any increase of the perihelion distance .
effect of both forces will be at each revoluition to shorteln the ellipses in which the stars move , and at the same time to augment or reduce the perihlelioni distance , according as the effect of the normal or tangential compolnent of the resistalnce preponderates .
If the normal force carry the day , the stars will at successive passages gradually work themselves clear of one another , a tesult which may be very much promoted by the behaviour of the atmospheres .
90 .
If what I here venture to offer as a surmise with respect to the proximate cause of stellar heat and the origin of double stars , is what really took place , we must conclude the sky to be peopled with countless hosts of dark bodies so numerous , that those which have met with such collisions as to render them now visibly incandescent , must be in comparison few indeed .
In the majority of those cases in which adequate collisions have taken place , the two stars must have emerged from the catastrophe , moulded into one , dilated by the conflagration to an enormous size* , and rotating .
Occasionally , however , the circumstalnces of the collision must have favoured the disentanglement of the two stars from one another by a predominating influence in these cases of the normal force acting in the way that has been traced in the last paragraph .
Wherever this happens , there is a prospect that a double star may form .
The heat into which much of the previous vis viva of the two components has been converted will dilate both to an immense size , and thus enable the two stars gradually in successive perihelion passages to climb , as it were , to the great distance asunider , which we find in the few cases in which the final perihelion distanice can be rudely estimated , a length comparable with the intervals between the more renmote planets and the sun .
While this is going on , the ellipticity of the orbits is at each revolution decreasing ; but if the stars suicceed in getting nearly clear of one another 's atmospheres before the whole ellipticity is exhausted , the atmospheres will begini to shrink in the intervals between two perihelion passages more than they expand when the atmospheres get engaged , and will thus complete the separation of the two stars .
When once this has taken place , a double star is permanently established .
91 .
It is a striking conifirmation of this view to find that the astonishing phenomena witnessed last year t in T Coronoe were precisely what we should expect to arise towards the end of the process which has been described .
The stars having been intensely heated by previous perihelion passages , and having begun to shrink , would , at ordinary times , present a spectrumll subdued by an abundance of very dark lines ; but immediately after one of the last occasions upon which their atmospheres brush against one another , the ouiter constituent of their atmospheres , and the outer constituent alone , would be raised by the friction to brilliant incandescence , which would reveal itself by the temporary substitution of four intensely bright for foutr dark hydrogen lines in a spectrum which everywhere else continues to be filled with dark lines .
And , moreover , these dark lines would for a while be renidered faint by the fierce heat radiated upon the outer parts of the atmosphere of each star by its coimipanion * .
It will be a matter of great interest to watch this star when sufficient time shall have elapsed to give a hope of seeing it double .
92 .
When a body of moderate dimensionis enters the atmosphere of a great star , the resistance to which it is subjected will be very nearly the same per square metre over the whole of its front surface ; but if it be of sufficient size to occupy a considerable height of the atmosphere through which it passes , it will be exposed to much more resistance beneath than above ; and those conditions will have arisen which may terminate in a double star .
The cases mtust be rare in which two stars that clash together happen to be of nearly equal mass .
But when this does occur , the circumstances which are the most favourable to the formation of a double star have taken place .
This seems to account for the very remarkable proportion of double stars which have nearly equal constituents .
It would appear , too , that in this class we slhould expect to find those instances in which the perihelion distanlc is greatest , since it will be nearly the sum of the radii of the distended atmosphieres of the two stars .
93 .
If two stars which are unidergoing the process of formation into a double star , be of very unequal mass , the smaller one will be stripped at each perihelion passage of some of its atmosphere .
All those parts which by the friction are brought into a state of rest relatively to the parts of the atmosphere of the larger star with which they come in contact , will , after the stars have beein separated , settle down upon the larger star .
They will , before the next perihelion passage , be replaced upon the smaller star by a fresh supply of the same gases diffuLsing , upwards from beneath , and almiiost to the same height .
When the stars come together again , this , in its turn , will be stripped off ; and by a sufficienit repetition of the process at successive perihelion passages several of the lighter constituenits of the atmosphere of the smaller star will be transferred over to the larger .
Upon the larger star this will not ; have any visible effect ; the acquisition will not even swell his bulk perceptibly ** But upon his satellite the consequences will be very remarlcable .
Hydrogen was the first gas to go ; then , in order , sodium , magnesium , calcium , chromium , manganese , iron , If the process has gone far enough to distil away all of these gases in the free state , the spectru-m of the companion has been robbed of the principal lines found in solitary stars , to be replaced by an entirely new system emanating from substances of higher vapour-density , which , to judge from the spectra of the few coloured double stars that Mr. Huggins has succeeded in examining , are crowded abnormally over the scarlet , oranige , yellow , and part of the green , giving to the companions of double stars those blue , violet , or greenish tints which are met with nowhere else .
If the process be continued still further , more gases will be swept away , and the pbotosphere laid nearly bare ; as a consequence , the smaller star will appear white and nearly destitute of lines .
This may have furnished that numerous class of double stars of which the companions are small and white .
94 .
No double star can come forth unless unequal pressure has acted so effectually on the smaller constituent as to communicate to it a svift motion of rotation .
It is likely that cases may occur where the forces that accomplish this act with such inordinate strength that the cohesion of the smaller star is unable to withstand them , and there result two or more fragments spinning violently , and destined thenceforward to traverse slightly separate paths .
This seems a not improbable account of such a multiple system as y Andromedae .
95 .
Upon the primary the consequences of the same violence would probably be entirely different .
They wotuld compel him to rotate at a great speed , perhaps so rapidly as to fling off his own equatorial partst .
These would form rings about him of the elliptic section which was investigated by Laplace ; at least , they would assume this form if they consisted only of gas , or of gas with cloud dispersed through it which is constantly dissolving and reforming , so as to keep always in a state of minute division , -so long , in fact , as the gaseous pressure caused by any accidental conden* A mment 's consideration will make this plain .
In fact , if the quantities of all the gases in the earth 's atmosphere were doubled , it would add only 3-L miles , or , more exactly , 5534 metres to its height .
The restult , after all disturbance had quieted down , would be the same as if a denser stratum of air of this trifling thickness were slipped in between the present atmosphere and the ground .
To spectators from without , who would juidge of our atmosphere chiefly as one which reaches upwards to a distance of about 200 kilometres ( the height at which meteors begin to glow ) , the effect would be wholly insensible .
t This would be most likely to occur when the friction had acted chieflv on the superficial parts of the larger star , since under these circumstances a star inight be enormously dilated without any ' considerable inierease of its moment of gyration ; so that , caeteris paribus , such a star would rotate swifter than one whose bulk was due to the equal expansion of all parts .
Siriuis may have been an instance of such a star ( see footnote , p. 53 ) .
We have perhaps some reason , judging from the existing areolar momentum of the parts of the solar system , to suspect that it was in a considerable degree the case of ouir sun also .
sation in one part of the ring tends to disperse the gas which had accumumulated there and so restore the balance , with better effect than the slight .
lie superior attraction of the condensed knot caln disturb it .
The gases first cast off } will soon be replaced on the star by a fresh supply of the same kilnds diffusing upwards from below , to be in turn flirted off inlto the rings , if the star have retained sufficient rotation .
It would seem , then , that the rings must of ' necessity consist of exceedingly light materials .
These rings.will obviously move nearly in the same plane as the companion , or fragments of the companion , as the case may be .
96 .
Now , as has been explainied above , when the circumstances are such as favour the formation of a douible star , the perihelion distance of the relative orbit is , after every revolution , on the increase , and the eccentricity on the decrease .
If the t'wo stars miianage to get clear of one another before the eccentricity is worn out* , the process is complete , and a double star has come into being .
But it must ofteni happeni , and is especially likely t where the companiion is small , or has brolken up into a number of fragments , that after the perihelion distance has become very considerable , but before the stars are quiite clear of one another , the orbit will have degraded into a circular one .
If this happen to any fiagment of which the distance is at the time less thanthe radius of the distenided primary , the two bodies must fall together and become one .
But if the perihelionl distanice had attained a sufficient mag-nitude to place the fragment in one of the ring , s surrounding the primary , it will there play a very important part .
It will by its attraction collect this ring about itself , and thus become covered with an enormous atmosphere , encircled by which it will continue to spin vigorously in the direction in which it moves in its now nearly circular orbit .
If this rotation should be rapid enough , the new planet will itself throw off rings ; and if any of these should afterwards become colncentrated into satellites 4 , they will , like our1 moon , keep the same face always turned towards their primary .
All this seems in a very renmarkable degree to be what we see about us in the solar system .
be due to such a moderate change of temperature as , for instance , wotuld convert the vapour of water into ice ?
It should be borne in mind that if the earth was at any time sufficiently hot , the ocean must have them formed an atmosphere of steam so vast , that it may perhaps have even reached to a ring which afterwards became the moon .
Possibly the giants of our system ( Juipiter , Saturn , Uranus , and Neptune ) owe their small density to their great mass , by reason of which they retain enough of their pristine heat to be still clothed in immense aqueous atmospheres .
If these surmises should prove to have any foundation , water was probably the material of rings thrown off originally by the sun , and is therefore not improbably an ingredient of the atmosphere of those dilated stars which do not exhibit hydrogen lines .
( See footniote , p. 50 .
) POSTSCRIPT .
[ ( Continuation of the note on p. 26 .
) I have during the present summer often received the impression that I saw several other faint bright lines in other parts of the spectrum , of which the principal is a line which is coincident with or very close to Kirchhoff 's copper line of wave-length 52 23 .
It should be borne in mind that if suich bright lines exist , they are due to constituents of the solar atmosphere which are eminently transparent to these rays , either from being intrinsically so , or from the excessive tenuity of the gas .
Hence the gas adds in these rays , but only adds a little , to whatever bright .
ness may be transmitted through it from beyond .
It behaves like a faintish flame of very high temperature placed between the eye and a more conspicuous but less hot coal .
Hence , if the background be the spectrum of the umbra of a spot , the bright line should be afaint streak across it .
On the only occasioni on which I had an opportunity of examining the spectrum of a spot , one of the rays I suspect to be bright lines presented this appearance to my eye .
Mr. Lockyer and Mr. Huggins have observed that some dark lines appear broader in the spectrum of a spot than in the spectrum of ordinary solar light .
This is no doubt because the wings of these lines lose brightness which had before shone through them from beyond , and the duskier parts of them in consequence become dark enough to add to the breadth of the central black stripe .
Wings appear to be always ( except in the anomalous case of the iron line 49 61 , which demands a careful experimental scrutiny ) fainter than the central band .
This may arise in either of two ways , either , 10 , because the gas is so rare , or else the perturbations which occasion the wings so evanescent , that the wings are in a conisiderable degree transparent , and much light from the photosphere streams through them ; or 20 , because though opaque they come from a region hot enough to render them less dark than the central stripe .
It is in the case of wings of the former kind only that the appearance recorded by Messrs. Lockyer and Huggins will present itself .
Lines of which the wings are quite opaque ought , on the other hand , to appear narrowest when seen in the spectrum of the umbra of a spot , since the brighter parts of the wings would be them undistinguislhable from the faint background , which would therefore seem to encroach upon them.-September 1868 .
]
|
112350 | 3701662 | Second List of Nebulae and Clusters Observed at Bangalore with the Royal Society's Spectroscope | 58 | 60 | 1,868 | 17 | Proceedings of the Royal Society of London | John Herschel | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1868.0004 | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 96 | 1,507 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112350 | 10.1098/rspl.1868.0004 | http://www.jstor.org/stable/112350 | null | null | Astronomy | 34.609898 | Atomic Physics | 28.502466 | Astronomy | [
82.46131896972656,
6.648447513580322
] | I. " Second List of Nebulae and Clusters observed at Bangalore with the Royal Society 's Spectroscope ; " preceded by a Letter to Professor G. G. STOKES .
By Lieut. JOHN HERSCHEL , R.E. Communicated by Prof. STOKES .
Received July 20 , 1868 .
Bangalore , June 17,1868 .
MY DEAR SIR , -As it is now three weeks since I have been able to make any use of the Royal Society 's telescope &c. , owing to the setting in of the rainy season , and as circumstances oblige me shortly to move my quarters and start the instruments for the eclipse , it seems better to send all the observations I succeeded in getting since I last wrote up to the time of the change of weather .
I am sorry this second list is not a fuller one .
But the fact is , that now that the planetary nebule list is exhausted , and the more conspicuous nebulae , I find no small difficulty in seeing anything .
It is true that the globular clusters alone form a long list for examination , a considerable number of which may be visible with the spectroscope ; but as they seem to show continuous spectra without exception , the interest attaching to this class is considerably diminished .
I have still a long list of nebulae proper to examine ; but the proportion of these which exhibit monochromatic spectra seems very small-so small , indeed , that I cannot report a single new instance in this class .
There are some conspicuous ones which will present themselves later in the year , among which one or two may possibly be recognizable as gaseous ; but the majority , I may say the large majority , seem otherwise , and therefore difficult of positive identification .
It will be necessary to despatch the instruments along with my camp equipage &c. in a fortnight or three weeks , as the spot selected for a station of observation is upwards of 300 miles distant from Bangalore .
I cannot expect that the return journey will have been effected before the middle or end of September .
For the next three months , therefore , the nebulae must be allowed to pass unchallenged .
Whether I shall have the opportunity of continuing my search then , or not , must depend on circumstances which I cannot now foresee .
Should the Society see fit to allow the instrument to remain in my hands for a few months longer , I will at least undertake to prosecute the search during such intervals of leisure as my other duties may leave at my disposal .
But at present , perhaps , the question of the disposal of the instrument after the eclipse is not an urgent one .
The station selected for the eclipse observations is Jamkandi ( vnlg .
Jumkhundee ) , about midway between Belgaum and Sholapore .
The selection has been determined chiefly by the small rainfall of that district , and by the spontaneous offers of assistance of II .
H. the Chief of Jamkandi .
I have no great fears about the weather ; but of course one may be disappointed .
There is certainly a better chance there than at any point on the east coast .
Yours truly , J. HERSCHEL .
Nos. 2068 .
3642 .
These are all of the class globular clusters .
They are all described as very bright or bright , and most of them well 42 resolved .
Their spectra were recognized , without excep4270 .
> tion , as continuous , and that generally without difficulty ; 4270 .
but 2068 and 4211 were very faint in the spectroscope .
4275 .
42 The spectrum of 4307 was unusually bright , and was 42 visible from about D to about F. No further details ap4307 .
| pear necessary about these .
4311. .
The following " planetary nebulae " have been recognized as showing monochromatic spectra : No. 1843 .
Faint monochromatic light at D+2'22 ( May 9th ) .
No. 2076 .
Faint monochromatic light , distinct , but not measured ( May 10th ) .
No. 1565 .
Faint monochromatic light , spectrum not seen until the sixth time of examination ( May 14th ) .
No. 1801 .
Monochromatic spectrum suspected only ( May 16th ) .
No. 3229 .
" Very bright ; round ; barely resolvable .
" Spectrum clearly continuous .
No. 3606 .
" Very remarkable ; very bright ; very large .
" Continuous spectrum distinctly .
No. 4189 .
" Bright ; pretty large ; partially resolved .
" Continued spectrum ( May 16th ) .
No. 4421 .
" Bright ; small ; well resolved .
" Continuous spectrum seen pretty easily- ?
very bright ; pretty large ( May 18th ) .
No other nebulae have been recognized ( since the previous report ) as having positively either monochromatic light or continuous spectra ; but the following list shows those which are believed to be continuous .
No. 3227 .
" Very bright ; large .
" No. 3397 .
" Very bright ; pretty small .
" No. 3477 .
" Very bright ; small ; round ; a star of the 10th magnitude following .
" No. 3504 .
" Very bright ; pretty small ; round .
" No. 3706 .
" Remarkable ; very bright ; very large .
" No. 2341 .
" Bright ; pretty large .
" No. 2586 .
" Bright ; pretty large ; barely resolvable .
" No. 3214 .
" Bright ; pretty large .
" 59 1868 .
] The evidence in the case of these is purely negative .
They have been brought on the slit with sufficient precision to make it in each case almost a certainty , taking into consideration their apparent brightness , that had their light been monochromatic in the sense in which other similar nebulae are so , it must have been recognized as such ; whereas , if dispersed , analogy would forbid any expectation of detecting the feeble continuous spectrum .
In each case I have satisfied myself that the inference was a iegimate one before recording it , both by testing the focal adjustment on a neighbouring star and by repeating ( if necessary ) the adjustment in respect of direction , until the case appeared a hopeless one .
Some instances , in which the presumption was not so strong as to seem to justify the inference , are omitted from this list .
Several nebuhle , the measurements of whose spectra were given in my previous list , were .
reexamined .
I am rather inclined to believe that the position of the principal light is not quite constant for all .
The newer and more careful measurements certainly throw doubts upon some of the earlier ones .
Nevertheless I have reason to believe that the discordances are not wholly due to inaccurate determination .
But on this and other points I hope to be able to write more fully on a future occasion , when a larger number have been remeasured .
The following were reexamined .
No. 4066 .
Very bright spectrum ; 3 lines certainly ; faint continuous spectrum suspected .
No. 4510 .
Very bright spectrum ; 2 lines only seen , both hazy ; comparatively distinct continuous spectrum of some length on both sides of the principal line .
No. 4390 .
Seen easily in a bright field ; 3rd line seen certainly .
No. 4361 .
Very large ; 2 lines only ; ill defined ; decided continuous spectrum at the brightest point ( not stellar ) .
P.S.-I have throughout used the word " monochromatic " in preference to " linear " intentionally , because , though not strictly correct , it appears more so than the latter .
Unless a cylindrical lens is used , or unless the object examined is so great as to be partially stopped out by the slit ( generally a very wide one ) , the term " linear " seems purely conventional .
I have reason to believe that some of my earlier measures were erroneous , partly through not realizing the " play , " so to speak , of the small image within a wide slit , the linear character being illusory .
The term has become so intimately associated with spectral appearances , that one is apt to forget how completely mechanical , and therefore conventional a characteristic of the quality of light is expressed by it ; Thus I find that , in more than one instance , expectation is entertained of possible bright " lines " being seen during the coming eclipse , without the intervention of a slit , as though this were an inherent quality in light itself .
|
112351 | 3701662 | On the Lightning Spectrum | 61 | 62 | 1,868 | 17 | Proceedings of the Royal Society of London | John Herschel | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1868.0005 | null | proceedings | 1,860 | 1,850 | 1,800 | 2 | 31 | 743 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112351 | 10.1098/rspl.1868.0005 | http://www.jstor.org/stable/112351 | null | null | Optics | 43.464199 | Atomic Physics | 31.275713 | Optics | [
19.369556427001953,
-35.199790954589844
] | II .
" On the Lightning Spectrum .
" By Lieut. JOHN HERSC-EL , R.E. Communicated by Prof. STOKES .
Received August 8 , 1868 .
I have had two or three opportunities of seeing this spectrum to advantage of late .
The storms at the period of the setting in of the south-west monsoon here are very frequent , and supply for a time almost incessant flashes , many of which are of course very brilliant .
The first time I examined the light in the spectroscope I had no idea of measuring , but was content to realize the principal facts of a continuous spectrum crossed by bright lines ; but subsequently I made several attempts ( with some success ) to obtain measures .
That I was unable to do more in this line is due partly to the difficulty of utilizing the short-lived appearance , partly to that fascination of waiting for " one more " bright flash to verify the intersection , which can only be thoroughly appreciated by the aid of a similar experience .
The principal features of the spectrum are a more or less bright continuous spectrum crossed by numerous bright lines , so numerous indeed as to perplex one as to their identity .
This perplexity is increased by the constantly changing appearance due to a variable illuminating power .
This variable character of the appearances is unquestionably the peculiar feature of the spectrum .
It is not that the whole spectrum varies in brightness in the same degree , but that the relative intensities are variable , not only among the various lines , but between these and the continuous spectrum .
The latter is sometimes very brilliant ; and when that is the case , the red portion is very striking , though in general the spectrum seems to end ab .
ruptly at D +-034 ( E-=D+ 1'38 , Kirchhoff 's 120 7=D+0'55 ) .
There is one principal line which I found equal to D+ 2'20 as the result of five independent measures .
The probable error of this value is about +'02 .
The general mean of all my measures of the principal nebular line ( obtained from twelve different nebule ) is 2 18 , with a probable error of about + -02 .
I have therefore very little doubt that these are the same , viz. the nitrogen line identified in the case of nebule by Mr. Huggins .
This line in the lightning spectrum is narrow and sharply defined , and is conspicuously the brightest , except as noted below .
The next in prominence is situated about D+ 3-58 ( F=D + 2'73 , Kirchhoff 's 2325 =D+3 50 ) .
It is broader and less vivid , and not so well defined at the edges .
There are several other conspicuous lines , but none comparable to the first .
I noticed a sharp line in the red , but did not get a measure .
I said that at D +0'34 the continuous spectrum ends abruptly .
A faint continuation is , however , seen frequently in bright flashes , very bright ones bringing out a brilliant red end crossed by a bright line .
The whole of the ordinary spectrum seems green and blue , or rather greenish blue ; but as the usual prismatic order of colours is recognizable in bright flashes , it is to be inferred that the region from E to F is so much 61 brighter as to give the character in question .
What strikes one most , however , is the varying relative brightness of the continuous and linear spectra ; sometimes the lines are scarcely seen , and sometimes very little else is seen .
This may be nothing more than an illusion ; but in the absence of any certainty that it is so , the impression left on the mind is worth recording .
The difficulty of discriminating between the many less prominent lines is immensely increased by the momentary character of the phenomenon .
Before the mind has selected an individual , the feeble impression on the retina has vanished ; and before another flash succeeds , the memory of the half-formed choice has vanished with it , and there is nothing on which to found a selection .
Otherwise it would be easy enough to measure many more lines .
|
112352 | 3701662 | Products of the Destructive Distillation of the Sulphobenzolates. No. II | 62 | 67 | 1,868 | 17 | Proceedings of the Royal Society of London | John Stenhouse | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1868.0006 | null | proceedings | 1,860 | 1,850 | 1,800 | 6 | 136 | 2,213 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112352 | 10.1098/rspl.1868.0006 | http://www.jstor.org/stable/112352 | null | null | Chemistry 2 | 84.556124 | Chemistry 1 | 7.941606 | Chemistry | [
-39.297061920166016,
-51.87733459472656
] | III .
" Products of the Destructive Distillation of the Sulphobenzolates .
-NO .
II .
' By JOHN STENHOUSE , LL. D. , F.R.S. , &c. Received September 8 , 1868 .
In a paper published by rue in the Proceedings of the Royal Society , 1865 , I described the manner of preparing sulphobenzolate of sodium and the products of its destructive distillation in a copper retort , 'These were chiefly sulphide of phenyl and a crystalline substance , of which too small a quantity was obtained to enable me properly to examine it .
As I wished to procure these products in larger quantities , instead of employing small copper retorts , which were rapidly destroyed , I conducted the operation in tolerably large cast-iron ones heated in a gas-furnace , and found that they were not sensibly corroded even after a great number of distillations .
The quantity of sodium-salt decomposed in each distillation was about 200 grammes .
The oily products obtained by this process , after separation from the supernatant watery layer , were introduced into a copper retort having a bent glass tube luted into the lneck and redistilled , the retort being heated to redness towards the close of the operation .
In this way a considerable amount of impurity was removed .
The bright yellow-coloured oil was then rectified in a glass retorlt .
It began to boil at 80 ?
C. , and rose rapidly to 16 50 C. , between which and 1800 C. about one-fourth of the liquid came over .
The temperature then againi rose rapidly to 290 ' C. , and from 290 ?
to 300 ?
a large quantity of nearly pure sulphide of phenyl distilled .
The small quantity of dark-coloured residue in the retort was poured inlto a beaker , where it became semisolid on cooling from the deposition of the crystalline substance I have before mentioned * .
PIenyl-Mercaptan .
The portion boiling between 16 5 ' C. and 1800 C. , on being repeatedly rec* Proc. Roy .
Soc. vol. xiv .
p. 353 .
tified , gave a liquiid boiling constantly at 172§ 5 .
This was subjected to analysis with the following results : I. '5345 grm. oil gave 1'280 grm. carbonic anhydride and *265 grm. water .
Theory .
1 .
C-=72 ... .
65'45 65-33 11=6 ... .
545 5'51 S =32 ... .
29-10 110 100 00 The numbers obtained correspond very closely with the formula c , IH3 } S , phenyl-mercaptan .
When pure it is colourless , having an aromatic but soiriewhat alliaceous odour , although not at all offensive .
It has a high refractive index , and boils at 172 ?
'5 C. Insoluble in water , but readily miscible with alcohol , ether , and benzol .
It is readily oxidized , yielding bisulphide of phenyl .
This takes place even when exposed to the air in imperfectly closed vessels .
Vogt* has described an oil which he obtained by the action of zinc and dilute sulphuric acid on sulphobelizolic chloride , C. H , Cl S 02 , and calls benzyl-mercaptan , C6 Ho S. He says it boils at " about 1650 C. , and has an extremely offensive odour .
" Ottot , by the action of nascent hydrogen on sulphophenylenethylene , Cc0 HS 02 } , obtained phenyl:mercaptan , which he showed to be identical with Vogt 's benzyl-mercaptan , but the boiling-point is " between 1700 C. and 173 ?
C. " From the description givenl by Vogt and Otto , it is evident that the phenyl.mereaptan obtained by the destructive distillation of sulphobenzolate of sodium in an iron retort is identical with theirs , and that the offerssive odour ascribed to it by Vogt is due to some slight impurity , probably arising from the phosphoric chloride emaployed in the preparation of the sulphobenzolic chloride .
Phlenyl-mercaptide of lead.-Oii adding acetate of lead to an alcoholic solution of the mercaptan , a bright yellow crystalline precipitate was formed .
This when heated fused , and at a higher temperature was decomposed .
Phenyl-merca:ptide of copper was prepared in a similar manner , substituting acetate of copper for acetate of lead .
On exposure to the air in a moist state it became oxidized , forming cupric oxide and bisulphide of phenyl , C. H1 S , which may be extracted and crystallized from boiling spirit .
The compounds with mercury , chloride of mercury , and silver are identical with those described by Vogt .
Decowposition of Pitenyl-mnercaptide of Lead .
When dry phenyl-mercaptide of lead is heated to a temperature suipelrior to 2800 C. it is decomposed , an oil distils over , and plumbic suiphide is left in the retort .
This oil boils constantly at 292§ 5 C. , and correspond(Is in all its properties with plenylic sulpiide .
By oxidation it vielded a substance crystallizing in oblique prisms , and which was proved to be sulphdobenzolene .
The action of heat on the lead mercaptide is therefore as follows:2 CG IOI5 S= cC , EIa S Pb S Pbf C I-I5fm2~ This decomposition is especially interesting , as it proves the body obtained by the destructive distillation of the siliphoberizolates to be the truie phenylic sulphide .
Bisulphidde of Pfeenty .
When the pure mercaptan was mnixed with about any equal blulk of coilcentrated suilphuric acid , the latter acquired a dirty purple coloui ' , and after the lapse of some time , with occasional agitatiou , became hot and gave off sulplhuron-s anhydride .
When cold the upper layer solidified to a mass of crystals , which , on being separated from the acid , washed with water , and crystallized several times from spirit , gave a white crystallinie substance .
It was dried in vacuo and analyzed .
I. *308 grm. substaniee gave 745 grm. carbonic alnhydride and * 133 grm. water .
Theory .
1 .
C6 =72 ... .
6605 ... .
65-98 I5= 5 ... .
4 59 ... .
480 S =32 ... .
29 36 109 10000 The analysis correspolnds to the formula Cc II5 S , 6isulplhide ofp henyl .
It is insoluble in water , soluble in alcohol , very soluble in ether , beiuzol , and bisulphide of carbon , melts at 6P C. ( Vog , t* g , ives 60 ' C. as the melting-poilnt of his bisulphide of benzyl ) .
It is again reduced to the mercaptan by zinc and dilute sulphuric acid , or better , by digestion with hydriodic acid and amorphous phosphorus .
As but traces of pheniyl-mercaptaii were obtained on decomposing the sulphobenzolate of sodiulmi in a copper retort , while a considerable pportion of the distillate consisted of the mereaptan when an iron one was used , I was induced to make some experimeents in order to see whether it was the copper which caused this difference .
This I ascertainied to be the case by distilling sulphobenzolate of sodium mi2ixed with copper cuttings in any iron retort , when the proportion of the mercaptan to the sulpllide was comparatively small , and the surface of the copper was converted into cupric sulphide .
Graniulated zinc produced a similar result .
Phenylene Sulphide .
The dark-coloured residue in the retort which did not come over at 3000 C. was distilled from a copper retort having a bent glass tube luted into it .
The orange-coloured distillate , on standing a few days , deposited a considerable quantity of large transparent plates .
These were drained as much as possible , and freed from adhering oil by pressure between paper .
The partly purified crystals were extracted with hot spirit to remove the bisulphide of phenyl and other impurities , and then crystallized from benzol or bisulphide of carbon .
A crystallization from spirit rendered them quite pure .
I. 243 grin .
gave *592 carbonic anhydride and.086 grm. water .
TI .
-221 grin .
gave '539 carbonic anhydride and *076 grm. water .
III .
*301 grm. gave -652 baric sulphate .
Theory .
I. II .
1IT .
Mean .
C6 = 72. .
66 67 66-45 66-53 ... .
6649 H14 = 4. .
370 3-93 3 82 ... .
3 87 S= 32. .
2963 ... ... . .
29171 29'71 108 100-00 The analyses of this substance lead to the formula C. 14 S , 8ulp1 de of pphenylene .
It crystallized in long lustrous prisms , which are quite transparent and colourless .
Is insoluble in water , slightly soluble in cold alcohol ( about 400 par-ts ) , but more so in hot .
It is far more soluble in benzol and bisulpbide of carbon , from the latter of which it may be obtained in fine crystals , sometimes half an inch or more in length .
It melts at 1590 C. and solidifies at 1530 C. It dissolves in concentrated sulphuric acid , forming a solution of a magniificent purple colour , and which when largely diluted with the concentrated acid appears purplish red .
On the addition of water the colour disappears , and a crystalline precipitate is produiced , apparently the unaltered phenylene sulphide .
With concentrated nitric acid a reaction takes place , red fumes are evolved , and a crystalline substance produced , probably a nitro-substitution compound .
This I have at present under investigation .
Sulphobromide of Phenylene .
When crystals of the pheniylene sulphide are exposed to bromine-vapour they combine with it and turn black , forming sulphobromide of plhenylene .
The best method , however , to obtain this pure , is to add perfectly dry brominie in slight excess to a cold saturated solution of sulphide of phenylene in dry bisulphide of carboni , when the compound is precipitated in the form of minute black prisms .
These are immediately collected , washed with cold dry carbonic disulphide , pressed , and the bisulphide of carbon removed by placing them under the receiver of an air-puimp , rapidly exbausting the air , and allowing it to reeniter several times .
It is theu weighed and treated with excess of pure solution of sulphurous acid , to convert the combined bromine into hydrobromic acid .
This is determined as bromide of silver .
By this miethod the following result was obtained : 821 grnm .
substance gave 1 154 grm. argentic bromide .
This gives 5981 per cent. combined bromine .
The formula CH SBr2 requires 59 70 per cent. bromine .
This substance is therefore analogous to the corresponding ethylene compound discovered by Carus * .
T'he sulphobromide crystallizes in black prisms , which slowly give off bromine oln exposure to dry air , and are rapidly decomposed by moisture with evolution of hydrobroinic acid .
They " are tolerably soluble in carbonic disulphide and tetrachloride .
Phenyl-hyposulphurous Acid .
Amongst the reactions which phenylic sulphide gave with various reagents t , that with sulphuric acid was particularly interesting .
On treating pure sulphide of pheniyl with an equal bulk of conicenitrated sulphuric acid , the oil changed first to a finie red colour , and as the heat increased it became purple , and ultimately dissolved , giving of traces of sulphurous acid .
The comnpound thus produced , when cold , was seinifluid , and gradually absorbed moisture from the air , becoming a semisolid crystalline paste .
This was dissolved in a large quantity of boiling water , neutralized with pure baric carbonate , filtered from the insoluble sulphate , and the solution of phenylbyposulphite of barium evaporated until a pellicle formed on the surface , and then allowed to cool .
The crusts which come out consist of mnicroscopic crystals .
These , after one or two recrystallizationis from boiling water , were dried at 100 and submitted to analysis .
*419 grin .
substance gave '1 7o grm. barle sulphate..334 grmi substance gave '141 grm. baric sulphate .
*320 grm. substance gave *312 grm. carbonic anihydride and 075 grm. water .
Theory .
1 .
i. III .
C= 72 co 2613. .
26161 1177 .
2-54 ... . .
2 61 Ba = 68-5 , , 24-85 24-56 24-82 S2 = 64. .
23'24 04 = 64 .
23-24 275'5 10000 These analyses agree tolerably well with the formula C0 11 Ba S2 03 120 , which I propose to call baric phenylbhyposulphite .
I have prepared the copper salt , which likewise form s crystalline crusts but neither the calcium nor sodium alt crystallizes as well as the barium .
Arn der Cbheim tid Pharmn .
vol , cxxiv p , 113 .
t Prcce .
Roy .
Soc , vol. x ; N p. 354 .
It is not improbable that ethylic and metliylic sulphides , &c. , when treated with concenatrated sulphuric acid , would formcorresponding compounds .
I cannot colnclude this paper without acknowledging the very efficient aid I have received from iny assistanit , Mr. Charles E. Groves , in the preceding investigation .
|
112353 | 3701662 | Compounds Isomeric with the Sulphocyanic Ethers.--II. Homologues and Analogues of Ethylic Mustard-Oil | 67 | 73 | 1,868 | 17 | Proceedings of the Royal Society of London | A. W. Hofmann | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1868.0007 | null | proceedings | 1,860 | 1,850 | 1,800 | 7 | 151 | 3,098 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112353 | 10.1098/rspl.1868.0007 | http://www.jstor.org/stable/112353 | null | null | Chemistry 2 | 93.630413 | Biography | 2.850107 | Chemistry | [
-40.87040328979492,
-61.12792205810547
] | IV .
" Compounds Isomeric with the Sulphocyanic Ethers.-II .
Homologues and Analogues of Ethylic Mustard-oil .
" By A. W. HOrMANN , Ph. D. , Mi .
D. , LLoD .
Received September 11 , 1868 .
In a former Note submitted to the Royal Society some months ago , I have sketched a series of compounds isomeric with the well-known sulphocyanic ethers ; today I shall endeavour to delineate more in detail the bodies the existence of which I then pointed out .
In order to prepare these substances , which , from their analogy with the essential oil of mustard-seed , I have designated by the name of mustard-oils , the monamines were in the first place treated with bisulphide of carbon ; the alcohol-sulphocarbonates of the monamines thus formed were then submitted to the action of heat and converted , by the loss of 1 molecule of sulphuretted hydrogen , into sulphuretted ureas , which were finally deprived of 1 molecule of monamine by means of anhydrous phosphoric acid .
Circuitous as this process may appear , it has the merit of being a general one , furnishing , in fact , the mustard-oils both of the fatty and aromatic series .
When working with fatty substances , however , the method may be very considerably curtailed .
Let it be ethylic mustardoil that is to be prepared .
Even on the threshhold of my inquiry I had hoped to see ethyl-sulphocarbamic acid split up into sulphuretted hydrogen and ethylic mustard-oil ; experiment , however , proved that the metamorphosis assumes another form , the acid yielding as products of decomposition its two components , ethylamine and bisulphide of carbon .
( C 8)"(C2 I , )N , I } C , }N +C 82 But a transformation which the free acid refuses , the metallic ethylsulphocarbamates undergo without difficulty , more especially in the presence of an excess of the metallic solution , a metallic sulphide being formed .
( C y ' ( C(2 T-15 ) N Of I sc(C:)ff N+ i S. On adding , for instance , nitrate of silver to a solution of ethyl-sulphocarbarnate of ethylamine , such as is produced by the action of bisulphide of carbon upon ethylamine , a white precipitate of ethyl-sulphocarbamate of silver is formed , nitrate of ethylamine passing into solution .
After some time , * Proceedings , vol. xvi p. 254 .
E however , this precipitate blackens , even at the common temperature , more rapidly on heating , with formation of sulphide of silver .
Simultaneously the odour of ethylic mustard-oil becomes perceptible ; and if the liquid be heated to ebullition , this oil distils in large quantity with the vapour of water .
The disengagement of sulphuretted hydrogen , which is observed at the same time , belongs to a secondary reaction , the unstable hydrosulphide of silver ( which is formed in the first instance ) splitting up into sulphide of silver and sulphuretted hydrogen .
In this experiment no excess of silver should be used .
Ethyl mustardoil , more especially upon protracted ebullition , exchanges its sulphur for oxygen , thus giving rise to the formation of cyanate of ethyl , easily recognizable by its fearful odour .
Ultimately this ether is entirely decomposed into carbonic acid and ethylamine ; after some time the solution contains nothing but nitrate of ethylamine .
Most of the metallic ethyl-sulphocarbamates , more especially the copper and mercury salts , behave exactly like the silver compound .
I have almost invariably employed mercuric chloride for preparing ethyl-mustard-oil .
In this case the hydrochlorate of ethylamine which is produced unites with the excess of corrosive sublimate to form an insoluble compound .
Accordingly the ethylamine , which in this reaction is separated as salt , exists partly in solution , partly in the precipitate ; it is easily recovered by treating with caustic soda the residue which is left after the mustard-oil has been obtained by distillation .
When working with pure ethylamine , one half of the base may thus be regenerated for a new operation .
But it would be useless to employ pure ethylamine for this purpose .
The crude mixture of bases , which is obtained by allowing alcoholic ammonia to stand for some time with iodide of ethyl and distilling the iodides thus formed with an alkali , is very well adapted for this operation .
This mixture , as is well known , contains , together with ammonia , the primary , secondary , and tertiary monamines of the ethyl-series .
I have satisfied myself , in the first place , that diethylamine is just as easily converted into ethylic mustard-oil as ethylamine .
The experiment was made with absolutely pure diethylamine prepared by means of diethyloxamic ether .
Bisulphide of carbon , more especially in alcoholic solution , acts with great energy upon diethylamine , diethyl-sulphocarbamate of diethylamine being formed , which , when treated by a metallic salt , furnishes a metallic diethyl-sulphocarbamate together with a salt of diethylamine .
On ebullition , the former is converted into ethylic mustard-oil ; but instead of the metallic hydrosulphide generated in the analogous metamorphosis of ethylamine , in this case a mercaptide is formed .
( C S)"(C21 ) N , ( C H , ) } C , C S ' N C , 11 }I should not leave unmentioned , however , that the formation of mercaptide is still to be further proved by direct experiment .
On working with mercuric chloride , the precipitate which remains after the ethylic mustard-oil is separated by distillation , neither dissolves in boiling water nor in boiling alcohol .
If this precipitate were pure mercaptide of mercury , it should be crystallizable from boiling alcohol .
Probably it is a double compound of mercaptide and chloride ; at all events , I have established by experiment that mercaptide and chloride of mercury unite to form a compound perfectly insoluble both in water and alcohol , even on boiling .
Triethylamine also unites with bisulphide of carbon ; but this compound , as might have been expected , yields no longer any mustard-oil .
Ultimately , as regards the ammonia , which invariably occurs in the crude mixture of the ethyl-bases , its presence rather increases than diminishes the quantity of mustard-oil which is formed .
This ammonia remains in the residue in the form of a salt , together with salts of ethylamine , diethylamine , and triethylamine ; and a corresponding quantity of the primary and secondary ethyl-bases is converted into mustard-oil , the yield of which may thus be very considerably augmented .
The mercuric salts also attack ethylic mustard-oil , although much less easily and rapidly than nitrate of silver .
A large excess of chloride of mercury , however , should be avoided .
If the ethylamine be prepared from iodide of ethyl , it is convenient to employ the mercury salt and the mixture of bases in such proportions that 1 molecule of mercuric chloride reacts upon the bases generated by means of 2 molecules of iodide of ethyl .
In an experiment carried out upon rather a large scale a quantity of ethylic mustard-oil was obtained amounting to from 60 to 70 per cent. of the theoretical proportion which might have been expected from the weight of iodide of ethyl employed .
Ethylic Mustard-oil .
As to the physical properties of ethylic mustard-oil , I have not to add anything to what I have formerly stated , except a determination of the gas-volumle weight , which was taken in the vacuum of the barometer at the temperature of 185 ?
( in the vapour of boiling aniline ) .
Referred to hydrogen .
Referred to air .
Theory .
Experiment .
Theory .
Experiment .
Gas-volume weight ... .
43-5 43'75 3-02 3-03 When operating with the isomeric sulphocyanide of ethyl , the following numbers were obtained : Referred to hydrogen .
Referred to air .
Theory .
Experiment .
Theory .
Experiment .
Gas-volume weight of sulphocyanide } of ethyl ( determined in the vapour 43-5 42-84 3-02 2-98 of boiling water ) ... ... ... .
J of Ethylic Mustard-oil .
69 1868 .
] Met hylic Mustard-oil .
I formerly obtained the methyl-compound as an oily liquid boiling at 120 ?
, and powerfully smelling of horseradish .
When a somewhat larger quantity of this body was prepared according to the process above described , the liquid , after distillation with the vapour of water , solidified to a splendid crystalline body .
Composition , 02 H3 N S(C St N. Boiling-point 1190 ; fusing-point 34 ?
; solidifying-point 26 ? .
Referred to hydrogen .
Referred to air .
Theory .
Experiment .
Theory .
Experiment .
Gas-volume weight of methylic 1 mustard-oil ( determined in the 36 ' 5 37-89 2-52 2-61 vapour of boiling water). .
J Amylic Mustard-oil .
I have also prepared the amyl-compound on a larger scale by a slight modification of the process above described .
Instead of separating the compound from the mercury precipitate obtained in the dilute alcoholic solution at once by distillation , it is advisable to return the vapours , condensed by a cooler , for some time ito the boiling mixture .
When the reaction is complete , the sulphide of mercury is filtered off , the amylic mustard-oil precipitated by water , dried over chloride of calcium , and ultimately purified by distillation .
The odour of the compound is analogous to those of the methyland ethyl-body , but less pronounced .
Composition , C , H , N S= S1 , t S. Boiling-point 183 ?
to 184 ? .
Referred to hydrogen .
Referred to air .
Theory .
Experiment .
Theory .
Experiment .
Gas-volume weight of amylic mustard-oil ( determinied in the va64-5 63-42 4-48 4-40 pour of boiling aniline ) ... ... Tolylic luszstard-oil .
As has already been pointed out , the new process cannot be used for preparing the mustard-oils of the aromatic series , at all events in the narrower sense of the word .
I may mention , however , that tolylic mustard-oil may be readily obtained by the process which I had formerly used for producing the corresponding compound of the phenyl-series .
The ditolylsulphocarbamide required for this purpose is known ; it was examined some years ago by MA .
Sell .
If this body be distilled with anhydrous phosphoric acid , aromatic vapours are evolved which may be condensed to a yellowish oil rapidly assuming the crystalline form .
The product of distillation 70 Rtecess , generally retains a minute quantity of ditolyl-sulphocarbamide , which may be separated by recrystallization from ether , tolylic mustard-oil being extremely , ditolyl-sulphocarbamide but slightly soluble in this liquid .
The mustard-oil of the tolyl-series readily crystallizes in beautiful white needles , attaining often the length of several centimetres ; they are easily soluble in alcohol , slightly so in water .
Tolylic mustard-oil possesses to an almost deceptive degree the odour of oil of aniseed .
Composition , C8 HI , NS =(C fI N. Boiling-point 237 ?
; fusing-point 26 ?
; solidifying-point 22 ? .
When gently heated with toluidine , tolylic mustard-oil is reconverted into ditolylsulphocarbamide .
With ammonia it forms sulphuretted monotolylurea .
Aniline gives rise to the mixed sulphuretted urea of the phenyl and tolyl-series , which is easily obtained in beautiful crystals .
Benzylic Mustard-oil .
Chemists are acquainted with a primary monamine isomeric with toluidine .
This is benzylamine , discovered by M. Mendius .
3ince the beautiful experiments of MM .
Fittig and Tollens have established the presence of the methyl-group in toluol , our views respecting the difference of constitution of the two isomeric monamines have acquired a solid foundation .
In toluidine the substitution of the primary ammonia fragment ( H2 N ) for hydrogen has taken place within the benzol nucleus ; in benzylamine , on the other hand , the substitution occurs in the methyl-group engrafted upon the benzol nucleus .
Benzylamine thus belongs , in a measure , to both the fatty and the aromatic series ; and the residue of ammonia , which in fact is exclusively affected during the formation of mustard-oils , is present in the fatty portion of the compound .
Under these circum stances it appeared rather probable that the base isomeric with toluidine would yield its mustard-oil by conversion into the bisulphide-of-carbon compound and distillation of the latter with perchloride of mercury .
Experiment has verified this anticipation .
Benzylamine dissolves in bisulphide of carbon with evolution of heat , a beautiful white crystalline compound being formed , which , when distilled with alcohol and mercuric chloride , yields a liquid of a penetrating odour .
On adding water to the alcoholic distillate , the mustard-oil separates in clear drops which are heavier than water .
Benzylic mustard-oil , c m , S= , af isomeric with tolylic mustard-oil , boils at about 243 ?
, a few degrees higher than the tolyl-compound .
The new body possesses in an eminent degree the odour of water-cresses .
The resemblance is so striking , that it becomes desirable to examine the essential oil of water-cresses .
I may here mention .
that menaphtylamine , the preparation and properties of which I have lately described to the Royal Society * , yields likewise a mustard-oil , if it be successively treated with bisulphide of carbon and mercuric chloride .
I have not , however , more minutely examined this compound .
All the mustard-oils here mentioned exhibit , more especially with reference to ammonia and its derivatives , the same reactive power which belongs to ethylic mustard-oil , more minutely described in my former communication , and by which the mustard-oil par excellence , the well-known allylcompound , has long fixed the interest of chemists .
Of the legion of urealike bodies which are here possible , I have prepared but few .
It may be stated that the sulphuretted methylic and amylic ureas , and also the sulphu. .
retted methylamylic and amyltolylic ureas vie with each other as to beauty and facility of crystallization .
I have not , however , examined more minutely these ammonia compounds , their study promising but very little scientific gain .
On the other hand , I have investigated with some care the metamorphoses of the mustard-oils , since their comparison with the corresponding transformations of the sulphocyanic ethers promised to elucidate the different construction of the two groups of bodies .
The results of these inquiries unequivocally confirm the view suggested by the formation of the two classes of compounds .
It is indeed only necessary to trace their origin in order to understand the nature of this difference .
We could not select better illustrations than the isomeric terms of the methyl-series .
Both bodies , methylic mustard-oil and sulphocyanide of methyl , are in the last instance derived from exactly the same compounds , viz. methylic alcohol , bisulphide of carbon , and ammonia .
Let the molecules of these three compounds unite with separation of 1 molecule of water and 1 molecule of sulphuretted hydrogen , and a body will be formed possessing the composition of both methylic mustard-oil and sulphocyanide of methyl .
CH O+C S2+H3 N=HO2 0+H2 +C2 H3 N S. Accordingly the nature of the body produced must depend upon the conditions ( it might be almost said upon the order ) in which the molecules of water and sulphuretted hydrogen are separated from the aggregate of atoms .
Conceived in its simplest form , the first step of the generation of methylic mustard-oil consists in the action of ammonia upon methylic alcohol , when methylamine is produced with separation of water .
C H14 0 +H3 N= H2 +C HI N. In a second phase of the process , methylamine is acted upon by bisulphide of carbon , the products being methylic mustard-oil and sulphuretted hydrogen .
CI N+C S2= H+C21N S. The reactions occur in the inverse order when sulphocyanide of methyl is produced .
Here the process commences with the reaction between bisulphide of carbon and ammonia , hydrosulphocyanic acid being formed with separation of sulphuretted hydrogen .
CS2+H13N=H,2S+CIHNS .
Hydrosulphocyanic acid and methylic alcohol , lastly , furnish water and sulphocyanide of methyl .
C HNS+-C H40=H1O2+C2HN S. This inverse order , in which the reactions succeed each other , gives a definite direction to our speculations as to the arrangement of the atoms within the molecules of the two compounds .
If bisulphide of carbon , S CS , in contact with methylamine , H3 CN -2 , is found to disengage sulphuretted hydrogen , we cannot doubt that the carbon-atom of the bisulphide , meeting , as it were , with its two freed attraction-units those liberated in the nitrogen atom , .
associates with this nitrogen-atom , and consequently that it must be by the nitrogen that the carbon of the methyl-group is chained to the carbon of the bisulphide .
On the other hand , if in hydrosulphocyanic acid we may conceive the hydrogen to be in union with the sul .
phur , we are , after this hydrogen has been converted into water by the hydroxyl of methylic alcohol , also justified in considering the sulphur-atom as the link of connexion between the two carbon-atoms of the compound , the attraction-unit , which has become available in the carbon-atom , being saturated by the free atomic power of the sulphur .
The relative position of the atoms il the molecules of the two compounds would thus be indicated by the following diagramMethylic mustard-oil .
Sulphocyanide of methyl .
HH H-C-r N=C=S , and H-Cs-C N ; or more concisely in the subjoined formula-S CNC If this conception be correct , it is obvious that whenever nitrogen and sulphur are found together in a molecule , this molecule must be capable of existing in two different forms , one corresponding to methylic mustardoil , the other to cyanide of methyl .
In a paper which I hope shortly to submit to the Royal Society , I propose to show how far this conception is supported by experiment .
1868 .
] 73
|
112354 | 3701662 | Account of Spectroscopic Observations of the Eclipse of the Sun, August 18, 1868 | 74 | 80 | 1,868 | 17 | Proceedings of the Royal Society of London | C. T. Haig | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1868.0008 | null | proceedings | 1,860 | 1,850 | 1,800 | 7 | 117 | 3,966 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112354 | 10.1098/rspl.1868.0008 | http://www.jstor.org/stable/112354 | null | null | Astronomy | 52.213896 | Optics | 18.990208 | Astronomy | [
83.0977554321289,
4.787115097045898
] | V. " Account of Spectroscopic Observations of the Eclipse of the Sun , August 18 , 1868 , in a letter addressed to the President of the Royal Society .
By Captain C. T. HAIG , R.E. Communicated by the President .
Received September 21 , 1868 .
Poonta , 24th August , 1868 .
MY DEAR SIR , -I hasten to send you an account of the observations I have fortunately been able to make at Beejapoor of the total eclipse on the 18th instant with one of the hand-spectroscopes sent out by the Royal Society in the care of Lieut. Herschel , R.E. , not waiting to let my report be forwarded by Colonel Walker , R.E. , my departmental superior , on account of the delay which would necessarily be caused thereby .
I may state at once that I observed the spectra of two red flames close to each other , and in their spectra two broad bright bands quite sharply defined , one rose-madder and the other light golden .
These spectra were soon lost in the spectrum of the moon 's edge just before emergence , which had also two well-defined bright bands ( one green and one indigo ) about a quarter the width of the bands in the spectra of the flames , this spectrum being again soon lost in the bright sunlight .
I will now proceed to give a somewhat detailed account of the observations , in which Captain Tanner , Bombay Staff Corps and of the Minar Survey ( who , on my earnest solicitation , accompanied me ) , and Mr. Kero Laxuman , Professor of Mathematics in the Deccan College , took part , and during which Mr. ilunter , Bombay Civil Service , and Dr. Kielhorn , Professor of Sanskrit in the Deccan College , were present as non-professional observers .
Our instrumental equipment consisted as follows:-Mr .
Kero Laxuman brought an ordinary pedestal-telescope of 2k-inch aperture and 36 inches focal length by Horne and Thornthwaite , which he temporarily mounted on a stand equatorially ; and he had a scale fitted inside a 60-power eyepiece , which , however , he was unfortunately not able to use , on account of a fall which his instrument sustained from being blown down by the high wind ; he therefore had to use another eyepiece of power 70 , not furnished with a scale .
He also had a pocket chronometer beating five times to two seconds , by Arnold and Dent .
Captain Tanner had an Everest theodolite by Troughton and Simms , having a remarkably good telescope , 1-7-inch aperture and 18 inches focal length , and an eyepiece of power 46 .
I had one of the Royal Society 's small hand-spectroscopes , and a small 6-inch transit theodolite by Troughton and Simms , the cap of the objectglass of which I had cut so as to receive the prism-cap of the spectroscope , and had fitted one to the other , so that I could at once shift the prism-cap from its own telescope to that of the theodolite , and vice versed .
I had also a black frame about 2 feet long by 1 foot high with a slit in the centre , the width of which was regulated by turning a black excentric cylinder .
This I had previously used in observing the lines in the solar and other common spectra , and I placed it 10 feet from the theodolite ( the shortest distance the telescope could focus ) ; and close at the back of it I placed a heliotrope held by a Survey Signaller , intending , if opportunity offered , to examine the lines in the spectrum of the corona .
In the diaphragm of the theodolite-telescope I had a system of wires ( shown by diagram below ) , which I had intended for assistance in general observations of the flames , in case I should find that I could make no satisfactory spectrum-observations , which , from the absence Fi .
of any slit arrangement in the spectroscope , I was rather inclined to anticipate .
The wires A A , BB were vertical , C C , D D , EE horizontal , FF the direction of the moon 's path at the middle of the eclipse , Gc and GG perpendicular to F F. This system gave so many fixed distances and points that I thought it would be useful both in estimating the position and the height of / the flames .
However , its utility was not put to the test ; for the little time I had was given to the spectroscope .
I also had an eight-day mean-time chronometer beating half-seconds , by Baker .
The sky in the early morning of the 18th was very cloudy , so that our hopes of success were very low ; but as it afterwards brightened up for a while rather suddenly , we were somewhat encouraged to hope for a similar brightening during part of the eclipse .
Soon , however , at about 7 o'clock , it darkened again , and remained so till after the total phase was over , occasional openings in the nimbi giving us glimpses of the sun through the cirrocumuli which were floating very high up .
At 7 o'clock we had reached our station of observation , which was on a large solid tower called the Upari Btiij , 67 feet high and about 60 feet diameter ( on the top were two guns , one of which was 31 feet long)-one of the many ruins of the city , and .
a most favourable position from which to observe the phenomena of the eclipse and the general aspect of the surrounding country .
On account of the prevailing very high wind , we planted our instruments on and near the top of the external stone staircase so as just to be protected by the tower from the wind .
Mr. Kero Laxuman at first set up his telescope on the top of the tower ; but it was blown down , as I have previously mentioned .
This accident much .
interfered with the carrying out of our preconcerted plan of observation , which was as follows .
Mr. Kero Laxuman and Captain Tanner were to take the times of first and last contact , the latter by observing the actual occurrences , the former by measuring several lengths of the common chord soon after first and before last contact , with the aid of the scale in his 60-power eyepiece and noting the times .
Captain Tanner ( an expert delineator ) was , during totality , to take command of Mr. Kero Laxuman 's telescope , measuring the heights of the flames at times which would be recorded by Mr. Kero Laxuman , whose whole attention during totality was to be given to recording the times of occurrence of any phenomena that he , or either of us , might observe .
Captain Tanner was also to make rapid sketches of all he saw , and I was to confine myself to spectrum-observations .
Unfortunately , contact was not observed until about fifty seconds after the commencement , when Captain Tanner at once made a sketch of the obscuration , Mr. Kero Laxuman recording the time .
The sketch made the common chord equal to 3 ' at 7h 51m 1.7s local time , giving 7h 50 " 17s as the time of first contact .
Captain Tanner afterwards tested that sketch by noting the time before last contact , when the chord appeared of a similar length , which gave an interval of 45s ; so that , taking the mean between the original estimate and its verification , we have 71 50"1 24S'5 as the time of first contact .
While the obscuration was increasing , Captain Tanner , during the few peeps we got at the eclipse , made drawings of the sun 's spots , and sketched the mountains on the moon 's edge , of which there were two plainly visible even wnith my small theodolite .
The darkness increased very slowly till just before totality , when the increase was very rapid and sudden , and a general spontaneous exclamation " Oh !
" from all of us gave Mr. Kero Laxuman the time of beginning of totality , which he recorded as 9h I1 49s .
The eclipse was at that time completely shut out from our view by the clouds-nimbi low down being carried past by the high wind ; we therefore felt at leisure to make our remarks on the degree of the darkness , which we were surprised to find so far from total .
We could easily write , read our writing , and read the seconds of our watches without the aid of artificial light .
We were all lamenting our misfortune in not being able to observe the eclipse , and had given up all hope of witnessing the phenomena we had come so far to see , and Captain Tanner had just noticed the faint reappearance of light in the west , when , contrary to all expectation , and to our intense satisfaction , a sudden opening in the nimbi showed us the eclipse through the cirrocumuli .
We were each at our telescopes in an instant .
I immediately saw through the naked telescope of the small theodolite that red flames were visible , and at once pointed the spectroscope , using the theodolite-telescope as a rest .
Very fortunately I directed the spectroscope with its " refracting edge " tangent to the moon where two red flames were protruding , separated from each other by a small interval ; so that their spectra , which were identical , were extended over the dark background of the moon 's disk , and stood out in m1ost marked and brilliant contrast with the feeble but continuous spectrum of the corona ; and in their spectrum there were the two broad bright bands I have above described .
Most fortunately also these red flames were on that part of the sun which first reappeared ; so that just before or just at emergence there appeared at the very part I was intently observing one brilliant wide spectrum with the green and indigo bands before described , remaining visible for an interval just long enough to enable me to make quite sure of the position of the bands , which were then obliterated by the bright light of the sun .
Of course , observing with the spectroscope alone it would have been impossible to say whether the spectrum with the green and indigo bands appeared just before or just after emergence ; but I think it must have been just before , because Captain Tanner called out when totality was over ; and I immediately remarked that I thought he was rather late , but he was quite confident about the accuracy of his observation .
What struck me as being very remarkable was the circumstance , that though the light of the red flames was to the naked eye so feeble : as to be outshone to extinction by that of the corona , nevertheless , when viewed with the spectroscope , the spectrum of the corona was very weak , and that of the flames remarkably brilliant .
On the first glimpse of the eclipse , before looking through the telescope , the corona appeared so bright , that it gave me the momentary impression ( as it did to Captain Tanner ) of its being an annular eclipse .
We are divided in our estimate of the length of the interval during which we observed the totality .
It appeared to me very short-so much so , that when it was over I was quite taken by surprise to hear that both Captain Tanner and Mr. Kero Laxuman had taken sketches of the flames ; and their sketches , both as to position and structure , were , with one slight exception , remarkably coincident .
From the time of my first pointing the spectroscope to the bursting out of the sun 's light I never once withdrew my eye , though it had been my intention to shift the prism-cap on to the telescope of the theodolite as soon as I should have carefully noted the spectrum of the flames ; but while I was intently gazing on the two bright bands to impress their colour well on my memory , the new spectrum of the moon 's edge appeared , so that I was under the impression that the length of the time of observation was very short .
On the other hand , Captain Tanner , judging from the amount of work he did in the time , estimated it at a minute .
Mr. Kero Laxuman estimated it at 40 or 45 seconds .
Immediately after the totality was over we all three made rough notes of our observations ; and Captain Tanner 's and Mr. Kero Laxuman 's notes agree together wonderfully in their description of the structure of the flames .
The accompanying rough sketch was made by Captain Tanner , who had not the means of making a more finished drawing .
The sketch shows the actual appearance of the eclipse .
It was observed by Captain Tanner wholly inverted , and by Mr. Kero Laxuman ( who used a diagonal eyepiece ) inverted vertically but not laterally .
Captain Tanner and Mr. Kero Laxu .
Capt. Haig 's Spectroscopic Observations man only differed in their position of the small flame c , the former placing it to the right , the latter at a similar distance on the left of the flames b ; but Captain Tanner at once yielded his conviction to that of Mr. Kero Laxuman , which , therefore , we accepted as most likely to be true .
The spectrum of c was not observed by me at all .
I therefore think it could only have appeared simultaneously with the bright spectrum of the moon 's edge .
I so held the spectroscope that I could not see the spectrum of the flame a. The following is an extract from Captain Tanner 's notes , taken almost immediately after the eclipse:- " I at first saw three prominences-one long curved pointed tongue , and two close together , straight but flat-topped , about two-thirds the height of the former .
They were of a rose-madder colour , and were decidedly more like flames than anything else , not only in their general appearance and colour , but by their being composed of smaller tongues of flame parallel ( or nearly so ) to the general axis of the flame , so that they had a streaky appearance and a ragged edge .
At the first glance , when the sun was somewhat obscured by clouds , I thought they were homogeneous and had hard edges ; but this idea was at once dispelled when the clouds cleared off .
The two protuberances , which were close together , were not , as far as I could see , joined by any smaller shots of flame .
I afterwards observed one small protuberance , and marked the position of it in my sketch .
I did not observe that it was streaky , as the others were-perhaps on account of its being so small , and perhaps because I had not sufficient time to examine it properly .
As regards the corona , when we first began to see the eclipse through the clouds , I was under the impression that the eclipse , instead of being total , was only annular , so bright was the corona near the moon 's limb .
I could not detect any irregularities in the structure of the corona , but the light appeared to be gradually shaded off all round .
" Captain Tanner also says , " The most careless observer would notice the streaks of which the flames b were composed ; but it required more careful inspection to determine the streaky nature of the flame a. " The following is from Mr. Kero Laxuman 's notes:- " The protuberance a appeared like a red flaming torch , width 2a minute , height about 2 minutes , colour dark red , lines stretched over a less-red ground .
The direction not perpendicular to the edge of the moon , but making an angle of 600 with it .
Those marked b were broader and almost as high as a , but not pointed .
They appeared to expand a little at the vertex .
They were also streaked by several dark-red lines .
That marked c appeared semicircular , with a breadth of about 2a minute .
The flame a was visible for about 2 minutes after the end of totality ; and had there been no clouds , I think it could have been seen longer .
" Both Captain Tanner and Mr. Kero Laxuman also agreed in describing the form of the red flames b as somewhat similar to hands with fingers slightly separated .
There is a curious coincidence which I may here mention , though I imagine it can only be regarded as purely fortuitous , viz. that the flames were almost exactly opposite the spots on the sun 's disk .
On the afternoon of the 18th , Captain Tanner and I went to Moolwar , eighteen miles south of Beejapoor , where the German astronomers had put up their instruments .
We there learnt that they had only seen the eclipse for less than 5 seconds during totality , and that through an upper stratum of clouds which rendered photometric observations impracticable ; but we were surprised to hear that neither a spectroscope nor a polariscope was attached to either of their equatorial telescopes at the time of visibility , but that both the observerswith these instruments were intent on measuring the heights of the flames .
They determined the normal height of flame a to be 3 minutes ; but as they must have seen it at an earlier phase than Captain Tanner and Mr. Kero Laxuman , it would appear slightly longer to them than to us .
It is very curious how the darkness during totality seems to have differed in degree in different places .
At Beejapoor we were told that down below in the town the darkness was so great that it was not possible to see one 's own hand .
We thought this account might be an exaggeration ; but we afterwards learnt that at Moolwar a gentleman dropped part of an eyepiece of a telescope , and that it was not possible to find it even by placing the eye close to the ground , until after the end of totality .
We have not had time during our continual travelling to compute the elements of the eclipse for Beejapoor for ourselves ; and it might have been waste of time to have done so before we started on our journey , for we were uncertain of our being able to get so far south as Beejapoor ; but I give below a statement of elements for Beejapoor as computed by Mr. Pogson , astronomer at Madras , and published in the 'Times of India , ' and with it the times as observed or estimated by us .
Mr. Pogson 's Our Remarks elements .
elements .
h m.s h mn s First contact ... ... ... ... ... . .
7 50 54 7 50 25 Mean of two estimates .
Beginning of totality ... ... . .
92991 49 Approximate .
End of totality ... ... ... ... ... 97 21 96 59 Actually observed .
Last contact ... ... ... ... ... ... 1028 44 0 28 14 , , , , Angle from 1 first contact ... 1 ?
right .
At vertex .
Approxie .
vertex of ... last contact ... 173 ?
right .
165 ?
right .
p imate There was a difference in our times of last contact .
Mr. Kero Laxuman made it at 1Oh 281 9 ; I made it 10h 28m 14 , and Captain Tanner 10h 28"'17 , .
I was observing with the little theodolite , and distinctly saw the moon 's limb after Mr. Kero Laxuman had called out ; so I attributed his error to the vibration of his telescope caused by the wind .
Capt. Tanner observed , I believe , the last contact ; but , strange to say , the point of the moon which made last contact was a mountain-peak of this shape ; Capt. Tanner would make it thus , dividing the mountain into two hills ; and he says I was a second too soon in my observation , which was of the spherical last contact ; and perhaps he was right , as he had a better telescope than I had .
His observation at 1 Oh 28m 17s was the time of the peak leaving the sun 's limb ; so that he and I differ only by 1 second , as to whether the spherical last contact occurred at 10h 28 " 14s or 10h 28 " 15 " .
I sent a native assistant to Moolwar ( the station selected by the German astronomers ) to take observations with a barometer , and with wet- , dry- , and black-bulb thermometers , continuously for some days before and after the eclipse , but I anticipate no interesting results ( from the rough glance I took at the records on the evening of the 18th ) .
The atmosphere was during the time in a very disturbed state .
Mr. Chambers , of the Bombay Observatory , went to a village called Mongoli , about six miles east of Moolwar , with the intention of observing the eclipse ; but he was disappointed , for it was completely obscured by clouds during the whole of the total phase .
I have not yet heard what success has attended Lieuts .
Herschel and Campbell with the spectroscope and polariscope at Jamkhandi , so that I am quite ignorant of the value of our observations ; but I trust that even should other observers have succeeded in contributing to physics more definite information , ours may at least be valuable as corroborative evidence .
I am , dear Sir , Yours faithfully , C. T. HAIG , Captain Royal Engineers .
General Sabine , R.A. , P.R.S. EXPLANATION OF THE PLATE .
Fig. 1 represents the total eclipse as it appeared during the last 20 seconds of the total phase .
Fig. 2 .
Red prominences , drawn to larger scale , and showing the streaked structure of a and the radiating thicker lines composing the double prominence at b. ( Note .
A light-red colour showed itself between these streaks , which gave the prominences a greater appearance of solidity .
) c2 , small red prominences as noted by Kero Laxuman ; ce , the same as noted by me ( e appeared just at the end of totality ) .
The height of a was a little over 2 ' , b about 1 ' 40 " ; c may have been 0 ' 20 " .
|
112355 | 3701662 | Account of Observations of the Total Eclipse of the Sun, Made August 18th, 1868, along the Coast of Borneo | 81 | 90 | 1,868 | 17 | Proceedings of the Royal Society of London | J. Pope Hennessy | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1868.0009 | null | proceedings | 1,860 | 1,850 | 1,800 | 10 | 191 | 4,649 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112355 | 10.1098/rspl.1868.0009 | http://www.jstor.org/stable/112355 | null | null | Astronomy | 39.127974 | Optics | 24.304881 | Astronomy | [
64.59703826904297,
45.39208221435547
] | seemed to be a tower of rose-coloured clouds .
The colour was most beautiful more beautiful than any rose-colour I ever saw ; indeed I know of no natural object or colour to which it can be , with justice , compared .
Though one has to describe it as rose-coloured , yet in truth it was very different from any colour or tint I ever saw before .
This protuberance extended from the right of the upper limb , and was visible for six minutes .
In five seconds after this was visible , a much broader and shorter protuberance appeared at the left side of the upper limb .
This seemed to be composed of two united together .
In colour and aspect it exactly resembled the long one .
This second protuberance gradually sank down as the sun continued to fall behind the moon , and in three minutes it had disappeared altogether .
A few seconds after it had sunk down there appeared at the lower corresponding limb ( the right inferior corner ) a similar protuberance , which grew out as the eclipse proceeded .
This also seemed to be a double protuberance , and in size and shape very much resembled the second one ; that is , its breadth very much exceeded its height .
In colour , however , this differed from either of the former ones .
Its left edge was a bright blue , like a brilliant sapphire with light thrown upon it ; next to that was the so-called rose-colour , and , at the right corner , a sparkling ruby tint .
This beautiful protuberance advanced at the same rate that the sun had moved all along , when suddenly it seemed to spread towards the left , until it ran around one-fourth of the circle , making a long ridge of the rosecoloured masses .
As this happened , the blue shade disappeared .
In about twelve seconds the whole of this ridge vanished , and gave place to a rough edge of brilliant white light , and in another second the sun had burst forth again .
In the meantime the long , rose-coloured protuberance on the upper right limb had remained visible ; and though it seemed to be sinking into the moon , it did not disappear altogether until the lower ridge had been formed and had been visible for two seconds .
This long protuberance was quite visible to the naked eye , but its colour could not be detected except through the telescope .
To the naked eye it simply appeared as a little tower of white light standing on the dark edge of the moon .
The lower protuberance appeared to the naked eye to be a notch of light in the dark edge of the moon-not a protuberance , but an indentation .
In shape the long protuberance resembled a goat 's horn .
As I have not time to attempt an elaborate drawing of these objects , I content myself with enclosing to your Lordship two pages from my rough note-book , showing the sketches taken at the moment .
Though the darkness was by no means so great as I had expected , I was unable to mark the protuberances in my note-book without the aid of a lantern , which the sailors lit when the eclipse becane total .
Fig. 3 .
Fig. 4 .
" '".].'*':::'. .
" ..~',.~ , ' : : : .
" iv iii : !
' / .- " .
' ... . .
: " " ... ... ... l.s ... :./ / ^'^ ^l f !
/\ I. , .
, ',. .
, -/ 1/ / ~~~~I -f l. .
''-_,.- , e / ' , \\ Those who were looking out for stars counted nine visible to the naked eye .
One planet ( Venus ?
) was very brilliant .
Its altitude at 11 3111 0 was 30§ 32 ' ( Carey 's Government Sextant , no error ) , and its distance from the nearest limb of the moon was 37§ 28 ' .
The altitude of the lower limb of the moon at 1 32 " 08 was 66§ 30 ' .
On board the ' Rifleman ' the fowls and pigeons went to roost , but the cattle showed no signs of uneasiness ; they were lying down at the time .
Whatever interest the foregoing observations may have for men of science , I am happy to be able to report that Capt. Reed has added to his public services by seizing this opportunity for determining the exact longitude of Barram Point .
Navigators have long been anxious to fix the precise longitude of some point along the coast of Borneo , and the event of yesterday has probably accomplished this .
When Capt. Reed 's calculations have been finally reduced , he will , no doubt , communicate them to the head of his department ; and in the meantime he has kindly undertaken to place in a cover , directed to your Lordship , the true time as worked out from the observations , so that the times given in this despatch may be corrected before the despatch is used .
The time given in this despatch was taken from one of Parkinson and Frodsham 's Government pocket chronometers , No. 1887 .
As I believe we were the nearest group of observers to the Equator , and as the other conditions were unusually favourable for our work , I venture to hope that even the inadequate and very unscientific account I have given may prove to be of some interest to your Lordship and to the men of science in England .
Before closing my despatch I received from Capt. Reed the error of the chronometer-watch used for taking the time .
It was fast on the mean time at Barram Point oh 41 8s7 .
I have the honour to he , My Lord , Your Lordship 's most obedient humble Servant , ( Signed ) J. POPE IHENNESSY , Governor of Labuan , and Consul-General in the Island of Borneo .
T'o the Right Honourable Lord Stanley , M.P. , Secretary of State for Foreign jffairs .
[ Note.-The phenomenon of the sun 's crescent reflected on to the disk of the moon would seem to have been something accidental , perhaps ( if seen by the writer only ) a mere ghost , depending on a double reflectio.n between the glasses of his instrument .
The figure represents the " reflected " image as in the same position as the crescent itself , not reversed , indicating either a refraction or a double reflectiono The slender beams of light or shade shooting out from the horns of the crescent would seem to admit of easy explanation , supposing them to have been of the nature of sunbeams , depending upon the illumination of the atmosphere of the earth by the sun 's rays .
The perfect shadow , or umbra , would be a cone circumscribing both sun and moon , and having its vertex far below the observer 's horizon .
Within this cone there would be no illumination of the atmosphere , but outside it a portion of the sun 's rays would be scattered in their progress through the air , giving rise to a faint illumination .
When the total phase drew near , the nearer surface of the shadow would be at no great distance from the observer ; the further surface would be remote .
Attend in the first instance to some one plane passing through the eye and cutting the shadow transversely , and in this plane draw a straight line through the eye , touching the section of the cone which bounds the shadow ; and then imagine other lines drawn through the eye a little inside and outside this .
In the former case the greater part of the line , while it lay within the lower regions of the atmo- .
sphere , would be in shadow , the only part in sunshine being that reaching from the eye to the nearer surface of the shadow ; but in the latter case the line would be in sunshine all along .
In the direction of the former line , therefore , there would be but little illumination arising from scattered light , while in the direction of the latter the illumination would , comparatively speaking , be considerable .
In crossing the tangent there would be a rapid change of illuminiation .
Now pass on to three dimensions .
Instead of a tangent line we shall have a tangent pla.ne , and there will of course be two such planes , touching the two sides of the cone respectively .
Each of these will be projected on the visual sphere into a great circle , a common tangent to the two small circles , which are the projections of the sun and moon .
In crossing either of these there will be a rapid change of illumination ( feeble though it be at best ) which will be noticed , According as the observer mentally regards darkness as the rule and illumination as the feature , or illumination as the rule and darkness as the feature , he will describe what he sees as a beam or a shadow .
The direction of these beams or shadows given by theory , as just explained , agrees very well with the drawing sent by Governor Hennessy , which does not represent the left-hand beam so distinctly divided as it appears in the woodcut .
The times mentioned in the above despatch have not been corrected for the error of the chronometer-watch .
In the following Tables , furnished by Staff Commander Reed , the corrected mean times alone are printed .
The observations of time by Capt. Reed , Mr. Ray , and Mr. Doorly were made by Government pocket chronometer No. 1887 , which was fast on mean time of place oh 4m 8's7 ; those by Mr. Ellis by a gold pocket watch , compensation balance , which was fast on mean time of place 011 17m 2S7 ; those belonging to the meteorological observations with a pocket watch , which was fast on mean time of place O0 2 " 47S'9 .
G. G. STOKES .
] Meteorological Observations taken on board I.M.S. 'Rileman , ' at Barram Point , during the Total Eclipse of the Sun , August 18th , 1868 .
Mean of Dry thermoWet thermoMcean time at , Marine barotwo thermeter hung in meter hung in placeQ .
meter in mometers the main rigthe main rigChart-house .
in Chartging exposed ging exposed house .
to the sun .
to the sun .
A.M. hms in .
o7 57 Iz'I 29'98 81 oo8 57 II 30'01 81 92 93'5 9 57 I2'i 30o00 85 86.5 83'5 Io 57 I1'I 29'99 84 91 87 ] II 57 1213 ' 29'98 85 88 85 , P.M. o 23 IX ' .
29'96 85 9I 88 o 42 I2'I 29'6 85 9 87 o 57 1z ' 2-9'94 85 88 86 I 12 X2'I 29'93 85 87 85 1 23 9'1 z9'92 85 85 83 32 12'1 29'92 85 85 83 1 57 I2 ' 29'91 85 91 85 2 27 Iz'I 29'91 85 96 90 2 48 5 ' 1 2991 86 96 89 JNO .
W..EED , Staff Commander in charge of China Sea Seurvey .
Total Eclipse of the Sun .
1868 .
] 89 Observations of the Total Eclipse of the Sun , lugust 18th , 1868 .
H.M.S. ' Rileman , ' Barram Point .
Mean Time at Place .
Phenomena observed .
C r. Reed .
Mr Ray .
Mr. Ellis .
Dory .
First contact of moon with sun 's lim b * ... ... ... ... ... ... ... ... ... ... ... Contact of moon 's limb with penumbra of No. I spot ... ... ... ... ... Contact of moon 's limb with left of No. I spot ... ... ... ... ... ... ... ... . .
Contact of moon 's limb with right of No. I spot ... ... ... ... ... ... ... ... Contact of moon 's limb with sun 's centre ... ... ... ... ... ... ... ... ... ... ... ... Contact of moon 's limb with centre of No. z spot ... ... ... ... ... ... ... ... . .
Contact of moon 's limb with No. 3 spot ( double ) ... ... ... ... ... ... ... ... Contact of moon 's limb with No. 4 spot ... ... ... ... ... ... ... ... ... ... ... . .
Sun totally obscured ... ... ... ... ... ... Rose-coloured mass left side disappeared ... ... ... ... ... ... ... ... ... ... . .
Altitude of planet Venus 30o 32 ' ( Carey 's GNovt .
sextant , no error ) ... Planet Venus distant froi nearest limb of moon 37§ 28 ' ... ... ... ... ... Rose-coloured protuberance appeared below ... ... ... ... ... ... ... ... ... ... Altitude of lower limb of moon 66§ 30 ' ... ... ... ... ... ... ... ... ... ... ... ... .
First appearance of sun 's limb I ... ... No. 1 spot reappeared ( centre ) ... ... Venus disappeared from view ... ... ... No. 2 spot reappeared ( centre ) ... ... No. 3 spot ( double ) reappeared ( centre ) ... ... ... ... ... ... ... ... ... ... ... No. 4 spot ( double ) reappeared ( centre ) ... ... ... ... ... ... ... ... ... ... ... Last contact of limbs ... ... ... ... ... ... hms 12 20 io'8 12 21 12 22 h mn S 12 20 ... ... ... ... I2 so II'5 hms II 56 07-I i6'3 I2 2z i6-8 12 2I 19'8 49'3 I2 22 49'3 I2 22 49'3 ... I ... ... . .
0o6 38-8 i 13 58'3 i 20 09'3 I 23 13'3 I 25 38'3 ... ... ... ... I 27 51'3 I 29 25-3 2 07 36'3 ... ... ... ... I2 40 06'3 i 06 38'8 I I3 57'3 o06 I 13 43-3 57'3 23 13'3 i 23 I4'3 26 5I'3 I 27 0o'3 ... ... ... ... I 27 5I'3 I 29 25'3 1 37 03'3 2 29 05-3 2 35 39'3 2 43 58'3 2 48 3I'1 I 27 I9'3 I 29 26'3 2 29 o5'3 2 35 39*3 2 48 32'1 rNSta .
v Co. tin arg in r Staff Golmmander in charge of China Sea Survey .
Remarks.-lll.0 O A.l. , wind W.S.W. 2 b. c. , a hazy appearance about the horizon .
made August 18th , 1868 , along the coast of Borneo , in a Letter addressed to H.M. Secretary of State for Foreign Affairs by His Excellency J. PorE HENNESSY , Governor of Labuan .
" Communicated by the Right Hon. Lord STANLEY , F.R.S. Received October 8 , 1868 .
Government Ilouse , Labuan , 19th August , 1868 .
MY LORD , -Seeing the interest which Her Majesty 's Government and the scientific public in England have shown in the remarkable eclipse which occurred yesterday , I took steps to make such observations as I could along the coast of Borneo , and I have now the honour of laying them before your Lordship .
After passing from the Gulf of Siam across the China Sea , the line of total eclipse passed across the Island of Borneo , touching the colony of Labuan on the east , and stretching not far from the River Bintulu on the west .
Having ascertained that the precise centre of this band of total eclipse would be found at Barram Point ( a place within my jurisdiction as ConsulGeneral in the Island of Borneo ) , I made arrangements with Capt. Reed , of H.M.S. 'Rifleman , ' to take my observations at that spot .
As that well-known officer has been for years in charge of the important survey of the China seas , his ship afforded special facilities for such an expedition .
We left Labuan on Monday at noon , and arrived off Barram Point at five o'clock next morning , Tuesday the 18th .
A tent was fitted up on an open space between a Casuarina-plantation and the sea , and the following corps of observers landed at ten o'clock : Captain Reed , Lieutenant Ray , Lieutenant Ellis , and myself , our four telescopes being securely adjusted on large tripod stands manufactured for the occasion .
Four 6ther officers landed with us:-Dr .
O'Connor to note the physiological phenomena , Mr. Wright to watch the magnetic needle , and Mr. Doyley and Mr. Roughton to mark the time .
A few intelligent sailors were in attendance to assist the observers , if necessary .
Mr. Petley and the other officers left on board the ' Rifleman ' had charge of the barometrical and thermometrical observations , and they were also directed by Captain Reed to watch the vibrations , if any , in the magnetic compasses .
Before leaving the ship I made some observations upon the solar spots .
At 8 A.M. I found some spots in a line from east to south b. The upper * It did not seem necessary to reproduce the sketch sent by the author , as the position of the spots may be represented by conceiving the next figuire to be turned round through about 65 ?
in the direction of the hands of a watch .
Governor Hennessy 's Observations on the spot was surrounded by a penumbra stretching towards the centre of the sun , the second spot was small and sharply defined , the third spot , or group of spots , had a penumbra , and the fourth spot was surrounded by a space of very brilliant light .
These spots I subsequently refer to as Nos. 1 , 2 , 3 , and 4 .
Moving with the rotation of the sun , the line of spots gradually became horizontal , and at 12 o'clock ( noon ) they lay thus ( see fig. 1 ) .
Fig. 1 .
IX the moon with the penumbra of spot No. 1 .
At 121 25m 25`'5 contact with left of No. 1 spot .
At 12 " 26m " 58s the spot was completely covered .
During all this time no vibrations or change of any kind was noticed in the magnetic needle .
At 12n 44dm 15S the moon 's limb had advanced to the sun 's centre .
At 1 " 10 " 47'*5 spot No. 2 was passed , and at I " 18 ' " 6 ' spot No. 3 was passed .
All this time not the smallest magnetic change could be noticed .
At Lh 2"7 22s the total eclipse took place , and lasted for 6 minutes and 13 seconds ; the first appearance of the sun 's limb from behind the moon being at 1 " 33 ' 35s .
The spots reappeared as follows : No. 1 at lh 4d1 " 128 2 , , 2 33 14 3 , , 2 39 48 4 , ,2 48 7 ; and at 21 52 " 39s'8 the last contact of the edge of the sun and moon was noticed .
During the 6"m and 13 of total eclipse not the slightest change of any kind could be observed in the magnetic needle , nor did it move or vibrate in any way on the appearance of the solar spots .
To complete the negative results of our magnetic observations , I have only to add that the officers who had been directed to watch the ship 's compasses report that they could not detect the slightest movement of any kind .
I now proceed to describe the general phenomena of the eclipse ; and in doing so I confine myself to copying from the rough notes I took at Barram Point , and from the note-books of Capt. Reed and his officers , also taken on the spot .
As the mail closes for Singapore to-morrow morning , I have not time to arrange the materials before me in anything like scientific order ; and the absence of any works of reference ( we have not even this year 's supplement to the Nautical Almanac ) renders me still less able to do justice to the facts we collected .
We were very fortunate in the weather .
The day was bright and clear ; not a cloud was near the sun .
A few round white clouds that lay on the horizon hardly moved .
There was a slight breeze from W.S.W. The sea was breaking heavily on the shore , and it had a slight brownish bluish tinge all over , except where the white breakers approached the land .
The grove of Casuarina trees behind us had the same deep-green colour which they always exhibit on a fine day in the tropics .
A few swallows were skimming about high in the air .
We also noticed some dragonflies , butterflies , and a good many specimens of a large heavy fly like a drone-bee .
When we left the ship at 10 o'clock the barometer was 30'00 ; the mean of the two thermometers in the deck chart-room ( in the shade ) was 85 ?
; the dry thermometer exposed to the sun was 91 ?
, and the wet thermometer exposed to the sun was 83 ?
'5 .
During the progress of the eclipse the barometer fell steadily .
At 121 0O ' 15s , first contact , it was 29-98 .
At 12h 26 " ' 0 it fell to 29-96 in .
, 12 44 15 it was 29-96 , ,1 0 0 , 29-94 1 15 0 , , 29-93 Total , , 1 27 22 , , 29-92 eclipse .
, , 1 33 35 , , 2992,2 0 0 , , 2991 2 30 0 , , 29'91 , 2 39 48 , , 2991 , , 2 52 39-8 , , 29-91 The mean of the two thermometers in the shade was 85 ?
, without any change whatever from 10 o'clock till the close of the eclipse .
At the close of the eclipse , 2 " 52 " 39S'8 , it rose to 86 ? .
The dry-bulb thermometer , hung in the sunlight , stood at 91 ?
at the first contact .
G At 12 " 44 " 15s it fell to 900 , ,1 0 0 , 88 1 , 15 0 , 87 Total f1 27 22 , , 85 eclipse.l , , 1 33 35 , , 85 , 20O itroseto 91 , , 2 30 0 , 96 , 2 52 39-8 , 96 It thus appears that the thermometer fell from 91 ?
to 85 ?
as the moon was covering the sun , and that it rose from 85 ?
to 96 ?
as the sun was reappearing .
The wet-bulb thermometer fell from 80 ?
'5 to 83 ?
at the total eclipse , and rose to 89 ?
at the termination of the whole eclipse .
Ten minutes before the total eclipse there seemed to be a luminous crescent reflected upon the dark body of the moon .
In another minute a long beam of light , pale and quite straight , the rays diverging at a small angle , shot out from the westerly corner of the sun 's crescent .
At the same time Mr. Ellis noticed a corresponding dark band , or shadow , shooting down from the east corner of the crescent ( fig. 2 ) .
Fig. 2 .
/ I. / .
At this time the sea assumed a darker aspect , and a well-defined green band was seen distinctly around the horizon .
The temperature had fallen * See note at the end .
and the wind had slightly freshened .
The darkness then came on with great rapidity .
The sensation was as if a thunderstorm was just about to break , and one was startled on looking up to see not a single cloud overhead .
The birds , after flying very low , disappeared altogether .
The dragonflies and butterflies disappeared , and the large drone-like flies all collected on the ceiling of the tent and remained at rest .
The crickets and Cicadre in the jungle began to sound ; and some birds , not visible , also began to twitter in the jungle .
The sea grew darker , and immediately before the total obscuration the horizon could not be seen .
The line of round white clouds that lay near the horizon changed their colour and aspect with great rapidity .
As the obscuration took place they all became of a dark purple , heavy looking , and with sharply defined edges ; they then presented the appearance of clouds close to the horizon after sunset .
It seemed as if the sun had set at the four points of the horizon .
The sky was of a dark leaden blue , and the trees looked almost black .
The faces of the observers looked dark , but not pallid or unnatural .
The moment of maximum darkness seemed to be immediately before the total obscuration ; for a few seconds nothing could be seen except objects quite close to the observers .
Suddenly there burst forth a luminous ring around the moon .
This ring was composed of a multitude of rays , quite irregular in length and in direction ; from the upper and lower parts they extended in bands to a distance more than twice the diameter of the sun .
Other bands appeared to fall towards one side ; but in this there was no regularity , for bands near them fell away apparently towards the other side .
When I called attention to this , Lieut. Ray said , " Yes , I see them ; they are like horses ' tails ; " and they certainly resembled masses of luminous hair in complete disorder .
1 have said these bands appeared to fall to one side ; but I do not mean that they actually fell or moved in any way during the observation .
If the atmosphere had not been perfectly clear , it is possible that the appearance they presented would lead to the supposition that they moved ; but no optical delusion of the kind was possible under the circumstances .
During the second when the sun was disappearing , the edge of the luminous crescent became broken up into numerous points of light .
The moment these were gone , the rays I have just mentioned shot forth , and at the same time we noticed the sudden appearance of the rose-coloured protuberances .
The first of these was about one-sixth of the sun 's diameter in length , and about one-twenty-fourth part of the sun 's diameter in breadth .
It all appeared at the same instant , as if a veil had suddenly melted away from before it .
1868 .
] 85
|
112356 | 3701662 | Further Particulars of the Swedish Arctic Expedition | 91 | 91 | 1,868 | 17 | Proceedings of the Royal Society of London | A. I. Nordenski\#xF6;ld | fla | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 1 | 11 | 306 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112356 | null | http://www.jstor.org/stable/112356 | null | null | Geography | 41.966559 | Biography | 31.797546 | Geography | [
58.3880500793457,
10.804266929626465
] | VII .
" Further particulars of the Swedish Arctic Expedition , in a Letter addressed to the President , by Prof. NOltDENSKIOLD .
" Communicated by the President .
Received October 15 , 1868 .
Kobbe Bay , Sept. 16th , 1868 .
SIR , In my last letter from Stockholm I promised to send you , with the returning naturalists , a detailed relation of the first scientific part of the Swedish Arctic Expedition of 1868 ; but unfortunately our last coalship , with which five of our fellow travellers , with the rich geological , zoological , and botanical collections , made during this season in the arctic regions , return to Tromso , and which gives us the last occasion of communicating with Europe , leaves this harbour in some hours , and that makes it impossible for me to keep my promise .
However , a detailed report will immediately be sent to you by one of the returning naturalists , Dr. Malmgren , a member also of the expeditions of 1861 and 1864 .
The remaining part of our expedition will from here go , first , to Seven Island , and then ( perhaps one of the first days of October ) , after having deposited a boat and a depot of provisions on Ross Islet , further northward .
The polar sea was in the end of August quite covered with ice north of 81§ 9 ' , the highest latitude hitherto reached by our steamer .
But a week later the sea was open to Walden and Table Island , and the 8th of September I could , from one of the highest peaks of Parry Island , discern only traces of ice further northward .
I remain , Sir , respectfully yours , A. I. NOIDENSKIOLD .
|
112357 | 3701662 | Notice of an Observation of the Spectrum of a Solar Prominence, by J. N. Lockyer, Esq | 91 | 92 | 1,868 | 17 | Proceedings of the Royal Society of London | J. Norman Lockyer | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1868.0011 | null | proceedings | 1,860 | 1,850 | 1,800 | 2 | 15 | 233 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112357 | 10.1098/rspl.1868.0011 | http://www.jstor.org/stable/112357 | null | null | Atomic Physics | 35.70877 | Biography | 34.58577 | Atomic Physics | [
18.015605926513672,
-36.291351318359375
] | VIII .
Notice of an Observation of the Spectrum of a Solar Prominence , by J. N. LOCKYER , Esq. , in a Letter to the Secretary .
" Communicated by Dr. SHARPEY .
Received October 21 , 1868 .
October 20 , 1868 .
SIR , -I beg to anticipate a more detailed communication by informing you that , after a number of failures , which made the attempt seem hopeless , I have this morning perfectly succeeded in obtaining and observing part of the spectrum of a solar prominence .
As a result I have established the existence of three bright lines in the following positions : I. Absolutely coincident with C. II .
Nearly coincident with F. III .
Near D. The third line ( the one near D ) is more refrangible than the more refrangible of the two darkest lines by eight or nine degrees of Kirchhoff 's scale .
I cannot speak with exactness , as this part of the spectrum requires remapping .
I have evidence that the prominence was a very fine one .
The instrument employed is the solar spectroscope , the funds for the construction of which were supplied by the Government-Grant Committee .
It is to be regretted that its construction has been so long delayed .
I have &c. , J. NORMAN LOCKYER .
The Secretary of the Royal Society .
|
112358 | 3701662 | On a New Series of Chemical Reactions Produced by Light | 92 | 102 | 1,868 | 17 | Proceedings of the Royal Society of London | John Tyndall | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1868.0012 | null | proceedings | 1,860 | 1,850 | 1,800 | 11 | 215 | 5,839 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112358 | 10.1098/rspl.1868.0012 | http://www.jstor.org/stable/112358 | null | null | Optics | 34.938506 | Thermodynamics | 21.021139 | Optics | [
0.020179251208901405,
-17.500791549682617
] | IX .
" On a New Series of Chemical Reactions produced by Light .
" By JOHN TYNDALL , LL. D. , F.R.S. , &c. Received October 24 , 1868 .
I ask permission of the Royal Society to draw the attention of chemists to a form or method of experiment which , though obvious , is , I am informed , unknown , and which , I doubt not , will in their hands become a new experimental power .
It consists in subjecting the vapours of volatile liquids to the action of concentrated sunlight , or to the concentrated beam of the electric light .
Action of the Electric Light .
A glass tube 2'8 feet long and of 2'5 inches internal diameter , frequently employed in my researches on radiant heat , was supported horizontally .
At one end of it was placed an electric lamp , the height and position of both being so arranged that the axis of the glass tube and that of the parallel beam issuing from the lamp were coincident .
The tube in the first experiments was closed by plates of rock-salt , and subsequently by plates of glass .
As on former occasions , for the sake of distinction , I will call this tube the experimental tube .
The experimental tube was connected with an air-pump , and also with a series of drying and other tubes used for the purification of the air .
A number of test-tubes ( I suppose I have used fifty of them in all ) were converted into Woulfe 's flasks .
Each of them was stopped by a cork through which passed two glass tubes : one of these tubes ( a ) ended immediately below the cork , while the other ( 6 ) descended to the bottom of the flask , being drawn out at its lower end to an orifice about 0'03 of an inch in diameter .
It was found necessary to coat the cork carefully with cement .
The little flask thus formed was partially filled with the liquid whose vapour was to be examined ; it was then introduced into the path of the purified current of air .
The experimental tube being exhausted , and the cock which cut off the supply of purified air being cautiously turned on , the air entered the flask [ lecess , 9 through the tube b , and escaped by the small orifice at the lower end of b into the liquid .
Through this it bubbled , loading itself with vapour , after which the mixed air and vapour , passing from the flask by the tube a , entered the experimental tube , where they were subjected to the action of light .
The power of the electric beam to reveal the existence of anything within the experimental tube , or the impurities of the tube itself , is extraordinary .
When the experiment is made in a darkened roomt , a tube which in ordinary daylight appears absolutely clean is often shown by the present mode of examination to be exceedingly filthy .
The following are some of the results obtained with this arrangement : Nitrite of amyl ( boiling-point 91 ?
to 96 ?
C.).-The vapour of this liquid was in the first instance permitted to enter the experimental tube while the beam from the electric lamp was passing through it .
Curious clouds were observed to form near the place of entry , which were afterwards whirled through the tube .
The tube being again exhausted , the mixed air and vapour were allowed to enter it in the dark .
The slightly convergent beam of the electric light was then sent through the tube from end to end .
For a moment the tube was optically empty , nothing whatever was seen within it ; but before a second had elapsed a shower of liquid spherules was precipitated on the beam , thus generating a cloud within the tube .
This cloud became denser as the light continued to act , showing at some places a vivid iridescence .
The beam of the electric lamp was now converged so as to form within the tube , between its end and the focus , a cone of rays about eight inches long .
The tube was cleansed and again filled in darkness .
When the light was sent through it , the precipitation upon the beam was so rapid and intense that the cone , which a moment before was invisible , flashed suddenly forth like a solid luminous spear .
The effect was the same when the air and vapour were allowed to enter the tube in diffuse daylight .
The cloud , however , which shone with such extraordinary radiance under the electric beam , was invisible in the ordinary light of the laboratory .
The quantity of mixed air and vapour within the experimental tube could of course be regulated at pleasure .
The rapidity of the action diminished with the attenuation of the vapour .
When , for example , the mercurial column associated with the experimental tube was depressed only five inches , the action was not nearly so rapid as when the tube was full .
In such cases , however , it was exceedingly interesting to observe , after some seconds of waiting , a thin streamer of delicate bluish-white cloud slowly forming along the axis of the tube , and finally swelling so as to fill it .
When dry oxygen was employed to carry in the vapour , the effect was the same as that obtained with air .
When dry hydrogen was used as a vehicle , the effect was also the same .
The effect , therefore , is not due to any interaction between the vapour of the nitrite and its vehicle .
This was further demonstrated by the deportment of the vapour itself .
When it was permitted to enter the experimental tube unmixed with air or any other gas , the effect was substantially the same .
Hence the seat of the observed action is the vapour itself .
With reference to the air and the glass of the experimental tube , the beam employed in these experiments was perfectly cold .
It had been sifted by passing it through a solution of alum , and through the thick doubleconvex lens of the lamp .
When the unsifted beam of the lamp was employed , the effect was still the same ; the obscure calorific rays did not appear to interfere with the result .
I have taken no means to determine strictly the character of the action here described , my object being simply to point out to chemists a method of experiment which reveals a new and beautiful series of reactions ; to them I leave the examination of the products of decomposition .
The molecule of the nitrite of amyl is shaken asunder by certain specific waves of the electric beam , forming nitric oxide and other products , of which the nitrate of amyl is probably one .
The brown fumes of nitrous acid were seen to mingle with the cloud within the experimental tube .
The nitrate of amyl , being less volatile than the nitrite , could not maintain itself in the condition of vapour , but would be precipitated in liquid spherules along the track of the beam .
In the anterior portions of the tube a sifting action of the vapour occurs , which diminishes the chemical action in the posterior portions .
In some experiments the precipitated cloud only extended halfway down the tube .
When , under these circumstances , the lamp was shifted so as to send the beam through the other end of the tube , precipitation occurred there also .
Action of Sunlight .
The solar light also effects the decomposition of the nitrite-of-amyl vapour .
On the 10th of October I partially darkened a small room in the Royal Institution , into which the sun shone , permitting the light to enter through an open portion of the window-shutter .
In the track of the beam was placed a large plano-convex lens , which formed a fine convergent cone in the dust of the room behind it .
The experimental tube was filled in the laboratory , covered with a black cloth , and carried into the partially darkened room .
On thrusting one end of the tube into the cone of rays behind the lens , precipitation within the cone was copious and immediate .
The vapour at the distant end of the tube was in part shielded by that in front , and was also more feebly acted on through the divergence of the rays .
On reversing the tube , a second and similar cone was precipitated .
Physical considerations .
I sought to determine the particular portion of the white beam which produced the foregoing effects .
When , previous to entering the experimental tube , the beam was caused to pass through a red glass , the effect was greatly weakened , but not extinguished .
This was also the case with various samples of yellow glass .
A blue glass being introduced , before the removal of the yellow or the red , on taking the latter away augmented precipitation occurred along the track of the blue beam .
Hence , in this case , the more refrangible rays are the most chemically active .
The colour of the liquid nitrite of amyl indicates that this must be the case ; it is a feeble but distinct yellow : in other words , the yellow portion of the beam is most freely transmitted .
It is not , however , the transmitted portion of any beam which produces chemical action , but the absorbed portion .
Blue , as the complementary colour to yellow , is here absorbed , and hence the more energetic action of the blue rays .
This reasoning , however , assumes that the same rays are absorbed by the liquid and its vapour .
A solution of the yellow chromate of potash , the colour of which may be made almost , if not altogether , identical with that of the liquid nitrite of amyl , was found far more effective in stopping the chemical rays than either the red or the yellow glass .
But of all substances the nitrite itself is most potent in arresting the rays which act upon its vapour .
A layer one-eighth of an inch in thickness , which scarcely perceptibly affected the luminous intensity , sufficed to absorb the entire chemical energy of the concentrated beam of the electric light .
The close relation subsisting between a liquid and its vapour , as regards their action upon radiant heat , has been already amply demonstrated * .
As regards the nitrite of amyl , this relation is more specific than in the cases hitherto adduced ; for here the special constituent of the beam which provokes the decomposition of the vapour is shown to be arrested by the liquid .
A question of extreme importance in molecular physics here arises : What is the real mechanism of this absorption , and where is its seat t ?
I figure , as others do , a molecule as a group of atoms , held together by their mutual forces , but still capable of motion among themselves .
The vapour of the nitrite of amyl is to be regarded as an assemblage of such molecules .
The question now before us is this : In the act of absorption , is it the molecules that are effective , or is it their constituent atoms ?
Is the vis viva of the intercepted waves transferred to the molecule as a whole , or to its constituent parts ?
The molecule , as a whole , can only vibrate in virtue of the forces exerted between it and its neighbour molecules .
The intensity of these forces , and consequently the rate of vibration , would , in this case , be a function of the distance between the molecules .
Now the identical absorption of the liquid and of the vaporous nitrite of amyl indicates an identical vibrating period on the part of liquid and vapour , and this , to my mind , amounts to an experimental demonstration that the absorption occurs in the main within the molecule .
For it can hardly be supposed , if the absorption were the act of the molecule as a whole , that it could continue to affect waves of the same period after the substance had passed from the vaporous to the liquid state .
In point of fact the decomposition of the nitrite of amyl is itself to some extent an illustration of this internal molecular absorption ; for were the absorption the act of the molecule as a whole , the relative motions of its constituent atoms would remain unchanged , and there would be no mechanical cause for their separation .
It is probably the synchronism of the vibrations of one portion of the molecule with the incident waves which enables the amplitude of those vibrations to augment until the chain which binds the parts of the molecule together is snapped asunder .
The liquid nitrite of amyl is probably also decomposed by light ; but the reaction , if it exists , is incomparably less rapid and distinct than that of the vapour .
Nitrite of amyl has been subjected to the concentrated solar rays until it boiled , and it has been permitted to continue boiling for a considerable time , without any distinctly apparent change occurring in the liquid * .
I anticipate wide , if not entire , generality for the fact that a liquid land its vapour absorb the same rays .
A cell of liquid chlorine now preparing for me will , I imagine , deprive light more effectually of its power of causing chlorine and hydrogen to combine than any other filter of the luminous rays .
The rays which give chlorine its colour have nothing to do with this combination , those that are absorbed by the chlorine being the really effective rays .
A highly sensitive bulb containing chlorine and hydrogen in the exact proportions necessary for the formation of hydrochloric acid was placed at one end of the experimental tube , the beam of the electric lamp being sent through it from the other .
The bulb did not explode when the tube was filled with chlorine , while the explosion was violent and immediate when the tube was filled with air .
I anticipate for the liquid chlorine an action similar to but still more energetic than that exhibited by the gas .
If this should prove to be the case , it will favour the view that chlorine itself is molecular and not monatomic .
Other cases of this kind I hope , at no distant day , to bring before the Royal Society .
Production of Sky-blue by the decomposition of Nitrite of Amyl .
When the quantity of nitrite vapour is considerable , and the light intense , the chemical action is exceedingly rapid , the particles precipitated being so large as to whiten the luminous beam .
Not so , however , when a well-mixed and highly attenuated vapour fills the experimental tube .
The effect now to be described was obtained in the greatest perfection when the vapour of the nitrite was derived from a residue of the moisture of its liquid , which had been accidentally introduced into the passage through which the dry air flowed into the experimental tube .
In this case the electric beam traversed the tube for several seconds before any action was visible .
Decomposition then visibly commenced , and advanced slowly .
The particles first precipitated were too small to be distinguished by an eye-glass ; and , when the light was very strong , the cloud appeared of a milky blue .
When , on the contrary , the intensity was moderate , the blue was pure and deep .
In Briicke 's important experiments on the blue of the sky and the morning and evening red , pure mastic is dissolved in alcohol , and then dropped into water well stirred .
When the proportion of mastic to alcohol is correct , the resin is precipitated so finely as to elude the highest microscopic power .
By reflected light , such a medium appears bluish , by transmitted light yellowish , which latter colour , by augmenting the quantity of the precipitate , can be caused to pass into orange or red .
But the development of colour in the attenuated nitrite-of-amyl vapour , though admitting of the same explanation , is doubtless more similar to what takes place in our atmosphere .
The blue , moreover , is purer and more sky-like than that obtained from Briicke 's turbid medium .
There could scarcely be a more impressive illustration of Newton 's mode of regarding the generation of the colour of the firmament than that here exhibited ; for never , even in the skies of the Alps , have I seen a richer or a purer blue than that attainable by a suitable disposition of the light falling upon the precipitated vapour .
May not the aqueous vapour of our atmosphere act in a similar manner ?
and may we not fairly refer to liquid particles of infinitesimal size the hues observed by Principal Forbes over the safety-valve of a locomotive , and so skilfully connected by him with the colours of the sky ?
In exhausting the tube containing the mixed air and nitrite-of-amyl vapour , it was difficult to avoid explosions under the pistons of the airpump , similar to those which I have already described as occurring with the vapours of bisulphide of carbon and other substances .
Though the quantity of vapour present in these cases must have been infinitesimal , its explosion was sufficient to destroy the valves of the pump .
Iodide of Allyl ( boiling-point 101 ?
C.).-Among the liquids hitherto subjected to the concentrated electric light , iodide of allyl , in point of rapidity and intensity of action , comes next to the nitrite of amyl .
With the iodide of allyl I have employed both oxygen and hydrogen , as well as air , as a vehicle , and found the effect in all cases substantially the same .
The cloud column here was exquisitely beautiful , but its forms were different from those of the nitrite of amyl .
The whole column revolved round the axis of the decomposing beam ; it was nipped at certain places like an hour-glass , and round the two bells of the glass delicate cloud-filaments twisted themselves in spirals .
It also folded itself into convolutions resembling those of shells .
In certain conditions of the atmosphere in the Alps I have often observed clouds of a special pearly lustre ; when hydrogen was made the vehicle of the iodide-of-allyl vapour a similar lustre was most exquisitely shown .
With a suitable disposition of the light , the purple hue of iodinevapour came out very strongly in the tube .
The remark already made as to the bearing of the decomposition of nitrite of amyl by light on the question of molecular absorption applies here also ; for were the absorption the work of the molecule as a whole , the iodine would not be dislodged from the allyl with which it is combined .
The non-synchronism of iodine with the waves of obscure heat is illustrated by its marvellous transparency to such heat .
May not its synchronism with the waves of light in the present instance be the cause of its divorce from the allyl ?
Further experiments on this point are in preparation .
Iodide of Isopropyl.-The action of light upon the vapour of this liquid is at first more languid than upon iodide of allyl ; indeed many beautiful reactions may be overlooked in consequence of this languor at the commencement .
After some minutes ' exposure , however , clouds begin to form , which grow in density and in beauty as the light continues to act .
In every experiment hitherto made with this substance the column of cloud which filled the experimental tube was divided into two distinct parts near the middle of the tube .
In one experiment a globe of cloud formed at the centre , from which , right and left , issued an axis which united the globe with the two adjacent cylinders .
Both globe and cylinders were animated by a common motion of rotation .
As the action continued , paroxysms of motion were manifested ; the various parts of the cloud would rush through each other with sudden violence .
During these motions beautiful and grotesque cloud-forms were developed .
At some places the nebulous mass would become ribbed so as to resemble the graining of wood ; a longitudinal motion would at times generate in it a series of curved transverse bands , the retarding influence of the sides of the tube causing an appearance resembling , on a small scale , the dirt-bands of the Mer de Glace .
In the anterior portion of the tube those sudden commotions were most intense ; here buds of cloud would sprout forth , and grow in a few seconds into perfect flower-like forms .
The most curious appearance that I noticed was that of a cloud resembling a serpent 's head : it grew rapidly ; a mouth was formed , and from the mouth a cord of cloud resembling a tongue was rapidly discharged .
The cloud of iodide of isopropyl had a character of its own , and differed materially from all others that I had seen .
A gorgeous mauve colour was developed in the last twelve inches of the tube ; the vapour of iodine was present , and it may have been the sky-blue produced by the precipitated particles which , mingling with the purple of the iodine , produced this splendid mauve .
As in all other cases here adduced , the effects were proved to be due to the light ; they never occurred in darkness .
I should like to guard myself against saying more than the facts warrant regarding the chemical effects produced by light in the following three substances ; but the physical appearances are so exceedingly singular that I do not hesitate to describe them .
Ilydrobromic Acid.--The aqueous solution of this acid was placed in a small Woulfe 's flask , and carried into the experimental tube by a current of air .
The tubebeing filled with the mixture of acid , aqueous vapour , and air , the beam was sent through it , the lens at the same time being so placed as to produce a cone of very intense light .
Two minutes elapsed before anything was visible ; but at the end of this time a faint bluish cloud appeared to hang itself on the most concentrated portion of the beam .
Soon afterwards a second cloud was formed five inches further down the experimental tube .
Both clouds were united by a slender cord of cloud of the same bluish tint as themselves .
As the action of the light continued , the first cloud gradually resolved itself into a series of parallel disks of exquisite delicacy ; the disks rotated round an axis perpendicular to their surfaces , and finally they blended together to produce a screw surface with an inclined generatrix .
This surface gradually changed into a filmy funnel , from the end of which the " cord " ) extended to the cloud in advance .
This also underwent modification .
It resolved itself into a series of strata resembling those of the electric discharge .
After a little time , and through changes which it was difficult to follow , both clouds presented the appearance of a series of concentric funnels set one within the other , the interior ones being seen through the spectral walls of the outer ones ; those of the distant cloud resembled claretglasses in shape .
As many as six funnels were thus concentrically set together , the two series being united by the delicate cord of cloud already referred to .
Other cords and slender tubes were afterwards formed , and they coiled themselves in spirals around and along the fuianels .
Rendering the light along the connecting-cord more intense , it diinished in thickness and became whiter ; this was a consequence of the enlargei meant of its particles .
The cord finally disappeared , while the funnels melted into two ghost-like films , shaped like parasols .
The films were barely visible , being of an exceedingly delicate blue tint ; they seemed woven of blue air .
To compare them with cobweb or with gauze would be to liken them to something infinitely grosser than themselves .
In a second trial the result was very much the same .
A cloud which soon assumed the parasol shape was formed in front , and five inches lower down another cloud was formed , in which the funnels already referred to were considerably sharpened .
It was connected as before by a filament with the cloud in front , and it ended in a spear-point -which extended 12 inches further down the tube .
After many changes , the film in front assumed the shape of a bell , to the convex surface of which a hollow cylinder about 2 inches long attached itself .
After some time this cylinder broke away from the bell and formed itself into an iridescent ring , which , without apparent connexion with anything else , rotated on its axis in the middle of the tube .
The inner diameter of this ring was nearly an inch in length , and its outer diameter nearly an inch and a half .
The whole cloud composed of these heterogeneous parts was animated throughout by a motion of rotation .
The rapidity of the rotation could be augmented by intensifying the beam .
The disks , funnels , strata , and convolutions of the cloud exhibited at times diffraction colours , which changed colour with every motion of the observer 's eye .
Moisture appeared to be favourable to the production of these appearances ; and it hence became a question how far they were really produced by the light : hydrobromic acid , even from its solution , fumes when it comes into contact with the aqueous vapour of the air ; its residence in water does not appear to satisfy its appetite for the liquid .
The same effect , as everybody knows , is observed in the solution of hydrochloric acid .
Might not , then , those wonderfully shaped clouds be produced by an action of this kind , the presence of the light being an unnecessary accident ?
The hydrobromic acid was permitted to enter the experimental tube and remain in diffuse daylight for five minutes .
On darkening the room and sending the electric beam through it , the tube was optically empty .
Two minutes ' action of the light caused the clouds to appear , and they afterwards went through the same variety of changes as before .
No matter how long the hydrobromic acid was allowed to remain in the tube , no action occurred until the luminous beam was brought into play .
The tube filled with the mixture of air , aqueous vapour , and hydrobromic acid was permitted to remain for fifteen minutes in the dark .
On sending the beam through the tube it was found optically empty ; but two minutes ' action of the light developed the clouds as before .
Permitting the beam to pass throlgh a layer of water before entering the experimental tube , no diminution of its chemical energy was observed .
Permitting it to pass through a solution of hydrobromic acid , of the same thickness , the chemical energy of the beam was wholly destroyed .
This shows that the vibrations of the dissolved acid are synchronous with those of the gaseous acid , and is a new proof that the constituent atoms of the molecule , and not the molecule itself , is the seat of the absorption .
Hydrochloric Acid.-The aqueous solution of this acid was also employed and treated like the solution of hydrobromic acid .
I intend to invoke the aid of an artistic friend in an effort to reproduce the effects observed during the decomposition , if such it be , of hydrochloric acid by light .
But artistic skill must , I fear , fail to convey a notion of them .
The cloud was of slow growth , requiring 15 or 20 minutes for its full development .
It was then divided into four or five sections , every adjacent two of which were united by a slender axial cord .
Each of these sections possessed an exceedingly complex and ornate structure , exhibiting ribs , spears , funnels , leaves , involved scrolls , and iridescent fleurs-de-lis .
Still the structure of the cloud from beginning to end was perfectly symmetrical ; it was a cloud of revolution , its corresponding points being at equal distances from the axis of the beam .
There are many points of resemblance between the clouds of hydrochloric and hydrobromic acid , and both are perfectly distinct from anything obtainable from the substances previously mentioned ; in fact every liquid appears to have its own special cloud , varying only within narrow limits from a normal type .
The formation of the cloud depends rather upon its own inherent forces than upon the environment .
It is true that , by warming or chilling the experimental tube at certain points , extraordinary flexures and whirlwinds may be produced ; but with a perfectly constant condition of tube , specific differences of cloud-structure are revealed , the peculiarity of each substance stamping itself apparently upon the precipitated vapour derived from its decomposition .
When the beam before entering the experimental tube was sent through a layer of the aqueous acid , thirteen minutes ' exposure produced no action .
A layer of water beMg substituted for the layer of acid , one minute 's exposure sufficed to set up the decomposition .
Hydriodic Acid.-The aqueous solution of this acid was also employed .
On first subjecting it to the action of light no visible effect was produced ; but subsequent trials developed a very extraordinary one .
A family resemblance pervades the nebulae of hydriodic , hydrobromic , and hydrochloric acids .
In all three cases , for example , the action commenced by the formation of two small clouds united by a cord ; it was very slow , and the growth of the cloud in density and beauty very gradual .
The most vivid green and crimson that I have yet observed were exhibited by this substance in the earlier stages of the action .
The de velopment of the cloud was like that of an organism , from a more or less formless mass at the commencement , to a structure of marvellous complexity .
I have seen nothing so astonishing as the effect obtained , on the 28th of October , with hydriodic acid .
The cloud extended for about 18 inches along the tube , and gradually shifted its position from the end nearest the lamp to the most distant end .
The portion quitted by the cloud proper was filled by an amorphous haze , the decomposition which was progressing lower down being here apparently complete .
A spectral cone turned its apex towards the distant end of the tube , and from its circular base filmy drapery seemed to fall .
Placed on the base of the cone was an exquisite vase , from the interior of which sprung another vase of similar shape ; over the edges of these vases fell the faintest clouds , resembling spectral sheets of liquid .
From the centre of the upper vase a straight cord of cloud passed for some distance along the axis of the experimental tube , and at each side of this cord two involved and highly iridescent vortices were generated .
The frontal portion of the cloud , which the cord penetrated , assumed in succession the forms of roses , tulips , and sunflowers .
It also passed through the appearance of a series of beautifully shaped bottles placed one within the other .
Once it presented the shape of a fish , with eyes , gills , and feelers .
The light was suspended for several minutes , and the tube and its cloud permitted to remain undisturbed in darkness .
On re-igniting the lamp , the cloud was seen apparently motionless within the tube ; much of its colour had gone , but its beauty of form was unimpaired .
Many of its parts were calculated to remind one of Gassiot 's discharges ; but in complexity and , indeed , in beauty , the discharges would not bear comparison with these arrangements of cloud .
A friend to whom I showed the cloud likened it to one of those jelly-like marine organisms which a film barely capable of reflecting the light renders visible .
Indeed no other comparison is so suitable ; and nt only did the perfect symmetry of the exterior suggest this idea , but the exquisite casing and folding of film within film suggested the internal economy of a highly complex organism .
The twoness of the animal form was displayed throughout , and no coil , disk , or speck existed on one side of the axis of the tube that had not its exact counterpart at an equal distance on the other .
I looked in wonder at this extraordinary production for nearly two hours * .
The precise conditions necessary to render the production of the effects observed with hydrobromic , hydrochloric , and hydriodic acids a certainty have not yet been determined .
Air , moreover , is the only vehicle which has been employed here .
I hazard no opinion as to the chemical nature of these reactions .
The dry acids , moreover , I have not yet examined .
|
112359 | 3701662 | Account of the Solar Eclipse of 1868, as Seen at Jamkandi in the Bombay Presidency | 103 | 125 | 1,868 | 17 | Proceedings of the Royal Society of London | J. Herschel | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1868.0013 | null | proceedings | 1,860 | 1,850 | 1,800 | 23 | 485 | 11,966 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112359 | 10.1098/rspl.1868.0013 | http://www.jstor.org/stable/112359 | null | null | Astronomy | 29.322792 | Optics | 26.646402 | Astronomy | [
26.34587860107422,
-38.87509536743164
] | " On the Physical Constitution of the Sun and Stars .
" By G. JOHNSTONE STONY , M.A. , F.R.S. , F.R.A.S. , Secretary to the Queen 's University in Ireland .
Received May 15 , 1867 .
( See page 1 .
) I. " Second List of Nebulae and Clusters observed at Bangalore with the Royal Society 's Spectroscope ; " preceded by a Letter to Professor G. G. Stokes .
By Lieut. JOHN HERSCHEL , R.E. Communicated by Prof. STOKES .
Received July 20 , 1868 .
( See page 58 .
) II .
" On the Lightning Spectrum .
" By Lieut. JOHN HERSCHEL , R.E. Communicated by Prof. STOKES .
Received August 8 , 1868 .
( See page 61 .
) III .
" Products of the Destructive Distillation of the Sulphobenzolates."-No .
II .
By JOHN STENHOUSE , LL. D. , F.R.S. , &c. Received September 8 , 1868 .
( See page 62 .
) IV .
" Compounds Isomeric with the Sulphocyanic Ethers.-II .
Homologues and Analogues of Ethylic Mustard-oil .
" By A. W. HOFMANN , Ph. D. , M.D. , LL. D. Received September 11 , 1868 .
( See page 67 .
) V. " Account of Spectroscopic Observations of the Eclipse of the Sun , August 18 , 1868 .
" In a Letter addressed to the President of the Royal Society by Captain C. T. HAIG , R.E. Communicated by the President .
Received September 21 , 1868 .
( See page 74 .
) VI .
" Account of Observations of the Total Eclipse of the Sun , made August 18th , 1868 , along the coast of Borneo .
" In a Letter addressed to H.M. Secretary of State for Foreign Affairs , by HIis Excellency J. POPE HENNESSY , Governor of Labuan .
Corn municated by the Right Hon. Lord STANLEY , F.R.S. Received October 8 , 1868 .
( See page 81 .
) VII .
" Further Particulars of the Swedish Arctic Expedition .
" In a Letter addressed to the President , by Professor NORDENSKIOLD .
Communicated by the President .
Received October 15 , 1868 .
( See page 91 .
) VIII .
" Notice of an Observation of the Spectrum of a Solar Prominence .
" By J. N. LOCIYER , Esq. , in a Letter to the Secretary .
Communicated by Dr. SHARPEY .
Received October 21 , 1868 .
( See page 91 .
) IX .
" On a New Series of Chemical Reactions produced by Light .
" By JOHN TYNDALL , LL. D. , F.R.S. , & c , Received October 24 , 1868 .
( See page 92 .
) X. " Account of the Solar Eclipse of 1868 , as seen at Jamkandi in the Bombay Presidency .
" By Lieut. J. HERSCHEL , R.E. Communicated by Prof. G , G. STOKES , Sec. R.S. Received October 19 , 1868 , To the President , Council , and Fellows of the Royal Society .
GENTLEMEN , -The time has arrived when I must offer for your acceptance a connected report of the employment of the instruments entrusted to me for the special purpose of observing the late solar eclipse .
1 .
Plan of this Report .
In framing this Report I propose in the first place to describe those instruments sufficiently in detail to render unnecessary such explanations as would otherwise be required in the course of my narrative , and then to show the circumstances which preceded their actual employment on that occasion .
2 .
Description of Telescope and clockwork .
The principal instrument is an equatorially mounted telescope , with a lens of 5 inches aperture and 62 inches focal length .
The mounting is adapted to any latitude ( except very low and very high ones ) , the polar axis being a moveable tangent to the circular-arched roof of the chamber containing the clockwork .
The latter , as well as the rest of the instrument , is by Messrs. Cooke and Sons , of York , and is , as I understood from Mr. Cooke , of a somewhat novel description .
I have not examined the mechanism closely , and therefore cannot describe itvery accurately ; but I believe the peculiarity consists in the maintenance of continuous motion in a fan-wheel , regulated by a pendulum time-keeper acted on through a remontoir escapement , whereby the irregularity of the surplus energy of the driving-weight , while it is prevented by the latter from interfering with the time-keeper at all , is modifed in its action on the tube by the former .
The mean rate of motion is 104 [ Nov. 19 , thus uniform ; and though there is very perceptible irregularity in the actual motion , it is not intermittent .
Thus , when the image of a star , for instance , is brought on the slit of the spectrum-apparatus , the spectrum is fitful in appearance , if the slit is perpendicular to the direction of diurnal motion .
The mean motion may be easily regulated as in a pendulum-clock .
The motion is communicated by friction to the first of a series of wheels which terminates in an endless screw working in the circumference of a large toothed arc attached to the hour-axis .
Motion imparted by hand to one of these wheels , grooved and provided for this purpose with an endless cord , is thus communicated directly to the tube without greater strain on the clock than is implied in overcoming the connecting friction .
3 .
Its MIounting .
The declination-axis terminates in a T-shaped head carrying two circular collars , in which the telescope-tube rests .
For convenience in mounting and dismounting , these collars are attached to the T-head by nut and pins , so that they lift off with the tube , while the balance can be adjusted by releasing their grasp of the tube when required .
This is a great convenience in a portable instrument .
The tube can be dismouinted and taken indoors readily without assistance ; and the body of the instrument ( which , besides being far less easily handled , has cost hours of adjustment ) may be left under a suitable waterproof case when no observatory has been constructed .
4 .
Its Stand .
The stand is a strong wooden one , of remarkably firm construction , considering that it is of the three-legged portable kind .
Its upper surface is a stout brass annulus , on which the clock-chamber rests and rotates , if required , for adjustment in azimuth .
Two of the legs have foot-screws for adjusting the level and completing the adjustment for latitude .
5 .
Of the Sectroscope .
The spectroscope intended for use with the above telescope was constructed by Messrs. Simms , on a pattern or design supplied ( I believe ) by Mr. Huggins ; but its construction was too much delayed to allow of a practical examination of all its parts before packing .
It consists of a single flint-glass prism , of refracting angle 60 ?
, contained in a cylindrical brass chamber , from which radiate three tubes in such directions as to fulfil the several purposes of ( 1 ) receiving the light to be analyzed , ( 2 ) delivering it after refraction and separation to the eye , and ( 3 ) admitting external light for reflection to the eye off the second surface of the prism .
The first consists externally of a long connecting tube for insertion into the telescope in place of the ordinary eye-tube , where it is grasped in the focusing-slide .
Internally it carries a smaller tube , carrying at one end a lens , and at the other , at the principal focal distance of the latter , a beautiful piece of workmanship by which a slit is obtained whose sides i2 1868 .
] approach each other equally .
Half the length of this slit may be obscured by the intervention of a right-angled prism , which reflects a side light through it if required .
The converging rays from the object-glass falling on the slit are admitted , while those which do not are stopped .
The former diverging again , as though from a luminous line , emerge from the next lens and fall on the prism as parallel rays , are independently refracted and dispersed in traversing it , and after emergence are again condensed , but not reunited , by the object-glass in the small telescope composing the second of the above-mentioned tubes , and , forming a spectrum in its focus , are viewed as such by an eyepiece .
Mleans of measurement.--The direction of emergence defines the position in the spectrum ; and the difference of direction is measured by the change of direction of the small telescope necessary to receive the several refracted rays directly .
This change of direction is effected and measured by a tangent screw , whose complete revolutions are indicated by the march of a graduated scale ( attached to the telescope-arm ) over a circle marked on the circumference of the divided cylindrical head of the screw .
The position of the centre of motion of the telescope-arms , it should be said , though optically unimportant , is practically within the prism .
By the help of a reading-lens the revolutions , and tenths and hundredths of a revolution , can be easily read off by a very slight movement of the eye from the eyepiece .
New graduated Scale for micrometer measures.-A mistake having occurred in graduating the scale , I substituted one of my own making .
As I was fortunate in this , I may venture to describe how it was effected .
The graduation required was too fine for any ink lines I could make ; I therefore varnished a piece of card , and drew fine lines at the proper intervals on the shellac-coating with a sharp blade ; and applying a little ink , these were instantly rendered visible .
I then cut the card across the lines and glued the scale so formed over the old one with varnish , giving the whole a dash of varnish for the sake of protection .
When dry I was gratified to find the graduation correspond well with the revolutions ; for it was rather a delicate job , and I did not succeed without failures .
6 .
Graduated Scale in the Field of View .
The third tube was intended to present in the field of view of the telescope last described , by external reflection off the second surface of the prisr , an illuminated image of a photographed scale placed at one end of the tube , in the principal focus of a lens at the other .
The tube carries a small moveable mirror outside .
Upon this mirror was intended to be thrown the light of a small lamp , held n position by a bent arm projecting from the prism-chamber .
I am sorry to say that this ingenious contrivance proved , in my hands , more unsatisfactory than perhaps it should have done .
As in not using it I departed from the letter of my instructions , I am in a measure bound to explain my reasons for discarding it .
Reasonsfor discarding it .
In the first place , I never could with any kind of illumination train my eye to read the scale , partly because ( whether from diffraction or irradiation ) the image was never distinct , partly because the figures were illegible .
In the next place the little lamp was capricious ; either it refused to keep alight , or it boiled its own oil and melted off its handles , and ended by burning my fingers !
Thirdly , it was an additional weight at the eye-end of the telescope and involved a counterpoise when not in use , and an additional projection to be avoided in every movement in the dark , -all implying additional distractions and sources of failure .
Lastly , I found I could do very well without it-in the preliminary training which I underwent on examining the nebulae .
At the same time I must confess that I made an oversight in trusting too much to the illuminating power of a hand-lamp , as will be apparent when I come to describe the actual eclipse-observations .
7 .
Smaller Telescopes and Polarizers .
The second instrument supplied was an achromatic refractor of 3 inches aperture mounted with vertical and horizontal axes , the socket of the former being supported on a three-legged wooden stand , afterwards replaced by one of greater stability and more convenient height .
Two cells , containing a double-image prism and quartz plate , and the combination known as Savart 's polariscope , respectively , were supplied for use with this telescope , but without any connecting adaptation .
8 .
Hand Spectroscopes .
The other instruments were hand spectroscopes for direct vision , four in number , which I was directed to distribute according to circumstances , It is needless to describe these instruments , as they are well known ; but I must venture to correct a statement made at a meeting of the Royal Asiatic Society last December , that they have a magnifying-power of 8 or 10 .
I do n't think they can be credited with a higher power than 3 ; and I was never able to recognize any of the peculiar characteristics of nebular or stellar spectra , the recognition of which might have been expected with the higher magnifying-power .
9 .
Arrival in India and communication with Colonel Walker , R.E. Soon after my arrival in India I communicated with Colonel Walker , with the object of receiving his instructions and of ascertaining whether hie had decided on any plan , and , if not , to learn his views with reference to the assistance I might expect from the Survey Establishment .
The choice of a station of observation and the disposal of the instruments were also discussed in the course of correspondence .
10 .
His Reply , and application to the Indian Government .
Colonel Walker 's action in this matter has been most gratifying .
He immediately promised me the assistance of Lieut. W. Maxwell CampbelI , of the Bombay Engineers , one of the executive officers of our Department , at that time engaged with myself and others in measuring a base-line in the neighbourhood of Bangalore , for the polarization-observations or otherwise , as I might arrange with him .
He also placed at my future disposal forth occasion the services of Lieut. Campbell 's assistants , in case such should be required , at the same time presenting to the Indian Government an urgent proposal to give the Royal Society 's expedition both countenance and support .
I enclose a copy of the reply to this proposal , in which it will be observed that the Governor General in Council " cordially approves , " and " sanctions the necessary expenditure , " and pledges the Government " to do everything in its power towards securing fill and accurate observations " on the occasion-a pledge fully redeemed by the ready assent given to more than one other application .
I am accordingly enabled to submit to your Society my present Report unaccompanied by any further appeal to your Treasurer .
11 .
Step-s taken to procure local information as to weather c. The local Governments were also applied to to give effect to the circulation of a series of queries calculated to elicit local information as to probable climate at numerous points situated along the line of shadow .
This was the more necessary , as my position at Bangalore ( in the very centre of the peninsula ) seemed to give a so much greater range of choice .
In this respect also a warm interest was evinced .
I wish I could add that the mass of correspondence which resulted was productive of an equal amount of valuable information .
The practical value was chiefly confined to extracts from rain-registers , the principal question relating to probable cloudiness or otherwise being perhaps necessarily replied to too vaguely to form legitimate grounds for decision , owing in great measure to the fact that August is one of the most uncertain months in the year , in that respect , in southern India .
Rough notion of rain distribution across the peninsula in August.-On the whole , however , it appeared that across the whole width of the peninsula cloudy weather was to be expected at that season ; and there was therefore no choice but what could be based on rainfall .
The annexed diagram represents the impression ( necessarily a vague one ) remaining on my mind after considering the reports .
On the west coast anything up to 25 inches a week has been recorded in August ; on the eastern slopes of the western Ghauts the fall seems both smaller and more regular , 6 to 10 inches being the usual fall in the month of August .
Further inland we come to a tract notorious for its dryness , several places , such as Gokak , Jamkandi , Bejapuir , and others thereabouts , being favoured with occasional showers only .
I attributed this to the descent into a lower and hotter region of the prevailing south-west current , the greater part of whose moisture had been deposited during the disturbance of strata caused by passing over the sudden barrier of the Ghauts .
Beyond this again , eastwards , their is a gradual rise in the amount due in August , until towards the east coast the average fall is again 6 or 8 inches .
12 .
Jamkandi selected .
Jamkandi , the residence of a native chief , was among the first to attract my attention , partly owing to the offers of assistance which were made in the name of the chief ; and this place was eventually selected for the advantages of climate which it appeared to offer .
13 .
Distribution of the Instruments .
Lieut. Campbell , R.E. In the meantime the distribution of the instruments was attended to .
The smaller telescope with polarizing eyepieces was made over to Lieut. Campbell with a copy of the " Instructions , " in the full assurance that he would acquaint himself with the theory and practice necessary to turn them to account .
I annex a copy of his Report , the perusal of which will show that the instrument was in good hands .
It is much to be regretted that he was not permitted to give more practical evidence of the forethought which characterized his prepaA rations .
I am also sorry that he has not given a fullerdescription of the ingenious contrivance which he designed and constructed for the ready application of the analyzers to the eyepiece .
The annexed rough sketch ( from memory ) mayhelp to give a correct idea of the contrivance .
I apprehend that in the event of fair weather he would be able to settle the question of polarity readily , and would have leisure to make use of a hand spectroscope as well .
One of these instruments also was therefore made over to him .
14 .
Captain Itaig , R.E. Colonel Walker had further consented to allow another of our executive officers ( Captain Haig , R.E. ) to leave his regular duties for a time if he wished .
As he was stationed at Poona and could avail himself of the railway as far as the border of the shadow 's path , I offered him , and he accepted , the charge of another of the hand spectroscopes .
Peninsular and Oriental Steam Navigation Company 's Agent , Captain Henry , Superintendent at Bombay .
Lastly , I communicated with the agents of the Peninsular and Oriental Company at Calcutta and Madras Bay , and eventually entrusted the remaining two spectroscopes to the latter for employment on board two vessels , outwardand homeward-bound , which would probably be on the track at the right time .
16 .
Memorandum of explanations and suggestions for use of Hand Spectroscopes .
It was necessary , however , not only to distribute these instruments , but also to provide for their being intelligently employed in unpractised hands .
I accordingly drew up a short memorandum with the object of putting it into the power of those interested to understand as much of the subject as seemed necessary , and of suggesting the probable appearances which might be presented .
A copy of the pamphlet accompanies this Report .
1 7 .
Examination of Nebul & e as bearing on the main subject .
While these arrangements were in progress I was myself engaged with the equatorial in the examination of the southern nebulae , to which I devoted as much time as the duties of my profession enabled me to do .
The weather was very favourable in March ( towards the middle of which month the base-line was completed ) , in April , and until the middle of May ; but from that time until the latter end of June , when the instrument had to be despatched , I hardly got a single observation , owing to the setting-in of the south-west monsoon .
I congratulated myself on having been able to use the fine nights we had had .
The results , showing the nature of the spectra of about fifty nebulae , have been already communicated to your Secretary ; there is therefore no occasion to enter into particulars on this subject here , except as bearing on instrumental peculiarities not previously touched upon , and as suggesting the probability that a considerable familiarity with the special kind of observation had been acquired , as well as with the individual instrument .
Those who are acquainted with the spectroscope as applied to a telescope will remember that it involves several additional screws to be attended to , and that the finding of these mechanically in the dark is no inconsiderable perplexity until habit has taught the way .
But this by the way .
18 .
The Finder , and the trouble it gave .
The finder attached to the telescope has a very low magnifying-power and decidedly bad definition-so much so that even Saturn can scarcely be recognized with it ; none but the most conspicuous nebulae and clusters are visible ; I have looked in vain for the planetary nebula in Lyra with it , though it was certainly in the field ; and of all the planetary nebulae in the southern hemisphere , only two ( Nos. 2102 & 4510 ) are noted by me as " visible in finder .
" It was therefore almost always necessary to find with the principal , by the setting ; and afterwards either to exchange the light eyepiece for the heavy spectroscope ( removing at the same time a counterpoise ) without disturbing the direction , if possible , or to take the bearings of the most conspicuous stars visible in the finder .
But as there never was and never could be any certainty that in the act of insertion a disturbance sufficient to displace the image from the position the slit should occupy would not take place , the latter method became the surest , if the most troublesome .
[ The connecting-tube , I should remark , cost me , literally , days of worry and grinding before I could induce it to slide in and out at all .
] If after these precautions the result of a blind search was negative , the whole had to be done de novo .
What with removing and replacing the spectroscope , inserting eyepieces and 'counterpoises , setting the readings , searching in both finder and telescope , winding the driving-clock over and over again , in endless combination , all by the light of a bull's-eye lantern , perhaps without catching a single spectrum all night , I often found four or five hours ' observing ( ?
) more fatiguing than a long walk .
It may appear strange that I did not replace the finder by a better telescope .
I can only say that India is not England , and Bangalore is not London .
The idea did not occur to me as a practical one , and I was nervously afraid of making any alteration which might leave me worse off than I was .
A bad finder was after all no great matter , for the eclipse and the nebule could wait .
At the same time I wish now that my finder had been more serviceable as a telescope for I got ; but a poor sight of the eclipse with it .
19 .
Further preparations , Observatory , yc .
To return to my preparations .
In the utter absence of any precise knowledge of the appearances which would be presented , but anticipating a faint spectrum as the most probable , all my preliminary arrangements had in view as complete an exclusion of external light as practicable .
A wooden frame was constructed for an observatory with a revolving roof , the latter being covered with painted canvas .
A large black curtain was provided , through the centre of which were to be passed the observing-end of the telescope and finder , and the declination-clamp and slow-motion screw .
A segment of the octagonal observing-chamber would thus be in a great measure protected from the light which might be expected to enter the limited aperture in the roof .
20 .
The Expedition leaves Bangalore .
The instruments , observatory , and camp-equipage started from Bangalore on the 7th of July , and reached on the 7th of August-a creditable march of 390 miles in 31 days ( including halts ) in the height of the rainy season .
My subsequent experience of the state to which so-called " made " roads may be reduced , in these parts of India , by a few days ' rain , afforded grounds for self-congratulation that the journey was accomplished as quickly as it was .
I followed on the 1st of August , and reached Jamkandi on the morning of the 14th .
The journey was so exceedingly disagreeable a one that I shall say no more about it .
21 .
Arrival at Jamkandi .
By the evening of the 14th the observatory was put together and the telescope &c. ready for adjustment .
22 .
Prospects .
I was surprised and considerably disappointed to learn that the weather had been for some days past as cloudy as I found it .
I had left heavy rain behind me at Belgaum , and found none at Jamkandi certainly ; but the sky was thick with passing cloud .
I was told that it was quite unusual , and that it could not last ; but by the morning of the 18th both Lieut. Campbell and myself had made up our minds not to be disappointed ( if we could help it ) , should we be denied more than a few glimpses .
23 .
Bad weather not unusual at this season .
I learned afterwards that at some time or other at that season a burst usually takes place on the Ghauts , causing a sudden and violent flood in all the rivers , and that the influence of this extends beyond their limits and occasions the fortnight of cloudy skies and scanty rainfall which such places as Jamkandi enjoy once a year .
This periodical flood had occurred between the time of our camp 's and our own arrival ; and we were now experiencing the cloudy season .
It was very unfortunate , but could hardly have been foreseen .
Not only our own party , but others in the neighbouring district of Bejapiur were unlucky .
Three days later the whole aspect of the country was changed .
The rivers subsided ; the heat which we had expected , but missed , began to make itself felt ; the villainous black soil hardened ; and the natives said confidently that their rainy season was past , and that the rivers would not rise again till next year .
24 .
Lieut. Campbell 's Station .
On the 17th Lieut. Campbell selected his position on a hill about a mile distant .
We had agreed that the character of the clouds was such that a greater separation was unnecessary , owing to their uniform distribution and regular current .
25 .
Final preparations .
I come at length to the more interesting part of my narrative .
The three days and nights which preceded the event were occupied in adjusting the polar axis , in examining every adjustment that could or could not require it , in exchanging the broad coarse pointer which I had used for night work for a stout but sharp needle , in going over and over again a mental review of the probable appearances and the possible contingencies which might arise .
The three months ' disuse , too , since I had to give up the nebulre , made fresh exercise necessary .
Among other things , I concluded not to alter the pendulum , long ago adjusted for sidereal time .
The difference of rate being only 1 in 365 for mean time ( and 1 in 388 for solar time at that date ) , the telescope would only gain on the sun by less than one second during the 5 ' minutes of totality ; so that even supposing I should wish to keep it directed on one and the same point the whole time , the practical effect would only be that that point would move along the slit by perhaps I5 part of its visible length ( estimating that length , or the width of the field , at 5 ' ) .
I mention this as the " Instructions " direct the adjustment to apparent solar time .
26 .
Disuse of the Barlow Lens accountedfor .
In one other respect , too , I must plead guilty to a departure from the letter of those instructions , which hardly perhaps needs justification ; I allude to the disuse of the Barlow lens .
My reason was principally this , that its insertion keeps the observer some 6 inches further from the body of the instrument , and , besides involving a complete disturbance of equilibrium , puts him out of reach of the declination screwresults which I could not but think had not been contemplated .
I should add that I was quite confident of the practicability of catching a prominence , without having its image doubled in size , though I was by no means so sure that I could spare any of the light , which would be reduced one-fourth .
27 .
Care in adjusting the Pointer during the approach of the Moon .
During the advance of the moon , and up to the last available moment , I paid particular attention to the collimation ( I use the word in its true sense of aim ) of the needle-point , being perhaps unnecessarily anxious to avoid my old difficulty of finding my object in the spectroscope .
The sharp cusps were well suited to this purpose , and the sun-spots were good tests .
I had been fortunate in getting the pointer very exact , and was therefore not troubled with any collimation-error to allow for .
28 .
Spectrum at the Moon 's centre .
While thus employed I had occasion to remark that at the centre of the moon , some nine or ten minutes before totality , the intensity of the solar spectrum was much about the same as that of the fuill moon .
29 .
Measurement of Solar Lines .
Intensity of Spectrum of Limb at D.-The principal solar lines were measured at intervals during the advancing eclipse .
A few minutes before totality , in going over these lines for the last time , the slit being as wide as was allowable for full sunlight , i. e. very narrow , I recorded an increasing brilliancy in the spectrum in the neighbourhood of D , so great in fact as to prevent any measurement of that line till an opportune cloud moderated the light .
I am not prepared to offer any explanation of this .
The clouds were arranged in two distinct strata , the lower one containing masses hurrying past with the monsoon-current at no great height , the upper consisting of light , thinly scattered cirri showing very little motion .
It is conceivable that the latter may have been obstinately interposed until the time when I remarked the recorded brilliancy ; but I cannot say that I should be satisfied with such an explanation .
Whiteness of the Crescent.-I also remarked that the whiteness of the crescent , as seen in the finder , was apparently intensified as it grew narrower .
Possibly this was the effect of contrast with the darkening background ; for at this time I began to be annoyed by the appearance of five or six phantom crescents , which seemed to be trying to rival the legitimate one .
I imagine I was indebted to the dark glass for these apparitions ; but whatever called them up , they most effectually confused the view of the closing scene ; whatever might otherwise have been seen at this stage was swamped in the confusion .
30 .
Restlessness during afpproach of shadow .
Up to within about ten minutes of totality I was every now and then outside watching progress through one or the other of two smaller telescopes of moderate power , one of which I had borrowed from the chief , who indulges a taste for the possession of English manufactures to an extraordinary degree .
I noticed no marked inequalities of surface in the advancing limb , nor any bluntness of the cusps ; but I must allow that I was not in a sufficiently composed state of mind to observe critically anything not bearing directly on the special problem before me .
I was impressed with a notion that everything must be subordinated , in my case , to the requisite freedom of attention when totality commenced , and was specially anxious to save my eyesight .
I studiously avoided looking at the sun except under cover of a cloud ; and though I had provided the telescopes with graduated smoked glasses , I was nervously afraid to look through them too long or too intently-all which can only be understood by referring to what has been said about the absence of any foreknowledge of the impending revelation .
My last view of external appearances showed nothing very striking-a few deeply neutral-tinted patches of sky in the zenith , and an increasing gloominess in all directions , being all the phenomena whose impression has outlived the excitement of the shortlived minutes which ensued .
I reentered the observatory , and retired behind my black curtain to watch the event .
31 .
Gentlemen , I have thus far endeavoured to lay before you , as far as possible , in an orderly manner , an outline of the preliminary arrangements for the employment of your Society 's instruments , and a sketch of my proceedings up to the hour of the eclipse .
If in so doing I have been unnecessarily tedious , I would ask you to remember that these few pages but faintly represent the months of anxious study and preparation which have passed since I accepted the responsibility involved in the charge of an ex pedition deputed by the illustrious body I have now the honour of addressing-a responsibility more engrossing , it may be , but not lessened , by the specific but novel character of the proposed object of the expedition .
I proceed now to describe how far that object has been attained ; and here I feel that I cannot well indulge in too great a minuteness of detail .
32 .
Relative positions of Pointer , Slit , and Sun 's Limb .
The spectroscope may be inserted , and employed with its slit in any direction perpendicular to the optical axis of the telescope .
It is therefore competent to the observer to place the slit perpendicular or tangential to the sun 's circumference at any point ; and there can be no doubt that , were the observations conducted at leisure , it would be desirable to examine the whole circumference in both positions ; but the operation of turning the spectroscope is not so very simple a one but that the advantages and disadvantages of any such proceeding require to be well considered where time is of the first importance .
I decided on employing the slit in one direction only , that which corresponded with the diurnal motion .
It so happened that this corresponded nearly with the direction of the relative motion of the sun and moon , so that the widest part of the crescent could be made to fall nearly perpendicularly across the slit .
The needle ( in the finder ) and its point accurately represented the direction and centre respectively of the slit ; therefore , when the needle-point touched the sun 's limb at the centre of the crescent , a solar spectrum of definite width appeared in the field , of which one edge ( the right-hand ) continued stationary , while the other ( the left ) advanced slowly but perceptibly towards it , the solar spectrum decreasing visibly in width .
33 .
Last view of Solar Spectrum .
About a minute 's breadth remained .
A few seconds more and it would vanish suddenly .
Whatever spectrum the corona could show must then be revealed , unless indeed a " prominence " or " sierra " should happen to be situated at that precisespot , in which case the double spectrum should be presented .
The nervous tension at the moment may be conceived : what would be seen ?
what call for action would be made ?
and for what action ?
or , if nothing were seen , what would have to be done ?
I cannot say that I was prepared , at that moment , either with these questions , or with ready answers to them ; but that was the sensation .
With regard to the last , I suppose I should have instinctively widened the slit ; and had that failed , should then have gone to the finder to look for a prominence .
As it was , the spectrum faded out as I looked , while it had still appreciable width , and I knew a cloud had intervened .
Totality commences unseen.-A few seconds more and the spectrum of diffuse light vanished also , and told me the eclipse was total , but behind a cloud .
34 .
On the watch for a glimpse .
I went to the finder , removed the dark glass , and waited ; how long , cannot say ; perhaps half a minute .
Soon the cloud hurried over ; following the moon 's direction , and therefore revealing first the upper limb , with its scintillating corona , and then the lower .
A prominence seen and aimed at.-Instantly I marked a prominence near the needle-point , an object so conspicuous that I felt there was no need to take any precautions to secure identification .
It was a long finger-like projection from the ( real ) lower left-hand portion of the circumference .
A rapid turn of the declination-screw covered it with the needlepoint , and in another instant I was at the spectroscope .
A single glance and the problem was solved .
Its Spectrum.-THREE VIVID LINES , RED , ORANGE , BLUE ; NO OTHERS , AND NO TRACE OF A CONTINUOUS SPECTRUM .
35 .
Measurement of lines undertaken , with partial success .
When I say the problem was solved , I am of course using language suited only to the excitement of the moment !
It was still very far from solved , and I lost no time in applying myself to measurement .
And here I hesitate ; for the measurement was not effected with anything like the ease and certainty which ought to have been exhibited .
Much may be attributed to haste and unsteadiness of hand , still more to the natural difficulty of measuring intermittent glimpses ; but I am bound to confess that these causes were supplemented by a failure less excusable .
I have no idea how those five minutes passed so quickly !
Clouds were evidently passing continually ; for the lines were only visible at intervals-not for onehalf the time , certainly-and not always bright ; but still I ought to have measured them all .
My failure was in insufficient illuminating power ; but why , I cannot tell .
I never experienced any difficulty of the kind with the nebulae , which required that I should flash in light suddenly over and over again .
I had found the hand-lamp the surest way ; but it failed me here in great measure .
The red line must have been less vivid than the orange ; for after a short attempt to measure it , I passed on to secure the latter .
Two lines measured .
In this I succeeded to my satisfaction , and accordingly tried for the blue line .
Here I was not so successful .
The glimpses of light were rarer and feebler , the line itself growing shorter and , what remained of it , further from the cross .
I did , however , place the cross wires in a position certainly very near the true one , and got a reading before the reillumination of the field told me that the sun had reappeared on the other limb .
These readings were called out , as those of the solar lines had been , to my recorder ; and it was only afterwards that I compared them .
I need not dwell on the feelings of distress and disappointment which I experienced on realizing the fact that the long-anticipated opportunity was gone , and , as it seemed to me then , wasted .
I seemed to have failed entirely .
Almost mechanically I directed the telescope to the bright limb , to verify the readings of the solar lines ; and in so doing my interest was again awakened by the near coincidence , as it seemed , of the line F with the position of the wires ; but a little reflection convinced me that the distance of the former was greater than the error which I might have made in intersecting the blue line .
Their readings and those of the solar lines.-I read F , and then D & C. The following were my readings up and dowrn : C. D. b. F. ( 191 2'96 4-58 5-64 91 90 2-94 4-56 5 ' 61 Before .
193 2-98 4-60 5 ' 65 1-92 2-97 4-58 5-62 Bright lines ... [ 300 ] ... [ 5-56 ] After ... 1-93 3-00 ... 5-65 36 .
Identity of the Orange Line .
I consider that there can be no question that the ORANGE LINE was identical with D , so far as the capacity of the instrument to establish any such identity is concerned .
37 .
Of the Blue Line : doubtful .
I also consider that the identity of the BLUE line with F is not established ; on the contrary , I believe that the former is less refracted than F , but not much .
38 .
Of the Red Line : uncertain .
With regard to the RED line , I hesitate very much in assigning an approximate place : B and C represent the limits ; it might have been near C ; I doubt its being so far as B ; I am not prepared to hazard any more definite opinion about it .
Its colour was a bright red .
This estimate of its place is absolutely free from any reference to the origin of the lines C and F. 39 .
Subsequent mental aberration : not unusual .
It is a fact not unworthy of notice that in all the accounts of eclipses , written soon after the event , which I have read , the record hurries rapidly to a close after the sun has reappeared ; the reason , no doubt , is that a reaction takes place after the excitement of witnessing the actual eclipse , and phenomena which might be noticed after , quite as well as before , pass unregarded on that account .
For my part I was surprised to find how utterly indifferent I felt to the appearance of things when I came out of my observatory .
I am almost ashamed to confess that I went straight to my tent , and tried to write down what I had seen , instead of going to the telescope to watch for what still might be seen .
It never even occurred to me to remove the spectroscope and use the fine telescope I had at command .
40 .
Afterconsideration of the phenomena witnessed .
I have not quite exhausted the statement of my observations , though what I have still to state was rather the result of subsequent reflection than of actual cognisance at the time .
I said that the prominence was situated close to the needle-point .
I estimate its position as at the east point , a few degrees to the left of the lowest , of the sun 's limb .
Its form was that of a projecting finger slightly curved to the southward , and its height nearly 2 ' .
The slit was at right angles to the hour-circle , and therefore perpendicular to the sun 's limb at this point .
A vertical section ( so to speak ) of the prominence was therefore admitted through the slit .
It appears , then , that the length of the lines corresponded with the height of the prominence , being limited ( as in the case of the spectrum of the section of the crescent ) on the one hand ( the left ) by the advancing moon 's limb at the centre of the field , and on the other by the natural summit of the prominence , or flame , as we are now entitled to call it .
Spectrum of Corona not seen.-Beyond this summit the light of the corona was free to enter ; it was also free to enter with that of the flame ; but I saw the spectrum of the latter only .
I thence conclude that the spectrum of the corona was a faint solar one , --a conclusion quite in accordance with the other characteristics of this phenomenon , such as the radiated appearance and the evidence from polarity , indicating a central source of light .
With regard to the latter , it is clear that the light of the corona is polarized in planes passing through the sun 's centre ( as the gist of Lieut. Campbell 's Report ) , and therefore that the corona shines mainly by reflected light .
At the same time it is possible that the absence of a spectrum of the corona at this particular spot may have been accidental .
I have since heard that the corona was particularly feeble at this point .
I had no opportunity of studying the corona myself .
After first catching sight of the eclipse in the finder , I never left the spectroscope but once , when a long interval of cloudiness sent me to the finder to make sure .
I then caught a few seconds ' glimpse again , and remarked a red blot ( I recognized no shape ) of a prominence at about the north point , or rather to the west of it .
41 .
Remarks on the ease with which the lines might be measured , and suggestions for future observations .
I have now a few remarks to add which may be of use to future observers , if not of any present value .
It is difficult to say what might or might not have been done but for the clouds ; but I am pretty certain that ( even labouring , as I was , under the difficulty of bad illumination ) not only might all three lines have been satisfactorily measured , but time would have sufficed for further examination .
The course which that examination should take is a question which it is of the highest importance for an observer to decide on previously .
I believe I was right in using a narrow slit to begin with , not anticipating such a totally darkfield ; but I should not do so again ; or if I did , with the object of getting exact measures of the three principal lines , I should be prepared to widen the slit to look for faint ones , the positions of which I should estimate with reference to those three .
I should then direct the telescope at the brightest part of the corona , taking very good care to prefer a part free from any appearance of sierra , and if possible near the east or west points , so that the slit might admit a vertical section .
Assuming that the corona does not emit tosochromatic light -if I may be allowed to coin a word to indicate definite but unspecified colours , both in respect of number and tint ( or pitch)-of very distinct character , the spectrum of such a vertical slice might indicate by its varying width that the light was not uriformlly constituted .
Another point to be ascertained is whether all flarnes are constituted alike .
This would require a more or less rapid glance at the spectra of several .
I have spoken of " the three principal lines " because I saw no others .
I have , however , heard rumours of a greater number having been seen by other observers , whether of equal brilliancy or not I do not know ; but it inclines me to enforce the statement I have already made of " three vivid lines-no more , " as seen with a narrow slit .
I had no suspicion whatever of the presence of any but those three ; and as I first saw them they were as sharp and bright as one could well wish to see .
Whether the prominence which I looked at was the same as those in which more than three lines were seen I do not know .
42 .
Lieut. Campbell 's Observations satisfactory in their result .
The determination of the polarization-plane of the corona is as satisfactory as can be desired , and Lieut. Campbell 's account is so clear that I have little to say about it .
It is to be regretted that he did not see the effect of polarization all round at the same time , with a power low enough to include the whole of the phenomena ; but the view fortunately obtained with the higher power remedies this in great measure by showing what would have been seen at points 90 ?
distant from that which he describes .
43 .
Results with Hand Spectroscopes unknown .
With regard to the hand spectroscopes I have scarcely any report to make .
Lieut. Campbell had no opportunity .
Capt. Haig has sent no report .
Neither have I heard anything of one of the two sent to sea .
The only record I have received is that of Capt. Rennoldson , of the 'Rangoon , ' P. & 0 .
Co. 's Steam Ship , which I enclose .
He mentions having seen with the spectroscope a prominence not seen by others with ( I presume ) ships ' glasses of greater power .
This is difficult to understand , except on the supposition that the light of the corona was weakened by dispersion , while that of the flame was not , or not in so great a degree .
Should it turn out that the prominence he describes was a reality , it is barely possible that the above explanation may be the true one ; in which case it suggests the possibility of seeing the proininences with a heavy battery of prisms when the sun is not eclipsed , especially if they are made of yellow glass ; nay , even of seeing them , without the help of dispersion , through a medium calculated to stop all light but that of the sodium flame .
Mr. Chambers prevented by Clouds from using two other Spectroscopes .
Two other hard spectroscopes in my possession were lent to Mr. Chambers , Government Astronomer at Bombay , who stationed himself not far from Begapur ; but I am sorry to say he was denied the opportunity of using them by the clouds .
Gentlemen , I beg to apologize for the length of my narrative , and to subscribe myself , with much respect , Your obedient Servant , J. HERSCInEL , Lieut. R.Eo Bangalore , Sept. 1868 .
LIEUT .
CAMPBELL'S REPORT .
" ' I was deputed to accompany Lieut. Herschel on his expedition to observe the phenomena of the total eclipse , and to use the instruments supplied by the Royal Society for the observation of polarized light in the corona and red flames .
" The instruments in question were as follows:--A telescope of 3-inch aperture , mounted on a rough double axis , admitting of motion in azimuth and altitude by hand only , unaided by any appliance for clamping and slow motion .
The telescope was provided with three eyepieces of magnifying-powers 27 , 41 , and 98 ; and with it were furnished two analyzers for polarized light , viz. a double-image prism and a ' Savart 's polariscope .
' " ; The first gives two images of the object viewed , which , when polarized light is present , become strongly coloured with complementary tints , by whose changes , according to the position in azimuth of the analyzer , the plane of polarization may be found .
" The second shows the presence of polarized light by the formation , across the image of the object viewed , of coloured bands , which alter in arrangement and intensity according to the position of the polariscope with reference to the plane of polarization , and hence afford a means of arriving at a knowledge of the latter .
" With the former , slight polarization would probably be more readily recognized at a glance ; while with the latter the plane of polarization could be more easily and accurately determined .
" To carry these arms I had a pair of jointed arms constructed , so attached by a collar and screw to the eye-tube of the telescope as to admit of the eyepiece being changed .
Each arm carried one of the analyzers in a cell , in which a rotatory motion could be given for analyzing purposes .
" Either analyzer could in this way be brought instantly into position before the eyepiece of the telescope , or both could be turned aside and the telescope used by itself at pleasure .
" Immediately behind the apparatus a circular piece of cardboard of about 12 inches diameter and neatly graduated was firmly attached to the eye-tube , and to each analyzer was affixed a long pointer by which its azimuth could be referred to the graduations on the card circle , should measures of position or change of azimuth appear desirable .
" I was also furnished with a hand spectroscope for direct vision .
" The point chosen for my station was on the northern slope of a low range of hills , about 1mile W. by S. of Jamkandi .
The flatness of the hills on top offered no point from which an uninterrupted view could be obtained in all directions ; and from my station [ I only had a view of the northern half of the distant horizon over the plains extending in that direction for many miles , above the level of which I was raised about 200 feet , " Early on the morning of the 18th I proceeded to the spot , having previously sent up the instruments and a tent for shelter in case of necessity .
" At sunrise the sky was beautifully clear , except in the northern horizon , where there were low clouds lying-over the river Kistna .
There was a gentle breeze from S.W. by W. A little later light flocculent clouds began to rise and form in an arch overhead from west to east , continuing to increase as the morning wore on ; then a light scud set in , and turned gradually into broken masses of thick dark clouds .
" Before the commencement of the eclipse I took observations for time with a small theodolite , from which I computed the error of my chronometer ( a mean time one by M'Cabe ) to be Ih 14m 55S'5 fast on local apparent time ; and by that quantity I have accordingly corrected all observed chronometer times in the statements of time which follow .
" I observed the first contact , which took place at 7 " 45m 13 ' ( local apparent time ) , about 150 from the vertex ; after which I watched the progress of the eclipse , and noted the times of occultation of three sunspots .
No. 1 was a large double ragged spot , No. 2a small well-defined one , No. 3 also double , but not so large or distinct as No. 1 .
After totality I saw a fourth spot very near the sun 's limb .
" During the progress of the eclipse I observed no unevenness in the moon 's limb , nor any want of sharpness in the cusps , using magnifyingpower 27 .
" The following notes were taken on the spot : At first contact .
Sun very slightly obscured by clouds .
At 8 " Om .
Clouds thick , and gathering from S.W. and W. Wind higher and gusty .
At 8h 10 ' .
Clouds overhead , increasing and thickening and rising steadily from west .
At 8 " 20'1 .
Sky nearly entirely overcast ; clouds thickest in neighbourhood of sun .
At 8h 25"L .
A clear break .
At 8h 30 " .
I thought I could discern very faintly the dark limb of the moon beyond that of the sun ; and at this time , making allowance for the general cloudiness , I did not perceive any decrease of light on the landscape .
At 8 " 40"1 .
But tenl minutes later the darkness was decided .
At 81 45^l .
Thick clouds well broken up , stil , gathered most closely in the region of the sun .
Light becoring lurid , and increase of darkness very apparent .
At 8h 521m .
Cusps perfect ( magnifying-power 27 ) .
" Closely before totality a bright line of light appeared to shoot out at a tangent to the mcon 's limb at its centre , as if running across the bright crescent of the sun ( though of course not visible against the superior light ) and extended beyond each cusp to a distance nearly , if not quite , 15 ' .
[ Note by Lieut. H. The sketch in the margin represents Lieut. Campbell 's meaning , as asceriained orally .
] The corona became visible immediately after , between the dark limb of the moon and the bright line .
The corona did not appear so briglit as the line , the brilliance and whiteness of the light of which was most striking .
This was seen through a highly smoked glass .
At this period , probably not more than 3 to:5 seconds before totality ensued , a thick cloud shut out everything , and the rest of the phenomenon was only seen fitfully through openings in the clouds , for an aggregate period which I estimate at somewhat less than half that of totality .
" This alternate appearance and disappearance troubled me greatly , and gave rise to nervousness and excitement ; for owing to the imperfect mounting of my telescope I was apt to lose myv place whenever the light was cut off by clouds , and to waste the precious moments of clearness in finding it again .
" On the first opportunity after the commencement of the eclipse I turned on the double-image prism with the eyepiece of 27 magnifying-power , as recommended in the Instructions , which gave a field of about 45 ' diamieter .
A most decided difference of colour was at once apparent between the two images of the corona ; but I could not make certain of any such difference in the case of a remarkable horn-like protuberance , of a brightred colour , situated about 210 degrees from the vertex , reckoned ( as I have done in all cases ) with reference to the actual , not the inverted image , and with direct motion .
I then removed the double-image prism and applied the Savart 's polariscope , which gave bands at right angles to a tangent to the limb , distinct but not bright , and with little , if any , appearance of colour .
On turning the polariscope in its cell the bands , instead of appearing to revolve on their own centre , passing through various phases of brightness , arrangement , &c. , travelled bodily along the limb , always at right angles thereto , and without much change in intensity , or any at all in arrangement .
" The point at which they seemed strongest was about 1403 from the vertex , and I recorded them as black centred .
" Believing that with a higher power and a smaller field I should find it easier to fix my attention on one point of the corona and observe the phases of the bands at that point , I changed eyepieces applying that of 41 power .
With this eyepiece the first clear instant showed the bands much brighter than before , coloured , and as tangents to the lirmb at a point about 200 ?
from the vertex ; but before I could determrinle anything further a cloud shut out the view , and a few seconds later a sudden rush of light told that the totality was over , though it was difficult to believe that five minutes had flown by since its commencement .
" I experienced a strong feeling of disappointment and want of success ; the only points on which I can speak with any confidence being as follows:-(1 ) When using the double-image prism , the strong difference of colour of the two images of the corona , and the absence of such difference in the case of the most prominent red flame .
( 2 ) With the ' Savart 's polariscope ' the bands from the corona were decided ; with a low power they were wanting , in intensity and colour ; excepting alternate black and white , making it difficult to specify the nature of the centre ; and their position was at right angles to the limb , extending over about 30 ?
of the circumference .
When the polariscope was turined the bands travelled bodily round the limb without other change in position or arrangement , as if indeed they were revolving round the centre of the sun1 as an axis .
With a higher power , when a smaller portion of the coroiia was embraced , the bands were brighter , coloured , and seen in a different position , viz. tangents to the limb .
" The appearance observed with a low power seems exactly what might be expected , supposing the bands to be brightest at every point when at right angles to the limb , in which case the bands growing into brightness at each succeeding point of the limb would distract attention from those fading away at the points passed over as the analyzer revolved .
' After totality was over the clouds cleared away somewhat , and I watched the eclipse till its conclusion , noting the times of emersion of the spots and of last contact .
" A light shower fell at 9.30 .
" )During totality several stars and planets were seen by those who were with me ; and a fowl which I had placed near me , out of curiosity , was observed to compose itself to sleep .
It was at no time so dark as I had expected : after the total phase had commenced I read the chronometer and wrote notes in pencil without difficulty ; and the light of a bull's-eye lantern when thrown on my paper appeared somewhat dull .
( " The brilliance of the light of the corona when it burst out through the openings in the clouds astonished me .
Also the very gradual decrease of light before totality , and the wonderful flood of light which followed the instant of the sun 's reappearance ( though behind a cloud ) were very striking .
" I was too much occupied in watching the position of the sun , so as not to lose an instant of the precious intervals of clearness , to see much of the general effect .
I had no opportunity of using the hand spectroscope .
iQj 0 la ?
lilm oj 1.j8 l868.1 123 There was no one in my neighbourhood ( except those of my own party , who had been warned to keep silence ) , but when totality commenced a wailing shout was heard in the distance , apparently rising all round us , which was succeeded after a few seconds by silence .
" The distant features of the landscape disappeared , and I noticed one light ( apparently a village fire ) some miles distant .
" I give below the different times I observed as of possible interest .
Local apparent time is used : First contact .
Last contact .
hmshms Sun and moon ... ... ... . .
7 45 13 10 21 59 SpotNo .
1 ... ... .7 ... ... . .
757 39 975 Entire disappearance ... .
7 59 5 Spot No. 2 ... ... ... ... ... .
8 40 28 9 54 39 Spot No. 3 ... ... ... ... ... 8 46 58 10 3 25 I cannot state with any approach to , accuracy either the instant of commencement or [ that of ] termination of totality .
" Latitude of station ... ... ... 16 30 10 Longitude , , ... ... ... .
75 20 ( Signed ) " W. R. CAMPBELL , Lieut. R.E. " " Bangalore , August 31 , 1868 .
" True copy .
J. HIERSCHEL , Lieut. R.E. Bangalore , September 15 , 1868 .
( Copy .
) No. 886 .
From J. Geoghegan , Esq. , Under Secretary to Government of India .
To The Superintendent of the Great Trigonometrical Survey of India .
Fort William , February 21 , 1868 .
SIR , -I am directed to acknowledge receipt of your letter No. 6 of 4th instant ; requesting permission to employ certain officers of the Government Trigonometrical Survey in taking observations of the total solar eclipse of the 17th , 18th August , and asking sanction to the expenditure on this account estimated roughly not to exceed 2000 Rupees .
In reply , I am directed to state that the Governor-General in Council cordially approves of your proposed arrangements , and sanctions the necessary expenditure .
The Government of India , I am to state , will be prepared to do every " thilg rin its power towards securing flll and accurate observations on this rare and important occasion .
I have , &c. , ( Signed ) J , GEOGHEGAN , Under Secretary to Government of india .
True copy .
J. HERSCHEL , Lieut. R.E. [ Commander Rennoldson 's letter , which was sent independently by the Secretary of the Peninsular and Oriental Steam Navigation Company appears below .
] *XI .
" Observations of the Total Solar Eclipse of August 18 , 1868 .
" By Captain CHARLES G. PERRINS , Communicated by Prof. STOKES .
Received October 30 , 1868 .
( Abstract .
) These observations are contained in a letter dated " S.S. ' Carnatic , ' Suez , 28th August , 1868 , " addressed to the Managaing Directors , Peninsular and Oriental Steam Navigation Company .
One of the hand spectroscopes sent out by the Royal Society had been entrusted to Captain Perrins ; but as his ship at the time of the eclipse was about 20 miles north of the track of the total phase , he had no opportunity of using it for the observations contemplated .
lie thus describes the appearance at the time of greatest obscuration:"That portion of the sun remaining uneclipsed consisted of a narrow streak ( in shape like a crescent ) of its upper left limb , in size about Tpart of its diameter .
The light emitted from this was of a very peculiar description and difficult to describe , being at the same time extremely brilliant and yet most remarkably pale .
The high sea running appeared like huge waves of liquid lead , and the ghastly paleness of the light thrown upon it and all around revealed a scene which , for its weird-like effect , it would be as impossible to depict as it is to describe .
" The slender crescent showed in the spectroscope several dark lines , as was to be expected .
|
112360 | 3701662 | Observations of the Total Solar Eclipse of August 18, 1868. [Abstract] | 125 | 125 | 1,868 | 17 | Proceedings of the Royal Society of London | Charles G. Perrins | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 1 | 9 | 90 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112360 | null | http://www.jstor.org/stable/112360 | null | 112,361 | Biography | 53.926303 | Astronomy | 24.237066 | Biography | [
84.25884246826172,
4.738755226135254
] | XII .
" Observations of the Total Solar Eclipse of August 13 , 1868 .
" By Captain D. RENNOLDSON .
Communicated by Prof. STOKES .
Received October 30 , 1868 .
( Copy. .
) From Captain D. Rennoldson .
" Peninsular and Oriental Company , Bombay , 22nd August 1868 .
D EAR SIR , -I enclose you a sketch of the eclipse seen on board the * This and the following three communications were transmitted by the Directors of the Peninsular andi Oriental Steam Navigation Company .
|
112361 | 3701662 | Observations of the Total Solar Eclipse of August 18, 1868 | 125 | 126 | 1,868 | 17 | Proceedings of the Royal Society of London | D. Rennoldson | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1868.0015 | null | proceedings | 1,860 | 1,850 | 1,800 | 2 | 46 | 683 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112361 | 10.1098/rspl.1868.0015 | http://www.jstor.org/stable/112361 | 112,360 | null | Astronomy | 45.105947 | Optics | 34.999557 | Astronomy | [
83.39897918701172,
4.477261066436768
] | XII .
" Observations of the Total Solar Eclipse of August 13 , 1868 .
" By Captain D. RENNOLDSON .
Communicated by Prof. STOKES .
Received October 30 , 1868 .
( Copy. .
) From Captain D. Rennoldson .
" Peninsular and Oriental Company , Bombay , 22nd August 1868 .
D EAR SIR , -I enclose you a sketch of the eclipse seen on board the * This and the following three communications were transmitted by the Directors of the Peninsular andi Oriental Steam Navigation Company .
125 'Rangoon ' on the morning of the 18th inst .
The ship was at that time on the central line , viz. in lat. 15§ 42 ' N. , long .
590 15 ' E. " The total eclipse lasted 4 ' 8 " .
The sketch shows what was seen by a large number of persons .
In observing with the spectroscope , I saw what none of the others could see with their glasses , viz. two prominences on the right limb of the moon ( showing in the spectroscope to the left ) of a yellow flame-colour , immediately opposite to the red ones , the whole forming a square , with the moon in the centre , showing out like a mass of rock .
'T'he colour of the corona , as seen through the prism , was red , a yellowish green , blue , and violet , the violet the brightest till the middle of the eclipse , when the red became ilumpyn and showed brighter .
" The spectrum from the mioon cut thirough the centre of this , but very fa int , the red thrown out with a curve .
" The motion of the ship was so great it was impossible to get minute observations ; so much haze and flying cloud , only Venus and one other star could be seen .
" c I return the spectroscope , and am only sorry I could not make more use of it .
" I am , &c. , ( Signed ) " D. RENNOLDSON , " Commander S. S. ' Rangoon .
' Capt. HenryF , Superintendent P. O0 .
S. N. C. , Bombay .
[ This letter was accompanied by four coloured sketches of the proninences and corona .
Of these No. 1 shows a small low prominence extending from about azimuth 144 ?
to 150 ?
, azimuths being measured in the direction of the motion of the hands of a watch , round the centre of the moon 's disk , from the highest point , and another low prominence from azimuth 160 ?
to 180 ? .
No. 2 shows a lofty prominence at azimuth 198 ?
, curved in the upper part , with the concavity turned in the direction of increasing azimuth , and a low prominence from azimuth 332 ?
to 345 ? .
No. 3 shows the long prominence at azimuth 202 ?
, and the upper prominence at azimuth 320 ?
to 338 ? .
No. 4 shows the long prominence , reduced in height , at azimuth 212 ?
, and the upper prominence at azimuth 230 ?
to 2550 .
The figures are thus described .
] No. 1 .
A small red flame or protuberance on the right-hand lower corner of the moon , visible for a few seconds before the sun was totally eclipsed ; disappeared a few seconds after .
No. 2 .
1-"1 aifer commencement of total eclipse .
A large red flame of about 5 ' of arc on lower left-hand corner , and a red flame or blotch on upperleft hand -both visible from commrencementof totality , andverybright .
No. 3 .
3"i after commencement .
The long red flame rather shorter , and the upper one increased in size .
No. 4 .
At reappearance of sun 's upper limb the upper protuberance disappeared ; the lower one was visible for about 10 ' after , about half its former size .
|
112362 | 3701662 | Observations of the Total Solar Eclipse of August 18, 1868. [Abstract] | 127 | 127 | 1,868 | 17 | Proceedings of the Royal Society of London | Somerville Murray | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 1 | 7 | 109 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112362 | null | http://www.jstor.org/stable/112362 | null | null | Biography | 35.441132 | Meteorology | 31.140499 | Biography | [
84.36347198486328,
4.782198905944824
] | XIII .
" Observations of the Total Solar Eclipse of August 18 , 1868 .
" By Captain SOMERVILLE MURRuAY .
Communicated by Prof. STOKES .
Received October 30 , 1868 .
( Abstract .
) In accordance with the instructions he had received from the Managing Directors of the Peninsular and Oriental Steam Navigation Company , Captain Murray made all observations that were possible of the eclipse of the 18th August ; but the high northern latitude of the ship 's ( ' Ellora ' ) position at the time precluded the possibility of observing any remarkable phenomenon , the obscuration of the sun being comparatively slight .
|
112363 | 3701662 | Observations of the Total Solar Eclipse of August 18, 1868. [Abstract] | 127 | 127 | 1,868 | 17 | Proceedings of the Royal Society of London | Henry Welchman King | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 1 | 30 | 421 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112363 | null | http://www.jstor.org/stable/112363 | null | null | Optics | 41.013082 | Astronomy | 40.341922 | Optics | [
83.25300598144531,
4.3223066329956055
] | XIV .
" Observations of the Total Solar Eclipse of August 18 , 1868 .
" By Captain HENRY WELCIHMAN KING .
Communicated by Prof. STOKES .
Received October 30 , 1868 .
( Abstract .
) The weather was cloudy throughout , but the clouds were thin , so much so as to allow two or three stars to be seen during the time of totality .
The corona exhibited itself quite suddenly on the instant of first totality .
It presented the appearance of a golden-yellow brightness of no very intense brilliancy .
It disappeared as suddenly as it appeared , on the first sign of the retiring sun .
The flames or prominences became visible simultaneously with the corona .
The paper was accompanied by four coloured sketches , the first representing the positions of the sun and moon , with the spots on the former , at an early stage of the eclipse , as observed with a 5-foot telescope by Ross of three inches aperture ; the remaining three representing different stages of the totality .
The second figure shows a red prominence about 25 ?
to the left or east of the lowest point , with a smaller green promitnence , also in contact with the moon , a little distance to the east of it .
The third shows a red prominence about 30 ?
to the right of the lowest point .
The fourth figure shows a broad prominence a little to the left of the highest point .
The figures 2-4 are thus described : Fig. 2 .
" First instant of totality .
This flame or prominence was visible during the whole period of totality by ordinary glasses .
The prismatic colours to the eastward of ' flame I did not see myself , and cannot vouch for them .
" Fig. 3 .
" Middle of totality .
This flame or prominence visible during the whole period of eclipse to ordinary glasses .
" Fig. 4 .
" First reappearance of sun .
I did not observe this flame in early stages of totality , though it may have been visible .
It was observed by the above-mentioned Ross , and was not so brilliatt as the others , though lmore extended .
Entire power of the totality extended over 2 minultes 48 secondls .
" The observations were made on board the steamer ' Rangoon , ' approximate latitude 16§ 44 ' N. , longitude 83§ 55 ' E.
|
112364 | 3701662 | Supplementary Note on a Spectrum of a Solar Prominence | 128 | 128 | 1,868 | 17 | Proceedings of the Royal Society of London | J. Norman Lockyer | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1868.0017 | null | proceedings | 1,860 | 1,850 | 1,800 | 1 | 6 | 122 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112364 | 10.1098/rspl.1868.0017 | http://www.jstor.org/stable/112364 | null | null | Biography | 41.289291 | Astronomy | 38.958087 | Biography | [
18.206710815429688,
-36.300071716308594
] | " Supplementary Note on a Spectrum of a Solar Prominence .
" By J. NORMAN LOCKYER , F.R.A.S. , in a Letter to the Secretary .
Communicated by Dr. SHARPEY , Sec. R.S. Received November 5 , 1868 .
SIR , -I have the honour , in continuation of my letter of the 20th ultimo , to inform you that I have this morning obtained evidence that the solar prominences are merely the expansion , in certain regions , of an envelope which surrounds the sun on all sides .
I may add that other facts observed seem to point out that we may shortly be in a position to determine the temperature of these circumsolar regions .
J. NORMrAN LOCKYER .
|
112365 | 3701662 | Account of Explorations by the Swedish Arctic Expedition at the close of the Season 1868 | 128 | 131 | 1,868 | 17 | Proceedings of the Royal Society of London | A. E. Nordenski\#xF6;ld | fla | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 4 | 65 | 2,011 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112365 | null | http://www.jstor.org/stable/112365 | null | null | Geography | 40.269774 | Biography | 37.085229 | Geography | [
57.33113479614258,
11.919106483459473
] | XVI .
" Spectroscopic Observations of the Sun."-No .
II .
By J. NORMAN LOCKYER , F.R.A.S. Communicated by Dr. SHARPEY , Sec. R.S. Received November 19 , 1868 .
The reading of this Paper was commenced .
November 26 , 1868 .
Lieut.-General SABINE , President , in the Chair .
In pursuance of the Statutes , notice was given from the Chair of the ensuing Anniversary Meeting , and the list of Officers and Council proposed for election was read as follows : President.-Lieut.-General Edward Sabine , R.A. , D.C.L. , LL. D. Treasurer.-William Allen Mliller , M.D. , LL. D. f William Sharpey , M.D. , LL. D. Secretaries .
George Gabriel Stokes , Esq. , M.A. , D.C.L. , LL. D. Foreign Secretary.-Prof .
William Hallows Miller , M.A. , LL. D. Other Members of the Council.-Frederick Augustus Abel , Esq. ; .Sir Benjamin Collins Brodie , Bart. , M.A. ; William Benjamin Carpenter , M.D. ; J. Lockhart Clarke , Esq. ; Frederick Currey , Esq. , M.A. ; Warren De La Rue , Esq. , Ph. D. ; Sir William Fergusson , Bart. ; William Henry Flower , Esq. ; Capt. Douglas Galton , C.B. ; John Peter Gassiot , Esq. ; John Hawkslaw , Esq. ; John Marshall , Esq. ; Joseph Prestwich , Esq. ; George Henry Richards , Capt. R.N. ; Archibald Smith , Esq. , M.A. ; Lieut.-Col. Alexander Strange .
Lieut.-Col. Cameron , Mr. Crofton , Mr. Griess , and the Rev. Dr. Tristram were admitted into the Society .
The following communications were read:128 I. " Account of Explorations by the Swedish Arctic Expedition at the close of the Season 1868 , in a Letter to the President .
" By Professor A. NORDENSK6ILD .
Communicated by the President .
Received November 20 , 1868 .
Troms6 , October 23 , 1868 .
SIR , -The second geographical part of our expedition anchored a few days ago in the harbour of Tromso , after a difficult and adventurous autumn cruise of a month in the polar basin north of 80 ?
lat. ; and as these regions were never before visited in such a late season , I hope that our observations will be of interest for the arctic men of Great Britain , as contributing to settle some points of the polar question recently much debated .
According to the plan adopted for the Swedish Expedition , five of its naturalists returned , in the middle of September , to Tromso with one of the small ships that brought coal to our depot at Amsterdam Island , and the same day the 'Sofia , ' with the remaining part of the expedition ( consisting of v. Otter , Berggren , Nystr6m , Palander , Lemstrim , and myself ) , steamed northward for Seven Islands , where it was our intention to wait for a favourable occasion to go further .
But finding these islands so surrounded by ice that no anchorage was accessible , we were compelled to abandon this plan and go directly northward , following a tolerably large opening in the pack .
After a cruise of some days among the ice we , on the 19th of September , at 17k ?
long .
east of Greenwich , reached 81§ 42 ' N. Lat. ; but , as may be seen by the adjoined photograph , the ice further northward was so closed that it was impossible even for a boat to advance .
We turned westward , in vain looking for another practicable opening .
Following the border of the pack , we were , on the 24th September , at a longitude of 2 ?
W. already south of 79 ?
lat. , after often having passed fields of drift-ice covered with particles of earth , which seems to indicate that land is to be met with further northward .
Despairing of finding the ice westward more favourable , and anxious to make a new survey later in the autumn of the position of the ice-field between 0 ?
and 20 ?
long .
, we returned to our coal-depot .
North of 80§ 30 ' the season was already far more advanced than one would presume from the observations at Spitzbergen during the first part of September .
The temperature of the air being -6 ?
to -8 ?
( Centigrade ) below zero , the surface of the sea was , when calm , covered by a layer of new ice more than an inch thick ; and after sunset the obscurity , increased by constant intense frost-rime , made the sailing or steaming among the ice both uncertain and dangerous .
As the salt water has no maximum of density , the freezing of the surface over a depth of 1000 to 2000 fathoms would be difficult to explain , were it not that the sea-water in the polar regions is by the melting of the ice and the heavy autumnal snowfalls less salt , and accordingly lighter , even when at a temperature lower than that of the layers beneath .
The last week of September was employed in filling our coal-boxes and refitting our steamer for a new struggle with the ice .
During these days a strong easterly snow-storm prevailed , which made us hope to find the newly-formed ice broken and the pack more dispersed than before .
Our N. 6 , intention was to employ this favourable circumstance for making a last attempt to go northward , and if this should prove to be unsuccessful to winter at Seven Islands .
This plan was frustrated by an accident similar to that which happened to the expeditions of Buchan and Ross in 1818 .
The calm that during the summer prevails in the Arctic Sea gave way after September 23rd to almost uninterrupted stormy weather , which caused such a violent and irregular sea on the border of the pack that it was impossible to advance without exposing the ship to be instantly crushed by the large rolling hummocks .
Consequently we were obliged to lay to under the 81st parallel , waiting for better weather and a calmer sea .
However , everywhere on the surface of the sea large pieces of ice were scattered , dangerous by their rolling movement , their hardness ( the terrperature was 14§ 5 Centigrade ) , and the obscurity that prevailed at night .
During a south-easterly storm on April 24 our steamer was so vehemently thrown against such a hummock that a large leak ensued , which forced us to make as soon as possible for land .
After hard work in keeping the steamer afloat , we reached Amsterdam Island , where the leak was provisionally caulked so as to enable us to reach a safer harbour in Kings Bay the following day .
Here we had the ship down , and the damage was repaired as well as possible .
October 12 we left this harbour , going through a large field of new ice .
Evidently the season was t ; oo far advanced for further enterprises to the northward ; besides , our steamer , having got two ribs broken , was no longer strong enough for a new encounter with the ice ; and as a wintering only on Seven Islands could not be of an interest great enough to outweigl the loss of time , privations , and dangers unavoidably associated with it , we resolved to employ the yet tolerably open sea around the southern part of Spitzbergen to make an attempt to reach Giles Land , But being , at Thousand Islands , prevented by ice from penetrating further , we turned southward and reached Troms6 , April 19 , after having at Beeren Eiland sustained a severe storm , during which our steamer was quite , ice down by the waves that washed over .
During our cruise in the polar basin interesting observations were obtained on the temperature , currents , &c. of the sea , and a number of carefully examined deep soundings were made with an apparatus resembling the 'Bulldog ' apparatus of M'Clintock , by the intelligent and intrepid commander of the 'Sofia , ' Captain Baron v. Otter , and I hope soon to be able to present you a copy of his map on these subjects , the position of the ice , &c. As you already know by the letter of Dr. Malimgren , the scientific results of the first part of our expedition have been very satisfactory , and I hope also that its second part will give important information about several arctic questions .
By the expeditions of Tschitschayoff ( 1765 & 1766 ) , Phipps , Buchan , Franklin , Scoresby , Sabine , Clavering , Parry , Torell , &c. , it was already long ago proved that in the summer compact masses of drift-ice prevented ~vessels frot }i enetrating far into the p}ola btsii. .
But during the most favourable season , i. e. the time before the formation of new ice , no vessel had as yet made such an attempt .
This was the aim of the Swedish Expedition , and it found(1 ) That the polar sea is far more open in the autumn than at any other season of the year , but that even then the passage is soon stopped by dense and impenetrable masses of broken ice .
( 2 ) That during the winter the polar basin is covered by an unbroken ice , and that the freezing of the surface begins as early as the end of September .
From September 23 to October 12 we had almost every day , either with the steamer or with boats , to cross new-formed ice .
( 3 ) That an autumn cruise north of 80 ?
2 lat. is attended with unusual dangers , owing to the darkness and storms then prevailing , no ships being able a long time to sustain a night storm among large rolling pieces of ice and a cold of 15 ?
Cent. If the ship has the good luck not to be more or less damaged by the constant unavoidable encounters withi the ice mounts , it will soon by the immediate freezing of the washing waves be itself quite covered and pressed down by ice .
( 4 ) The idea of an open and comparatively milder polar basin is quite chimerical ; on the contrary , 20'-30 ' north of Spitzbergen a region of cold seems to begin which no doubt stretches far around the pole .
( 5 ) The only plan to attain the pole , from which success can be expected , is that adopted by most English arctic men , namely of going northward by sledges in the winter either from Smith Sound or Seven Islands .
I remain , Sir , Your obedient humble Servant , A. E. NORDENSKIOLD .
P.S. As soon as the magnetical observations of Dr. Lemstrom shall be duly worked out I will send you a copy of them .
Should you think it worth communicating this letter to the Rloyal Geographical Society , I beg you especially to inform its celebrated President , Sir R. Murchison , that besides other specimens interesting in a geological point of view ( for instance , a mass of Miocene and coal plants , bones of Ichthyosaurus ?
&c. ) , we found a number of large fish fragments , probably belonging to the Devonian age , in the red slate of Liebde Bay , constituting the overmost layer of what I in my 'Geology of Spitzbergen ' called Hecla block formation .
Accordingly Sir Roderick probably is right in supposing that the deeper layers of this " formation " belong to the Silurian age .
The underlying crystalline plates are evidently Laurentian .
|
112366 | 3701662 | Spectroscopic Observation of the Sun, No. II. [Abstract] | 131 | 132 | 1,868 | 17 | Proceedings of the Royal Society of London | J. Norman Lockyer | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 2 | 21 | 627 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112366 | null | http://www.jstor.org/stable/112366 | null | null | Atomic Physics | 40.597487 | Astronomy | 30.569634 | Atomic Physics | [
19.236482620239258,
-33.945068359375
] | II .
The reading of Mr. Lockyer 's Paper , " Spectroscopic Observation of the Sun , No. II .
, " was resumed and concluded .
( Abstract .
) THE author , after referring to hisi ineffectual attempts since 1866 to observe the spectrum of the prominences with an instrument of small dispersive powers , gave an account of the delays which had impeded the construction of a larger one ( the funds for which were supplied by the Government-Grant Committee early in 1867 ) , in order that the coincidence in time between his results and those obtained by the Indian observers might not be misinterpreted .
Details are given of the observations made by the new instrument , which was received incomplete on the 16th of October .
These observations include the discovery , and exact determination of the lines , of the prominencespectrum on the 20th of October , and of the fact that the prominences are merely local aggregations of a gaseous medium which entirely envelopes the sun .
The term Chromosphere is suggested for this envelope , in order to distinguish it from the cool absorbing atmosphere on the one hand , and from the white light-giving photosphere on the other .
The possibility of variations in the thickness of this envelope is suggested , and the phenomena presented by the star in Corona are referred to .
It is stated that , under proper instrumental and atmospheric conditions , the spectrum of the chromosphere is always visible in every part of the sun 's periphery ; its height , and the dimensions and shapes of several prominences , observed at different times , are given in the paper .
One prominence , 3 ' high , was observed on the 20th October .
Two of the lines correspond with Fraunhofer 's C and F ; another lies 8 ?
or 9 ?
( of Kirchhoff 's scale ) from D towards E. There is another bright line , which occasionally makes its appearance near C , but slightly less refrangible than that line .
It is remarked that the line near D has no corresponding line ordinarily visible in the solar spectrum .
The author has been led by his observations to ascribe great variation of brilliancy to the lines .
On the 5th of November a prominence was observed in which the action was evidently very intense ; and on this occasion the light and colour of the line at F were most vivid .
This was not observed all along the line visible in the field of view of the instrument , but only at certain parts of the line which appeared to widen out .
The author points out that the line F invariably expands ( that the band of light gets wider and wider ) as the sun is approached , and that the C line and the D line do not ; and he enlarges upon the importance of this fact , taken in connexion with the researches of Pliicker , Hittorf , and Frankland on the spectrum of hydrogen-stating at the same time that he is engaged in researches on gaseous spectra which , it is possible , will enable us to determine the temperature and pressure at the surfaces of the chromosphere , and to give a full explanation of the various colours of the prominences which have been observed at different times .
The paper also refers to certain bright regions in the solar spectrum itself .
Evidence is adduced to show that possibly a chromosphere is , under certain conditions , a regular part of star-economy ; and the outburst of the star in Corona is especially dwelt upon .
|
112367 | 3701662 | Extract from a Letter Addressed by Chas. Babbage, Esq., F.R.S., to Dr. Bache, of Washington, May 10, 1852 | 133 | 133 | 1,868 | 17 | Proceedings of the Royal Society of London | Chas Babbage | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1868.0020 | null | proceedings | 1,860 | 1,850 | 1,800 | 1 | 17 | 321 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112367 | 10.1098/rspl.1868.0020 | http://www.jstor.org/stable/112367 | null | null | Astronomy | 39.01866 | Biography | 32.745771 | Astronomy | [
73.29039001464844,
33.0498161315918
] | III .
" Extract from a Letter addressed by CHAS .
BABBAGE , Esq. , F.R.S. , to Dr. BACHE , of Washington , May 10 , 1852 .
Communicated by Mr. BABBAGE .
Received November 26 , 1868 .
" In reading the account of the great solar eclipse of last year ( 1851 ) I was much struck by the description of the pink excrescences apparently attached to the sun 's disk , and connected with its spots ( see Proceedings of Royal Astronomical Society ) .
They are only visible during a few minutes in a total eclipse .
It occurred to me that it might be possible to render them visible at other times by two different methods:"1st .
By placing in the focus of an equatorial telescope moved by clockwork an opake disk , equal to or a little larger than the sun 's image .
This would represent a continuous total eclipse ; and if every known means of excluding light were adopted , it might be possible to see those faint pink objects , which are probably clouds raised by the eruption of solar volcanoes .
" 2nd .
If this fail , it might yet be possible to render them visible by taking daguerreotype or photographic images .
" It is really surprising that nobody has yet taken such images regularly , for the sake of recording the solar spots and their changes .
I have no clock-moving equatorial myself fit for these observations , nor have I time to spare for them .
" I cannot persuade my countrymen that they are important , so you are at liberty to try them , or publish the plan on your side of the Atlantic .
" Mr. Gould will probably have explained to you an old plan of mine for mapping zones of stars without moving the eye from the telescope .
"
|
112368 | 3701662 | Anniversary Meeting | 133 | 154 | 1,868 | 17 | Proceedings of the Royal Society of London | null | fla | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 22 | 360 | 11,281 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112368 | null | http://www.jstor.org/stable/112368 | null | null | Biography | 65.161881 | Optics | 8.901109 | Biography | [
73.2907485961914,
33.071170806884766
] | III .
" Extract from a Letter addressed by CHAS .
BABBAGE , Esq. , F.R.S. , to Dr. BACHE , of Washington , May 10 , 1852 .
Communicated by Mr. BABBAGE .
Received November 26 , 1868 .
" In reading the account of the great solar eclipse of last year ( 1851 ) I was much struck by the description of the pink excrescences apparently attached to the sun 's disk , and connected with its spots ( see Proceedings of Royal Astronomical Society ) .
They are only visible during a few minutes in a total eclipse .
It occurred to me that it might be possible to render them visible at other times by two different methods:"1st .
By placing in the focus of an equatorial telescope moved by clockwork an opake disk , equal to or a little larger than the sun 's image .
This would represent a continuous total eclipse ; and if every known means of excluding light were adopted , it might be possible to see those faint pink objects , which are probably clouds raised by the eruption of solar volcanoes .
" 2nd .
If this fail , it might yet be possible to render them visible by taking daguerreotype or photographic images .
" It is really surprising that nobody has yet taken such images regularly , for the sake of recording the solar spots and their changes .
I have no clock-moving equatorial myself fit for these observations , nor have I time to spare for them .
" I cannot persuade my countrymen that they are important , so you are at liberty to try them , or publish the plan on your side of the Atlantic .
" Mr. Gould will probably have explained to you an old plan of mine for mapping zones of stars without moving the eye from the telescope .
" November 30 , 1868 .
ANNIVERSARY MEETING. .
Lieut.-General SABINE , President , in the Chair .
Mr. Newmarch , on the part of the Auditors of the Treasurer 's Accounts appointed by the Society , reported that the total receipts during the past year , including a balance of ?
495 10s .
3d .
carried from the preceding year , amount to ?
4780 5s .
lld .
; and that the total expenditure in the same period amounts to ?
4286 1 Is .
5d .
, leaving a balance of ?
479 16s .
Id. at the Bankers ' , and of ?
13 1Ss .
5d .
in the hands of the Treasurer .
The thanks of the Society were voted to the Treasurer and Auditors .
The Secretary read the following Lists : Fellows deceased since the last Anniversary .
Royal .
Ilis Imperial and Royal Highness the Archduke Louis of Austria ( 1864 ) .
134 Charles Dickson Archibald , Esq. Charles James Beverly , Esq. Capt. Benjamin Blake ' .
Rev. Miles Bland , D.D. Sir David Brewster , K.H. , LL. D. , D.C.L. Henry , Lord Brougham and Vaux , M.A. Rev. Jonathan Cape .
Robert John , Lord Carington .
Antoine Francois Jean Claudet , Esq. The Right Hon. Sir George Clerk , Bart. , D.C.L. John Crawfurd , Esq. Charles Giles Bridle Daubeny , M.D. , LL. D. Johrn Davy , MT .
D. Rev. William lRutter Dawes .
George Douglas , Esq. ( 1853 ) .
Marie Jean Pierre Flourens .
Jean Bernard Leon Foucault .
[ Nov. 30 , Sir William Francis Eliott , Bart. ( 1864 ) .
John Elliotson , M.D. The Right Hon. Sir Edmund Walker Head , Bart William Bird Herapath , M.D. Sir Charles Lemon Bart. Sir John Liddell , K.C.B. , M.D. John Carnac Morris , Esq.- " Rev. Henry Noel-Fearn , McA .
, D.C.L. Robert Porrett , Esq. Archibald John , Earl of Rosebery , K.T. , M.A. , LL. D. The Yen .
Archdeacon Tattam , D.D. Thomas Pridgin Teale , Esq. Nathaniel Bagshaw Ward , Esq. Alexander Luard Wollaston , M.B * .
the Foreign List .
Julius Pliicker .
Jean Victor Poncelet .
Withdrawn .
Rear-Admiral Thomas Edward Lawes Moore .
Sir John Macneill .
Edward Solly , Esq. Defaulters .
The Right Hon. Charles Pelhamt Villiers .
Fellows elected since the last Anniversary .
John Ball , Esq. , M.A. A Augustus G. Vernon Harcourtt , Esq. IHenry Charlton Bastian , M.D. Rear Ad .
Astley Cooper Key , C.B. Lieut.-Col. John Cameron , R.E. Rear-Admiral E. Ommanney , C.B. Prof. Robert Bellamy Clifton , M.A. James Bell Pettigrew , M.D. Morgan William Crofton , Esq. , B.A. Laurence Parsons , Earl of Rosse .
Joseph Barnard Davis , M.D. Edward James Stone , Esq. , M.A. Peter Mlartin Duncan , 3cM .
B. IRev .
Henrv Baker Tristram , M.A. John Peter Griess , Esq. Wm. S. Wright Vaux , Esq. , M.A. On the Foreign List .
Theodor Ludwig Wilhelm Bischoff .
Hugo von Moil .
Rudolph Julius EmmanuelClausius .
Samuel Heinrich Schwabe .
Readmitted .
Colonel John Le Couteur .
- ' Date of decease unknown .
President 's Address .
The President then addressed the Society as follows : GENTLEMEN , I HAVE the satisfaction of now laying before you the second volume of the Catalogue of Scientific Papers .
The volume now completed carries on the list of titles in alphabetical order as far as GR A , inclusive .
The Library Committee , under whose superintendence the Catalogue is published , had hoped that the printing of the work would have made greater progress than it has done during the time that has elapsed since the appearance of the first volume ; but notwithstanding their earnest endeavours to attain that object , they found that , with due regard to the careful revision of the press , the rate of printing could not be materially accelerated .
In fulfilment of the understanding with Her Majesty 's Government , explained in my Address last year , copies have been presented to various Scientific Institutions and individuals , according to a list drawn up by the Council , and approved by the Treasury .
It is gratifying to know that in the numerous letters of acknowledgment received in return , as well as more publicly through the press , the value of the work as an aid to scientific research has been warmly recognized .
As a special instance of this favourable expression of opinion , I would refer to the ample notice of the book written by our Foreign Member , Hofrath W. Ritter v. Haidinger , of Vienna , and circulated by him in different parts of Europe .
Already of the remaining copies 120 have been sold .
My last year 's Address contained an account of the proceedings of the Committee of the Royal Society , which , at the request of Her Majesty 's Government , had undertaken the reorganization and superintendence of the meteorological department of the Board of Trade .
The year that has since elapsed has been employed , 1 ?
, In perfecting the instrumental arrangements , and the systematic working of the staff , at the seven British Observatories which have been supplied , under the Committee 's direction , with continuously self-recording meteorological apparatus .
For this purpose one or more of the staff of each Observatory has passed some days at the Central Observatory at Kew ; and the Observatories themselves have been visited , some by Mr. Scott , the Director of the Meteorological Office in London , and all by Mr. Stewart , the Superintendent of the Central Observatory , and also by Mr. Beckley , the Engineer of the Kew Establishment .
By these means it is hoped that uniformity of action on thoroughly well considered principles has been secured , and a considerable advance made towards the systematic record of the meteorological phenomena over the British Islands .
The monthly records are now beginning to be received at the Office in London with regularity from all the Observatories , but have scarcely yet quite attained in all instances to that uniform accuracy which it is hoped will be fully secured at the close of the present year .
The means and the methods by which the facts thus considerately and systematically obtained may be communicated to the public , in the form which may be at once suitable for the study of the weather phenomena over the very limited territorial area of the British Islands-and may at the same time contribute in the most satisfactory manner to the important investigations which are now in progress on the Continent of Europe regarding the periodic and non-periodic variations will be the next point to which the careful attention of the Committee will be directed .
2 ? .
In the branch of ocean meteorology the cooperation of several of our leading oceanic steam companies has been secured ; and a large number of the commanders of their vessels are now actively engaged in the work of observing .
Instruments have also been supplied to other masters of vessels of our mercantile marine , care being always taken that the recipients are both competent to observe and willing to do so regularly and accurately .
The zeal and judgment displayed by Captain Henry Toynbee , the Marine Superintendent of the Office , in the selection of observers , has already begun to bear fruit in the marked improvement in the quality of the information in the registers which are now received compared with those which had previously accumulated in the office .
The discussion of the material which has been thus collected and is still collecting is in progress ; but some time must elapse before a significant portion of the immense arrear can be advanced to such a stage as to afford a prospect of its speedy publication .
The staff of clerks is already fully occupied ; so that the rate of progress cannot be much accelerated , unless the Committee find themselves in a position to devote more funds to this object than they are at present able to do .
The special subject to which the attention of this department of the office has been first directed , is the discussion of information respecting the district of the Atlantic Ocean comprised between the parallels of 20 ?
N. and 10 ?
S. , for which region it is in contemplation to ascertain the conditions of atmospheric pressure , temperature , and vapour tension , as well as the direction and force of wind , the character of the weather , and the surface temperature of the sea .
These elements will be discussed for spaces of a single square degree in area for the different months .
As regards the temperature of the surface of the sea ( a subject so much dwelt on by the President and Council of the Royal Society in their letter to the Board of Trade of February 22 , 1855 ) , a very valuable series of monthly charts has been published by the Royal Meteorological Institute of the Netherlands , exhibiting the temperature for each degree of latitude for the North and South Atlantic Oceans , and for the Indian Ocean .
The Committee considered that a conversion of the data in these charts into British measures would be likely to be of immediate use to our own marine , and they have accordingly directed that a set of charts should be prepared in the first instance for the South Atlantic Ocean , exhibiting the Dutch resutlts , as well as those obtained from the British registers received by the meteo rological department of the Board of Trade under its former management .
These latter , however , were only calculated for spaces of five degrees square .
In addition , some of the work left in an unfinished state by Admiral Fitz Roy has been undertaken by the office at extra hours , and a series of wind-tables for the Atlantic have been ordered to be printed .
The discussion of general meteorological information for the Pacific seaboard of South America is in a state far advanced towards completion .
3 ? .
The system of telegraphic weather-intelligence , described in my last year 's anniversary address , has received a further development , and at present the Drum signal is hoisted at 97 British stations , to convey the intelligence of the existence of atmospherical disturbance in each case to such ports as may appear to the central office to be reasonably liable to be affected by it .
Similar intelligence has been telegraphed to Hamburg since February 1868 ; and in the course of last month Herr von Freeden , the Director of the newly established meteorological office in that city ( the Nord-deutsche Seewarte ) , has informed the London office that the harbour authorities on the Elbe have resolved to hoist the Drum signal at 1amburg and Cuxhaven whenever intelligence implying probable danger shall be received from London .
In France also the ministry of the marine has adopted , for the present at least , the practice of telegraphing facts and not prophecies .
In addition to the telegraphic communications already referred to , the London Office sends , by special request , telegraphic intelligence of the existence of a certain amount of difference of barometric pressure between two stations within a defined area , to Mr. Rundell ( Secretary of the Underwriters ' Association at Liverpool ) , and to the Dutch authorities .
The influence which the distribution of atmospheric pressure exerts on the motion of the air has been much dwelt upon by Dr. Buys Ballot , of Utrecht , and a rule has beeu propounded by him for inferring the coming direction of the wind from simultaneous readings of the barometer at different places .
In order to lay the foundation of a systematic study of our weather , and , at the same time , to test the truth of this rule , it has been the practice of our meteorological office , for more than a year past , to prepare , and subject to systematic discussion , daily charts of the meteorological condition over the area embraced by the daily telegraphic reports which it receives , viz. the British Islands and a portion of the nearer continental coasts .
The results of this investigation are on the whole encouraging , and favour the hope that with a more extended experience a real , if slight , advance will have been made in this most intricate but interesting inquiry .
The magnificent but rare phenomenon of a total solar eclipse is not more striking as a spectacle than interesting in a scientific point of view , from the precious opportunity it affords of gathering information , then only to be obtained , which bears on the constitution of our great luminary .
The corona which surrounds the dark body of the moon must have been seen from the earliest times ; but what does it import ?
Has it its seat in our own atmosphere , or in an atmosphere of the moon , or in something surrounding the sun ?
and , in the latter case , is it self-luminous , or does it shine by reflected light ?
What , again , is the nature of those singular rose-coloured luminous objects seen just outside the dark disk of the moon , which were first brought prominently into notice by the observers who watched the eclipse of July 7 , 1842 , and have subsequently been seen on the occasion of total solar eclipses ?
Evidence bearing in an important manner on the true answers to these questions had already been obtained on the occasion of former total eclipses .
In that of July 18 , 1860 , M. Prazmouski ascertained that the light of the corona was strongly polarized in a plane passing through the centre of the sun , while that of the prominences was unpolarized .
The fact of the polarization discarded the hypothesis , sufficiently improbable on other grounds , that the corona belongs either to our own atmosphere or to a lunar atmosphere ( since in that case the light would be reflected or scattered at an almost grazing incidence ) , and proved it to belong to the sun , and to shine mainly , if not wholly , by reflected light .
The absence of polarization in the light of the prominences proved that they are very probably selfluminous .
The elaborate photographic observations of Mr. Warren De La Rue on the same eclipse proved , by the motion of the prominences relatively to the moon , that they belong to the sun , and showed that their light is remarkable for its actinic power .
In the interval between this eclipse and that of the present year , a new method of research had sprung up , in the application of the spectroscope to the celestial bodies , and already , in the hands of Mr. Huggins , had revealed in many of the nebule a constitution hitherto unsuspected .
It was important to apply this method oftresearch to the red prominences .
Should they give a continuous spectrum , the conclusion would be that the matter of which they consist is probably in a solid or liquid condition , such as clouds formed by precipitation ; should the spectrum be one of bright lines , we must conclude that they are glowing gas .
To solve this important problem , independently of what might be done by other scientific bodies or by individuals , the Royal Society procured an equatorially mounted telescope , furnished with a spectroscope and clockmovement .
With the sanction of Colonel Walker , R.E. , Director of the Great Trigonometrical Survey of India , this instrument was entrusted to Lieut. John Herschel , R.E. , who is attached to the Survey , and who , being at the time in England , had the advantage of instruction from so skilful an observer as Mr. Huggins before his return to India .
After his return to India , Lieut. Herschel worked diligently at the spectra of the southern nebulae , thereby at the same time making an important addition to our knowledge , and practising for the approaching eclipse .
Four directvision hand-spectroscopes , intended for distribution to observers at different stations , were also sent out , -partly that the occasion might not be wholly lost in case clouds should prevent observations from being taken at the principal station ; partly because a more rough and general view of the whole phenomenon might reveal features which would be missed in a more careful scrutiny of a particular part .
Another telescope , furnished with analyzers for the examination of polarization , was also sent out ; for from the shortness of the time at the disposal of an observer , it would be satisfactory that the results obtained , even by so skilful an observer as M. Prazmouski , should be confirmed .
The observations of the observers entrusted with these instruments were greatly impeded by flying clouds , notwithstanding which , however , important work was done .
With the principal instrument , Lieut. Herschel ascertained that the spectrum of the prominences showed 'three isolated bright lines-red , orange , and blue .
He had time to take a good measure of the position of the orange line , which proved to be coincident with D , as nearly as the instrument could measure .
Clouds prevented the measure of the blue line from being equally good ; it proved , however , to be nearly coincident with F , apparently a very little less refrangible .
With one of the hand-spectroscopes Captain Haig , R.E. , observed the spectrum of the red prominences to consist of two bands , " rose-madder " and " golden yellow , " corresponding , doubtless , to the " red " and " orange " of Herschel .
But besides these , just before the emergence of the sun , Capt. Haig observed , " in the spectrum of the moon 's edge , " two well-defined bright bands , one green and one indigo .
The seizing of this almost momentary phenomenon , establishing as it does the existence of a thin envelope of glowing gas ( unless , indeed , the constitution thus revealed were merely local , and its occurrence just at the part of the sun first measured were a mere matter of chance ) , proves the advantage of not neglecting the use of a comparatively rough instrument intended for a general scrutiny of the phenomenon .
Of the remaining hand-spectroscopes , one was entrusted to Mr. Chambers , Director of the Bombay Observatory , but could not be used on account of clouds , and two were placed in the hands of the commanders of homeward-bound steamers , belonging to the Peninsular and Oriental Steam Navigation Company .
Capt. Charles G. Perrins , of the ' Carnatic , ' who had charge of one , was unable to apply it to the intended observations , as his ship was about 20 miles north of the track of the total phase ; with the other , Capt. Rennoldson , of the 'Rangoon , ' ascertained the discontinuous character of the red prominences , and his observation would have been very valuable had clouds prevented observations from being taken on shore .
The telescope furnished with analyzers was placed in the hands of Lieut. Campbell , R.E. , who has fully confirmed the previous observation of M. Prazmouski relative to the strong polarization of the light of the corona .
A feature of the prominences , which is specially noticed in Capt. IHaig 's account , resting on the observations of Capt. Tanner and Mr. Kero Laxuman , who were of his party , is their streaked character .
This had been noticed before , in the eclipse of 1860 .
Mr. Warren De La Rue , in speaking of the prominences , expressly mentions their structure ; and M. Chacornae , who devoted himself to this object , has given a long description of their appearance* , which , however , is a little difficult to follow for want of a figure .
The strong actinic power , the streaked character , and the bright-line spectrum of the prominences seem certainly to accord very well with the hypothesis in which they are regarded as gigantic aurorsea view , however , which may be rendered less probable by the apparently general prevalence over the sun 's surface of a lower stratum of similar nature , of which the prominences are merely elevated portions .
The great Melbourne Telescope was despatched to its destination in an Australian packet ( ' The Empress of the Seas ' ) , which sailed from Liverpool on the 18th of July last ; and M. Le Sueur proceeded overland to await its arrival .
The micrometer and spectroscope which are to follow are quite ready , and the photographic apparatus is also nearly ready , to be despatched to Melbourne .
In June last the President and Council received from Dr. Carpenter and Professor Wyville Thomson letters strongly recommending that the Zoology of the Deep Sea , especially in the North Atlantic Ocean , should be more thoroughly and systematically examined than has hitherto been accomplished , and requesting the intervention of the Royal Society with the Admiralty for the purpose of obtaining the services of a vessel , with proper means and appliances for deep-sea sounding and dredging , to carry on a systematic research , in the seas immediately north of our own island , for a month or six weeks in the approaching autumn-and tendering their own services to accompany the vessel .
With the thoroughly efficient aid of the Hydrographer , Capt. Richards , R.N. , the'Lightning , ' surveying-ship , Staff-Commander May , was selected and equipped expressly for this service ; and Dr. Carpenter and Professor Thomson embarked in her on the 10th of August , at Stornoway .
After examining the seas between Scotland and the Faroe Islands , the 'Lightning ' returned on the 9th of September to Stornoway , to land Professor Thomson ( whose presence was required elsewhere ) , and sailed again ( this time accompanied by Dr. Carpenter only ) for a second , more westerly cruise , which lasted until the 26th of September .
A preliminary report of the results has been received from Dr. Carpenter , and will be read to the Society at an early evening meeting in the present session ; I will only venture to anticipate the contents of this very valuable report so far as to say that it will be found of very high interest both in respect to the temperature of the sea at great e Verrier'.s ' Bulletin ' for Sept. 4-8 , 1860 .
140 [ Nov. 30 , Anniversary Meeting .
depths , and to the nature of the sea-bottom , and the life existing in its vicinity .
The report strongly recommends the continuation and extension of these researches-a recommendation which in due time will require and receive the attention of your Council , who may confidently anticipate that should a further application to the Admiralty be deemed desirable it will receive favourable consideration , and , if approved , will be secure of the same cordial and invaluable cooperation on the part of the Hydrographer as that which has been enjoyed on this occasion .
We have to rejoice in the safe return of the Swedish and North-German Expeditions , engaged in the past summer in the endeavour to extend the domain of Arctic Exploration to the north and to the west .
Though the limits previously attained have not been passed in either direction , much valuable information has been obtained regarding the Natural History of Northern Lands , as well as many important facts bearing on the Hydrography of the Arctic Seas ; while an experience has been gained in Arctic navigation , and habits acquired of surmounting the difficulties which it presents , that may yield good fruit hereafter .
The Arctic explorations of the Swedes included , from their commencemenit , the design of accomplishing such a preliminary survey of Spitzbergen as might solve the question of the practicability of the measurement of a degree of the meridian in that high latitude .
The idea of such an undertaking having originated in this country and in this Society more than forty years ago , it is natural that we should regard the steps taken towards its accomplishment with a lively sympathy .
A sketch of what was effected in 1861 and 1864 by MM .
Chydenius , Diiner , and Nordenskiold , communicated to the Royal Society by Captain Skogman , of the Royal Swedish Navy , was printed in the Proceedings of December 1864 .
An official and elaborate Report has since been published ( in Sept. 1866 ) by the Royal Swedish Academy , entitled " :Foirberedande Undersikningar rorande Utforbarheten af en Gradmitning pi Spetsbergen " ( preliminary researches touching the facilities for a measurement of a degree at Spitzbergen ) , by MM .
Diiner and Nordenskiold ( Chydenius having unfortunately died ) .
In the Map accompanying the Report the triangles are laid down which connect the extremes of land , and comprehend an arc of about 4 ? ?
11 ' .
One of the objects contemplated by the expedition which has just returned was , to examine the possibility of the extension of the arc to lands existing to the north of the north-easternmost part of Spitzbergen-a question , however , which cannot be regarded as yet perfectly solved , the northern progress of the ' Sophia ' having been stopped by ice , which is described by M. Nordenskiold as " consisting in part of fields of drift-ice , covered with particles of earth , which seems to indicate that land is to be met with further north .
" Should these preliminary researches and surveys eventuate in a Scandi1868 .
] Presidents Addressnavian arc-measurement at Spitzbergen , I need scarcely say with what interest such an undertaking would be regarded by this country and by its Royal Society .
With reference to the operations of the Committee , appointed at the Nottingham Meeting of the British Association , for the Exploration of the Tertiary Plant-beds of North Greenland , it was stated in my last Address that a large collection of fossil plant-remains had been brought from Greenland by Mr. Edward Whymper .
The entire collection has been sent , for examination and description , to Prof. Oswald Ieer , of Zurich , who has already published a work , ' Flora Fossilis Arctica , ' containing the results of his examination of the fossils brought at various times from Greenland and other parts of the arctic regions and deposited in the museums of this country and of Denmark and Sweden .
The Committee , finding that their funds were exhausted , made a fresh application to the Government-Grant Committee , and received an additional sum to defray the expense of carriage of the specimens to and from Zurich .
The collection was forwarded to Switzerland at the end of last year ; and within the last week Prof. Heer has sent the description of the fossils to London , with the view of submitting it to the Royal Society .
The localities which were examined by Mr. Whymper were situated on the shores of the Waigat , at two points on Disco Island , and at Atanekerdluk , on the mainland of Greenland .
From Disco , whence specimens had only once been obtained before ( by Dr. Lyall ) , 14 species were procured .
Among them the occurrence of two cones of Magnolia present the greatest interest , as they prove to us that an evergreen , such as Mlagnolia , could ripen its fruit at the high north latitude of 70 ? .
The collection from Atanekerdluk is especially rich , but this locality was well known before ; the number of species from it in this collection is 73 .
Among the most important of these are the flowers and fruit of a Chestnut , proving to us that the deposits which contain them must have been formed at different seasons , corresponding to the times of flowering and fruit of the Chestnut .
The collection is not rich in animal remains ; however , some insects have been noticed , as well as a freshwater bivalve , probably Cyclas .
" The results of this expedition have been eminently satisfactory , whether we look to the number of new species discovered , or to the additional facts , confirmatory of previous determinations , which have been ascertained .
This latter remark is of special importance when we find that the identification of a tree by means of its leaves has been supported by the subsequent discovery of its flowers and fruit .
Thenumber of fossil species of vegetable remains discovered in Green land has increased to 137 , of which 46 , or exactly one-third , belong to it in common with the Miocene deposits of Europe .
Four of these are found in our own Bovey Tracey beds , which have been already described by Prof. Heer in the ' Philosophical Transactions .
' Among these is Sequoia Couttsice , the commonest tree in the British locality .
Accordingly the age of the Greenland deposits has been fixed beyond a doubt as Lower Miocene .
The collection itself is expected to arrive in London shortly , when a complete series of the specimens will be deposited in the British Museum , in accordance with the terms prescribed by the British Association and the Government-Grant Committee of the Royal Society .
The redaction of the great scientific work , the Mfagnetic Survey of the South Polar Regions-commenced in 1839 , under the auspices and at the expense of Her Majesty 's Government has been completed in the present year by the presentation to the Royal Society , and the publication in the Philosophical Transactions , of Maps of the three Magnetic Elements in Southern Parallels , commencing in 30 ?
south , and extending far beyond the limits of ordinary navigation .
These Maps are accompanied by Tables containing the numerical coefficients to be employed in a revision of ' Gauss 's General Theory , ' at the intersection of every fifth degree of latitude and every tenth degree of longitude , between 30 ?
south latitude and the south terrestrial pole .
The magnetical determinations of the Survey correspond to the epoch 18421 .
Similar Maps for the corresponding latitudes of the Northern Hemisphere , from 30 ?
north latitude to the north terrestrial pole , are in preparation , founded on a coordination of results obtained by magneticians of all countries in the fifteen years preceding and the fifteen years following the same mean epoch of 1842 , and reduced to it .
It is hoped that these Maps , with an accompanying Memoir , will be presented to the Royal Society before the close of the present session .
There will then remain for subsequent completion the filling up ( still for the same epoch ) of the space between the parallels of 30 ?
north and 30 ?
south latitude , for which much preparation has been made in the assemblage of materials , requiring only , for their coordination , the allotment of the time needed for the due examination and treatment of so large a body of materials .
Should I be so happy as to be able to complete this task also , ( my occupation in Terrestrial Magnetism has now extended , more or less , over half a century , ) I venture to express a hope that the great work of which the foundation will thus have been laid , viz. " the Revision of the Gaussian Theory , corresponding to a definite epoch in the great cycle of terrestrial magnetism , " may , when a suitable time shall appear to have arrived , be taken up and completed under the auspices of the Royal Society .
Whilst on the subject of Terrestrial Magnetism , I may remark that , in a recent number of his Wochenberichte , ' Dr. Lamont has called the attention of magneticians to the probable occurrence of the epoch of maximum of the magnetic disturbances at the end of the present year 1868 , in accordance with the hypothesis of a decennial period , and has noticed the already great increase in the number of days of unusual magnetic disturbance observed at Munich in the months of August , September , and October last .
Coincidently with Dr. Lamont 's experience in this respect , the continuous records of the magnetometers at Kew have shown larger and more frequent magnetic disturbances than usual ; and the Photoheliographs , taken there on all days when the sun is visible , have shown larger and more numerous groups of sun-spots .
It may be worthy of remark in this connexion , that 1868 is the fourth decennium since the occurrence of the first well-ascertained maximum of magnetic disturbance ; I mean that which , resting on the authority of Arago 's admirable and systematic series of observations ( 1821-1830 ) , has been shown to have taken place in 1828 * .
It may be proper , however , to await the more decisive evidence which the years 1873 to 1879 may afford , as to the preference to be given to either of the periods assigned by different magneticians ( respectively 10 and 11-jll years ) as the duration of this remarkable phenomenon , which appears to attest the simultaneity of physical affections of the sun and of the earth .
If the decen , nial hypothesis be correct , 1873 will be the year of minimum , and 1878 that of maximum ; if , on the other hand , the period be one of 11 years and a small fraction , 1873 should be the year of maximum , and 1878 the year of minimum ; and the order of progression and sequence be reversed .
I mentioned in my last year 's Address that the operations of the Bombay Observatory were delayed by the non-reception of the necessary self-recording magnetical and meteorological instruments of the best modern construction .
I am glad to be able to state on this occasion that a communication which I ventured to make to Sir Stafford Northcote , Secretary of State for India , had the immediate effect of removing the difficulty which had intervened , and that advice has recently been received of the safe arrival of these instruments at Bombay .
We may now confidently anticipate that , under the able and zealous superintendence of M1r .
Chambers , the Bombay Observatory will speedily take a place in the first rank of institutions specially devoted to these two branches of Physical Science .
A paper of considerable interest and importance , entitled " Scientific Exploration of Central Australia , " was presented to the Society in April last .
The geographical and scientific researches of its author , Dr. Neumayer , published under the authority of the Victorian Government , attest 'his competency to discuss a subject of this magnitude in its various points of view .
The paper itself is an able and interesting one ; it contains the outline of a large and apparently well-considered scheme , with estimates and other essential details ; it contemplates an expedition to last three or four years , starting from the eastern shores of Queensland , and terminating in an exploration of the western portion of the Australian continent ; and he offers his own services for the conduct of such an undertaking .
Should the plan find favour with the different Australian Colonies who would bear its expense and reap the chief material advantage of its results , there can be no doubt of its producing a rich harvest in physical geography and natural history , and as little doubt of the warm interest it would command in the Scientific Societies of the mother country , especially in the Royal Society , and of the pleasure with which they would give to it every assistance in their power .
I proceed to the award of the Medals .
The Copley Medal has been awarded to Sir Charles Wheatstone , F.R.S. , for his researches in Acoustics , Optics , Electricity , and Magnetism .
The researches of Sir Charles Wheatstone in acoustics , optics , electricity , and magnetism , numerous and important as they are , have already taken their place as integral parts of science , and have become so completely incorporated into its teaching that it will be hardly necessary on the present occasion to do more than enumerate the leading ones , in recognition of which the Copley Medal has this year been awarded .
The earliest of these researches in point of time were those connected with acoustics ; and among these we may mention a paper on the transmission of sound through solid conductors , which ( in 1828 ) describes the means discovered by the author of transmitting musical performances to distant places , where they are made audible by sounding-boards through the intervention of wires or wooden rods .
His paper on the acoustic figures of vibrating surfaces was published in the ' Philosophical Transactions ' for 1832 .
In this the laws of the formation of the varied and beautiful figures discovered by Chladni were first traced .
His subsequent invention of the Kaleidophone furnished him with an elegant means of showing optically the coexistence of different forms of vibrations in sounding bodies .
His wave-machine furnished a still more complete method of demonstrating the composition of undulations by mechanical means .
In optics his contrivance of the Stereoscope and the Pseudoscope , and his discussion of the modes in which binocular vision is effected , described in the ' Philosophical Transactions ' for 1838 and 1852 , were even more ingenious and important , as showing us how we obtain a perception of solidity or relief , or of its reverse , by the simultaneous observation of two plane images .
Another ingenious optical invention was the Polar Clock , described to the British Association at their Meeting in 1849 .
This is an instrument which indicates the time by means of the changes of polarization of the blue light of the sky in the direction of the pole , founded on the discoveries of Arago and Quetelet .
In 1835 he communicated to the British Association a paper on the Prismatic Analysis of the Electric Light , proving that the electric spark from different metals presents for each a different spectrum , exhibiting a definite series of lines , differing in position and colour from each other , and thus enabling very small fragments of one metal to be distinguished with certainty from all the others .
This was a starting-point in a new and fertile field of physical inquiry which has abundantly rewarded the labours of subsequent investigators .
But no series of his researches have shown more originality and ingenuity than those by which he succeeded in measuring the velocity of the electric current and the duration of the spark .
The principle of the rotating mirror employed in these experiments , and by which he was enabled to measure time to the millionth part of a second , admits of application in ways so varied and important that it may be regarded as having placed a new instrument of research in the hands of those employed in delicate physical inquiries of this order .
Scarcely less valuable are the instruments and processes which Sir Ch. Wheatstone devised for determining the constants of a voltaic circuit , including , among others , the rheostat and the differential resistance measurer ( or Wheatstone 's bridge , as it is usually called ) , which , in one or other of its modifications , is become an indispensable means of measuring the resistance of telegraphic wires and cables , as well as for determining electromotive forces .
The description of these methods is contained in a paper in the 'Philosophical Transactions ' for 1843 .
But it is with the Electric Telegraph that the name of Sir C. Wheatstone is in the public mind most completely identified ; and ever since the first messages were transmitted along the Great Western Railway by insulated copper wires enclosed in iron tubes , to the present day-when a network of copper wires insulated by means of caoutchouc is suspended across our public thoroughfares for the instantaneous transmission of intelligence , not merely from one district to another in our large towns , but from one continent and capital to another-Sir C. Wheatstone has not ceased to contribute the most important aid towards perfecting the means of electrotelegraphic communication .
A bare enumeration of these various inventions would carry us beyond our limits on the present occasion .
In 1840 he devised a cable adapted for transmitting intelligence under the sea ; and it is to him that we are indebted for the Alphabetic Dial Telegraph working without any clockpower , and in which a magneto-electric machine supplies the place of a voltaic battery .
These instruments were first used in the Paris and Versailles Railway in 1846 .
A more recent invention is his High-Speed Telegraph , in which the messages , previously prepared on slips of paper , are , by passing through a very small machine constructed somewhat on the principle of the Jacquard Loom , made to print the messages at the remote station , in the ordinary telegraphic characters , with a rapidity unattainable by the hand of an operator .
Allied to these inventions are others where electro-magnetism is the motive power , as , for example , the electro-magnetic clock for telegraphing time , a modification of which has since been employed to aid in determining the longitude of distant places ; also the Chronoscope , for measuring the velocity of projectiles or falling bodies .
In this enumeration of his discoveries , inventions , and researches , we have passed over many , such as his speaking machine , the investigation of Fessel 's Gyroscope , his experiments in illustration of Foucault 's proof of the rotation of the earth , and others .
More than enough , however , has been stated to justify the presentation of the Copley Medal on this occasion to our eminent fellow-countryman .
SIR CHARLES WHIEATSTONE , I have the very agreeable duty of presenting to you this Medal , which you will receive as a testimony of the sense so universally entertained by your countrymen , and specially by the Fellows of the Royal Society , of the high scientific merit and practical value of your many discoveries and inventions , and of their varied applications .
The Council has awarded a Royal Medal to the Rev. Dr. George Salmon , Regius Professor of Divinity in the University of Dublin , for his original investigations on Analytical Geometry , published in the Transactions of the Royal Irish Academy and in the Philosophical Transactions , and , specially , for his solution of the problem of the degree of a surface reciprocal to a given surface-and for his researches in connexion with surfaces subject to given conditions , analogous to those of Chasles in plane curves .
Besides the original investigations thus referred to , Dr. Salmon is the author of a series of works on Conic Sections , on higher Plane Curves , on Geometry gof Three Dimensions , and on higher Algebra ( the modern Analysis ) , full of original matter of great value to the advanced mathematician , and at the same time adapted to the requirements of the student .
These works have become widely spread as text-books throughout Europe ; and the estimation in which they are held is attested by the fact that they have already been translated into French , German , Italian , and Russian .
DR. SALMON , I have the pleasure of presenting you this Medal in testimony of the high estimation in which your attainments and labours in the higher branches of mathematics are held by the Royal Society .
A Royal Medal has been awarded to Mr. Alfred Russell Wallace , in recognition of the value of his many contributions to theoretical and practical zoology , among which his discussion of the conditions which have determined the distribution of animals in the Malay archipelago ( in a paper on the zoological geography of that region , published in the Proceedings of the Linnean Society for 1859 ) occupies a prominent place .
The case may be briefly stated thus:-The strait separating the islands of Baly and Lembok is only fifteen miles wide ; nevertheless the animal inhabitants of the islands are widely different , the fauna of the western island being substantially Indian , that of the eastern as distinctly Australian .
Mr. Wallace has described , in a far more definite and complete manner than any previous observer , the physical and biological characters of the two regions which come into contact in the Malay archipelago ; he has given an exceedingly ingenious and probable solution of the difficulties of the problem , while his method of discussing it may serve as a model to future workers in the same field .
Another remarkable essay , " On the tendency of Varieties to depart indefinitely from the Original Types , " published in the Proceedings of the Linnean Society for 1858 , contains an excellent statement of the doctrine of Natural Selection , which the author , then travelling in the Malay archipelago , had developed independently of Mr. Darwin ; and , apart from its intrinsic merits , this paper will always possess an especial interest in the history of science , as having been the immediate cause of the publication of the ' Origin of Species .
' Mr. Wallace 's ability as an observer and describer of animal forms is shown in his numerous and valuable contributions to our knowledge of the animals , and especially the Pigeons , Parrots , and Butterflies , of the Malayan region .
It must not be forgotten that a knowledge of the circumstances under which the majority of these contributions to the higher branches of zoological science were made must greatly enhance our respect for the author .
Mr. Wallace has spent the greater part of his life amidst the exhausting and often dangerous fatigues of a traveller in tropical countries rarely explored by Europeans ; and some of his most valuable papers are dated from places which some might consider so little favourable to study as Ternate and Sarawak .
MiR .
WALLACE , I have the pleasure of presenting to you this Medal in recognition of the great merit of your researches both in practical and theoretical ZoologZ-y , carried out in countries where such pursuits are necessarily attended with .
more than usual difficulties and dangers.8 The Rumford Medal has been awarded to Mr. Balfour Stewart , for his researches on the qualitative as well as quantitative relations between the powers of emission and absorption of bodies for heat and light , published originally in the Transactions of the Royal Society of Edinburgh and in the Proceedings of the Royal Society of London , and now made more generally accessible by the publication , in 1866 , of his treatise on heat .
When a body is placed within an opaque envelope which is kept at a constant temperature , it soon acquires the temperature of the envelopeand that , whatever be the nature or form of the envelope or of the body .
The same is true if any number of bodies of different kinds be placed within the envelope ; in the permanent state each of the bodies attains a fixed temperature , the same as that of the walls of the envelope .
The equilibrium of temperature is not , however , of the nature of statical equilibrium ; according to the theory by which Prevost so beautifully explained the apparent radiation of cold , each body radiates heat all the while , at a rate depending only on its nature and temperature , and not at all on its environment ; and it is because the other bodies and the envelope are also radiating heat , and the first body absorbs a portion of the radiant heat thus falling upon it , that its temperature remains unchanged .
The equality of radiation and absorption follows as a simple corollary .
It had long been known that rock-salt is remarkable for its transparency for obscure radiant heat .
According to Melloni , a plate of rocksalt of the thickness of three or four millimetres transmits 92 per cent. of heat-rays from whatever source .
Now , on measuring by the thermopile the radiation from thin and thick plates of rock-salt , as well as from two or more plates placed one behind the other , all being heated up to a definite temperature , 3ir .
Stewart found that the radiation from a thick plate , or from many plates , was , indeed , greater than from a thin plate or from a single plate , but that the difference was not by any means so great as it ought to have been on the supposition that the heat radiated by the hinder portion of a thick plate , or by the hinder plates of a group , passed through the front portion of a thick plate , or through the front plate of a group , as freely as obscure heat would have passed which was radiated by lampblack or most other substances .
It thus appeared that rock-salt at any temperature is by no means transparent to heat radiated by rock-salt of the same temperature-that it exerts a preferential absorption on rays of the quality of those which it emits .
This conclusion was confirmed by using a plate of cold rock-salt as a screen by which to sift the heat-rays falling on the thermopile .
It was found that a much larger proportion of the heat was stopped by the screen when the source of heat was a plate of heated rock-salt than when it was a body coated with lampblack .
The proportion stopped was also sensibly greater when the source of heat was a thin than when it was a thick plate of rock-salt , the reason being that the heat radiated from the hinder portion of a thick plate was partially sifted , in passing across the front portion , before it reached the rock-salt screen , and therefore was transmitted by it in greater proportion than the heat which radiated from the front portion .
Similar conclusions were obtained from experiments on glass and mica , though the numerical results were not so striking , in consequence of the comparatively great opacity of those substances for obscure radiant heat .
It thus appeared , 1st , that the heat radiated by a body is not confined to that which comes from the immediate neighbourhood of the surface , but emanates from various , in the case of rock-salt considerable , depths ; 2ndly , that there is a relation between the quality of the heat radiated and that absorbed by any given element of a body , and consequently by a sufficiently thin plate of a body , of such a nature that the kind of heat most freely radiated is also most freely absorbed .
These results and others were comprehended by Mr. Stewart in a definite theory , by means of his extension of Prevost 's theory of exchanges .
According to this extension , the stream of radiant heat within a uniformly heated enclosure is the same throughout in quality as well as quantity ; i. e. the uniformity of radiation exists for each kind of heat in particular of which the total flux is made up .
Few now can doubt the identity of nature of radiant heat and light ; and , accordingly , the application to light of the extension of Prevost 's theory was an obvious step .
This step was taken by Mr. Stewart , who verified by experiment that which theory predicted-that a coloured glass when heated , as compared with an opaque body glowing at the same temperature , gives out by preference rays of the kind which it absorbs , and consequently tends to glow with a colour complementary to its own .
For a similar reason a plate of tourmaline cut parallel to the axis , when heated , and viewed in a direction perpendicular to the axis , is seen to glow with light which is partially polarized in a plane parallel to the axis .
It is right to mention that , in regard to the extension of Prevost 's theory in its application to light , Mr. Stewart was slightly anticipated by Professor Kirchhoff , whose brilliant application of the theory to the lines of the spectrum has attracted general attention , whose researches , however , had hardly , if at all , reached this country when Mr. Stewart 's papers were presented .
As regards Radiation , however , without specifying of what kind , the priority in the extension of Prevost 's theory belongs to Mr. Stewart , whose papers on Heat were published before those of Professor Kirchhoff , to whom , however , they were not known when he published his earlier papers .
MR. STEWART , I have particular pleasure in presenting to you this Medal , because it will testify to you that all that really conduces to the advance of our knowledge meets sooner or later with its due recognition-and because I hope that this tribute to your earlier labours will be especially agreeable to you now that you are engaged in work of high public value , but which must necessarily leave you little leisure for such original researches .
On the motion of 8ir Charles Lyell , seconded by Sir Thomas Watson , it was resolved , - " That the thanks of the Society be returned to the President for his Address , and that he be requested to allow it to be printed .
" The Statutes relating to the election of Council and Officers having been read , and Sir Edwin Pearson and Mr. Erasmus Wilson having been , with the consent of the Society , nominated Scrutators , the votes of the Fellows present were collected , and the following were declared duly elected as Council and Officers for the ensuing year : President.-Lieut.-General Sabine , R.A. , DX .
C.L. , LL. D. Treasurer.--William Allen Miller , M.D. , D.C.L. , LL. D. Secretaries._ William Sharpey , M.D. , LL. D. cretaries .
George Gabriel Stokes , Esq. , M.A. , D.C.L. , LL. D. Foreign Secretary.-Prof .
William lallows Miller , M.A. , LL. D. Other Members of the Council.-Frederick Augustus Abel , Esq. ; Sir Benjamin Collins Brodie , Bart. , M.A. ; William Benjamin Carpenter , M.D. ; J. Lockhart Clarke , Esq. ; Frederick Currey , Esq. , M.A. ; Warren De La Rue , Esq. , Ph. D. ; Sir William Fergusson , Bart. ; William Henry Flower , Esq. ; Capt. Douglas Galton , C.B. ; John Peter Gassiot , Esq. ; John Hawkshaw , Esq. ; John Marshall , Esq. ; Joseph Prestwich , Esq. ; George Henry Richards , Capt. R.N. ; Archibald Smith , Esq. , M.A. ; Lieut.-Col. Alexander Strange .
Reeipts and Payments of the Royal Society between Decenber 1 , 1867 , and -overber 30 , 1868 . ? .
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251 50 Dimvdends ... ... ... ... ... ... ... ... ... ... ... ... ... . .
145 ... .
1455 67 Ditto , Trust Funds ... ... ... ... ... ... ... ... ... ... . .
280 12 4 Sale of Transactions , Proceedings , &c. ... ... ... ... ... ... ... ... ... 371 01 RepavmeAts ... ... ... ... ... ... ... ... .1 ... ... ... ... ... ... ... ... .
41 7 8 ?
4780 5 1 ?
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342 15 0 Instruments for India and freight ... ... ... ... ... ... ... ... ... ... 293 50 Books for the Library and Binding ... ... ... ... ... ... ... ... ... 219 90 Printing Transactions and Proceedings , Paper , Binding , Engraving , and Lithography ... ... ... ... ... ... ... ... ... ... . .
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r0 !
'I ; I iIi1fI II i i/ Scientific Relief Fund .
Investments up to July 1865 , New 3 per Cent. Annuities ... ... ... ... ... ... ... ... ... ... S6052 17 8 ?
6052 17 8 ?
s. d , I ' Balance ... ... ... ... ... ... ... . .
197 6( 0D onation ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... . .
500D ividends ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... .
7 0 ?
379 70 Statement of Icome and Expenditure ( apart from Trust Fvsnds ) d uritg the Year ending November 30 , 1868 .
Annual Subscriptions ... ... ... ... ... ... ... ... ... .
Admission Fees ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... . .
Compositions ... ... ... ... ... ... ... ... ... ... ... ... .
R ents ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... Dividends on Stock ( exclusive of Trust Funds ) ... ... ... .
, on Stevenson Bequest ... ... ... ... ... ... ... ... ... . .
Sale of Transactions , Proceedings , &c. ... ... ... ... ... ... ... ... Cost of Instruments , repaid ... ... ... ... ... ... ... ... ... ... ... ... Chemical Society , Tea Expenses ... ... ... ... ?
18 0 01 Linnean Society , Tea Expenses ... ... ... ... ... 14 0O Geographical Society , Gas at Evening ' 84 AM eetings ... ... ... ... ... ... ... ... ... ... ... ... ... J Caminbridge Local ExaminationCommittee , Gas 3 12 0 Sundry Petty Receipts ... ... ... ... ... ... ... ... ... ... ... ... ... . .
Income available for the Year ending Nov. 30 , 1868 ... ... Expenditure in the Year ending Nov. 30 , 1868 ... ... ... ... Excess of ' lncome over Experiditure in the Year ending ] ov .
, 30 , 18,8 ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... S s. d. 1049 40 160 00 376 00 251 50 1006 62 449 05 371 01 284 18 6 $32 00 it ]8 12 12 6 4004 34 3899 11 7 ?
104 11 9 00 oll .
C ?
r. .
cS 5 .
d. Salaries , Wages , and Pension ... ... ... ... ... ... ... ... ... ... ... 1037 60 The Scientific Catalogue ... ... ... ... ... ... ... ... 342 15 0 Instruments for India and freight ... ... ... ... ... ... .
293 50 Books for the Library ... ... ... ... ... ... ... ... ... ... ... ... ... .
122 11 3 Binding ditto ... ... ... ... ... ... ... ... ... ... ... ... ... 96 17 9 Printing Transactions , Part II .
1867 , and 8 Part .
1868 ... ... ... ... ... ... ... ... ... ... ... ... .
Ditto Proceedings , Nos. 96-104 ... ... ... ... ... 289 18 6j Ditto Miscellaneous ... ... ... ... ... ... ... ... ... . .
68 6 .
5 1651 13 10 Paper for Transactions and Proceedings ... 311 46 Binding and Stitching ditto ... ... ... ... ... ... . .
92 10 9 Engraving and Lithography ... ... ... . .
480 52 Fittings , Cleaning , and Repairs ... ... ... ... ... ... ... ... ... ... ... 45 44 Miscellaneous Expenses ... ... ... ... ... ... ... ... ... ... ... ... ... . .
37 10 6 Coal , Lighting , &c. ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... 130 73 Tea Expenses ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... 54 14 11 Fire Insurance ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... . .
28 11 6 Taxes ... ... ... ... ... ... ... ... ... ... ... ... ... .
10 11 .
3 Advertising ... ... ... ... ... ... ... ... ... ... ... ... ... ... ... . .
12 10 6 Postage , Parcels , and Petty Charges ... ... ... ... ... ... ... ... ... 35 12 6 ?
3899 11 7 WILLIAM ALLEN MIILLER , Treasurer .
e Pir .
clS Q Cl-I cc 023 The following Table shows the progress and present state of the Society with respect to the number of Fellows : Patron and Foreign .
CTotnal .
R oyal.pounders .
yearly .
yearly .
RToyal .
November 30 , 1867 .
5 48 298 2 264 617 Since elected ... ... +4 +7 +9 +20 Since re-admitted. .
l1 Since compounded. .
+1 --1 Since deceased ... -1 17 -12 -34 Since withdrawn. .
-1 -Defaulters ... ... . .
-3 November 30 , 1868 .
4 48 289 2 257 600
|
112369 | 3701662 | On the Phenomena of Light, Heat, and Sound Accompanying the Fall of Meteorites | 155 | 160 | 1,868 | 17 | Proceedings of the Royal Society of London | W. Ritter v. Haidinger | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1868.0022 | null | proceedings | 1,860 | 1,850 | 1,800 | 6 | 109 | 3,090 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112369 | 10.1098/rspl.1868.0022 | http://www.jstor.org/stable/112369 | null | null | Biography | 33.364131 | Headmatter | 25.652806 | Biography | [
17.34786605834961,
-39.758697509765625
] | I. " On the Phenomena of Light , Heat , and Sound accompanying the fall of Meteorites .
" By W. RITTER V. HAIDINGEt , For .
Mem. R.S. &c. Received October 6 , 1868 .
A particular incident caused me to return to some portions of my earlier studies in regard to meteors and meteorites .
It was the fall of a meteorite at Kakowa on the 19th of May 1858 that first induced me to bestow some more attention on this department of physical science .
A report on the subject I laid before our Imperial Academy of Vienna on the 7th of January , 1859 .
On the same day also I gave the first list of the meteorites forming the meteorite collection in our Imperial Mineralogical Museum .
A series of reports on meteorites followed , as well as a number of catalogues of meteorites , in accordance with the growing riches of the collection , embracing from 137 to 236 numbers of localities preserved up to the date of July 1 , 1867 .
But the studies relating to the recent fall of Ausson on the 9th of December 1858 , and the ancient fall of the meteoric iron of HIraschina , near Agram , on the 26th of May 1751 , others on the Cape meteorites of 1838 , on those of Shalka , 1850 , Allahabad , 1822 , Quenggouk ( Pegu ) , 1857 , Assam , found 1846 , Segowlee , 1853 , St. Denis-Westrem , 1855 , Nebraska , found 1356 , but particularly some studies relating to meteorites of Stannern , 1858 , and of that most remarkable meteoric iron from Tula , discovered in 1856 by Auerbach , all of them within the period of 1851 to 1860 , and then the fall of New Concord , 1860 , and of Parnallee , 1857 , had forcibly called upon me to draw up , as it were , a general rule of the nature and succession of events which probably might have taken place in the history of their existence , though in each particular case only fragments of that history came to our notice .
A general survey of this kind I had the honour to lay before our Imperial Academy on the 14th of March 1861 , " On the nature of Meteorites , relating to their composition and the phenomena of their fall"* .
I felt , it is true , that I had rather too boldly ventured to transgress the limits of my former studies ; but at the same time , led on by the high interest connected with the subject , I wished to gain some more publicity for it .
As to England , I was most kindly and effectively patronized by that energetic promoter of meteoritic science my most honoured friend Mr. R. P. Greg .
He laid a notice of mine before the British Association for the Advancement of Science , held that year at Manchester , and accompanied it with several considerations of his own T ; then , also , he kindly had the pages of the Philosophical Magazine opened for me , and presented me with an edition of separate copies of a memoir on the subject-nearly a translation , by my honoured friend Count A. F. Marschall , of my original communication to our Academy y. At the Meeting of German naturalists and physicians at Speyer , my honoured friend Dr. Otto Buchner kindly called the attention of the friends of this department of natural science to my memoir , which had been favourably mentioned in the reports .
A note of mine , containing the leading views of my papers , was likewise laid by my honoured friend M. Elie de Beaumont before the Paris Academnie des Sciences in their Meeting of September 9th , 1861 , while I also sent a French translation by my excellent friend Count Marschall , together with a copy of my original memoir ? .
Since that time , up to this day , I had frequently , in several communications on meteoritic subjects , had an opportunity to refer to these leading papers , and to support the views which they contained .
Therefore I had every reason to be astonished when I read , in a recent work on meteorites by M. Stanislas Meunier l , the following assertion:- " ' We may observe that a great number of particular phenomena occurring in the fall of meteorites have hitherto remained without explanation .
Thus the reason of the ex* " Ueber die Natur der Meteoriten in ihrer Zusammensetzung und Erscheinung , " Sitznngsberichte der Kaiserlichen Akademie der Wissenschaften , der MI.athem.-naturw .
Class , 1861 , Band xliii .
Abth .
ii .
S. 389-425 .
t " An attempt to account for the Physical Condition and the Fall of Meteorites upon our Planet , by W. Haiclinger , Hon. Memb. E.S.L. & E. &c. , " Report , 1861 , Transactions of the Sections , p. 15 .
" Some Considerations on M. Haidinger 's Communication on the Origin and Fall of Aerolites , by R. P. Greg , F.G.S. , " ibid. p. 13 .
$ Considerations on the Phenomena attending the Fall of Meteorites on the Earth , by W. Iaidinger , For .
Memb. R.S.L. & E. ; and Philosophical Magazine for November and December 1861 . ?
" De la nature des bolides et de leur mode de formation .
Lettre de M. iaidinger , " Comptes Rendus hebdomadaires des seances de l'Acad6mie des Sciences etc. t. liii .
Juillet-Decembre 1861 , pp. 456-461 .
II Etude , descriptive , theorique , et experimentale sir les Meteorites , par M. Stanislas Meunier .
Paris , 1857 , p. 18 .
plosions , and particularly of the repeated explosions , that of the rumblings , that of the incandescence , are still absolutely unknown " * .
But I had still more reason to be astonished when I found M. Daubr6e himself nearly upon the same level in his views respecting the origin of light , heat , and sound in the fall of meteorites .
I certainly heartily appreciate the high merit of my honoured friend M. Daubree , in regard both to his deep studies on meteorites and his eminent success in forwarding the interests of the Paris Museum of Meteorites ; but I at the same time may be permitted to consider my own views , as given in the memoirs quoted , as representing a scientific advance compared with the statements of M. leunier and those of M1 .
Daubree himself in his last memoir on the Orgueil fall f. Neither M. Daubree nor M. Meunier had refuted or even objected to my views ; they had only passed them over in silence , doubtless because they had escaped their notice .
But I believe I am fulfilling a duty to scientific progress if I endeavour to place the discrepant and even contradictory views on these subjects together , with the view once more to excite attention and recommend them to further study on the part of the votaries of natural science ; and it was with this view that I prepared a new memoir , to be laid before our Imperial Academy in their approaching period of session , on the light , heat , and sound accompanying the fall of meteorites .
I begin with some of the statements put forth by M. Daubre'e , as taken from his memoir on Orgueil : " Things go on as if the greater part of the mass of the meteor got out of our atmosphere , in order to continue its course , after having left us some particles , the velocity of which , in consequence of the explosion , was reduced " 4 .
M. Daubree does not admit the arrival of groups or swarms of meteorites as has been asserted ? .
" The carbonaceous meteorites contradict the hypothesis that the heat of the meteorites is due to the loss of their vis viva " 1 .
The sounds , detonations under the name of explosions , remain without explanation ?
[ .
M. Daubree attributes to mere chance the situation of what he calls " scales , " or " ecailles de meteorites , " at the moment of an explosion , if they present certain particular seams of crust surrounding their most ex* " ' emarquons qu'un grand nombre de particularites offertes par la chute des met6orites sont restees jusqu ' " pr6sent sans explication .
Ainsi , la cause des explosions et surtout des explosions multiples , celle des roulements , celle de l'incandescence , sont absolument inconnues .
" f " Complement d'Observations sir la chute de meteorites qui a eu lieu le 14 My 1864 aux environs d'Orgueil , " Nouvelles Archives da Museum d'HIistoire Naturelle , t. iii .
pp. 1-19 .
+ " Les choses se passentldone comme si la plus grande party de la mass me6torique ressortait de l'atmosphere pour continuer sa trajectoire , n'abandonnant que quelques parcels dont la vitesse , a la suite de l'explosion , se trouvait amortie."-Op .
cit. p. 15 . ?
Comme on 'a dit .
1| " Les meteorites eharbonneuses contredisent l'hypothese que la chaleur des meteorites est due a la perte de leur force vive."-Op .
cit. p. 8 .
[ " Sans explication."-Op .
cit. p. 16 .
tended surface , by which , being foremost , they forced their way through the opposing atmosphere .
In regard to this position I had long ago advanced that it must have been a necessary result , while the rectilinear movement of the meteorite was in the way of being checked , of part of the force having been expended in producing a rotatory motion , perpendicular to the direction of the course .
This I did in particular , in a paper on the meteoric iron of I-raschina , on the 14th of April 1859 , then on an aerolite from Stannern on the 22nd of May 1862 , and in other instances .
The above-mentioned quotations of M. Danbree 's views are now compared with the successive periods of progress in the fall of meteorites , nearly in the same words as I proposed them in 1861 .
In the arrival of meteorites on our earth:1 .
Single or agglomerated fragments , in their cosmical course , come into contact with our globe .
2 .
The fragments are arrested by the resistance of atmospheric air .
3 .
Pressure , in their progress through the atmospheric air , elicits light and heat ; rotation ensues , and a melted crust is formed .
4 .
The white-hot compressed air is spread out in the form of a fireball , closed up behind , and enclosing the fragment , or fragments , and a vacuumspace .
5 .
The cosmic course is at an end when the fragment , or the fragments , have been arrested by air .
6 .
Light and heat are no longer generated ; the vacuum-ball will collapse with a loud report , or several reports following each other .
7 .
The cosmic cold within the aerolite assists in reducing the heat of the melted crust .
8 .
The meteorite falls down upon the earth like any other ponderous body , the hotter the better conducting material it consists of .
In this way I believe it was my duty again to lay before the public the differences of the views newly taken by M. Daubree from those which I hitherto had advocated .
But while w was engaged in contrasting them I found myself conspicuously supported by a number of recent publications relative to the subject in question .
In one of his own papers M. Daubree had to register the statement of M. Leymerie , of Toulouse , who considered the fall of Orgueil as presenting not one meteoric mass exploded , but a swarm of aerolites arrived at the same moment .
But above all , two reports of the fall of 30th January 1868 , near Pultusk , both of them kindly presented to me by their respective authors , bore ample testimony in favour of a number of my theses , and enlarged them by deeper and more accurate investigation beyond what I formerly proposed .
These are the memoir " On the Course of the Pultusk Meteorite " * , by Ueber die Bahn des am 30 .
Januar 1868 beobachteten und bei Pultusk imr Konigreiche Polen als Steinregen niedergefallenen Meteors durch die Atmosphare .
Voin Professor Dr. C. G. Gall , Direktor der Sternwarte zu Breslau .
Vorgetragen am 4 .
158 [ Dec. 10 , Professor J. G. Gall in Breslan , and another , " On the Meteorites of Pultusk " * , by Professor G. vom Rath , in Bonn .
In both of them the most evident proofs are given of the actuality of a swarm , consisting of a very great number of distinct airolites , having entered our atmosphere .
The course of the Pultusk meteor , according to M. Gall , met the horizontal line under an angle of 44 degrees at the place of dispersion , at a height of 25'25 English miles , or 5German miles .
After its movement was checked , and the force of it expended in the development of light and heat , how would it have been possible that , as it would follow from M. )aubree 's supposition , the great mass of the meteor should have risen again and left our atmosphere to continue its cosmical orbit ?
Nor could such be the case with the Knyahinya meteor , which pounced upon our earth almost from the zenith of the place , the course making an angle only of 6 degrees with the perpendicular .
But even the Orgueil meteor moved in a direction meeting the horizontal line at the point of dispersion under an angle of about 11 26 ' , from which position it certainly could not rise again higher up into the atmosphere , and still less leave it altogether .
I availed myself of the circumstance that I had been gratified by several honoured friends with a number of important publications closely connected with the subject , to quote some appropriate passages .
I would refer especially to that grand 'Atlas of Charts of Meteor-tracks , ' by Messrs. R. P. Greg and A. S. Herschel t , together with the " Reports of Luminous Meteors for the years 1865 and 1866-1867 " , and to the recent memoir by M. G. V. Schiaparelli on the astronomical theory of falling stars ?
, kindly sent to me by the late lamented Mlatteucci .
Schiaparelli holds forth that in shootingstars " the vis viva , while the meteoric matter is dispersed in the atmosphere , is completely destroyed by being transformed into heat and light " II .
From Maiirz u. s. w. Besonderer Abdruck aus den Abhandlungen der Schlesischen Gesellschaft fur vaterlandische Cultur .
Breslau , 1868 .
Mr. A. S. Herschel 's observations with the spectroscope , we learn that the condition of the August meteors is exactly that of a flame of gas in a Bunsen 's burner freely charged with the vapour of burning sodium , or of the flame of a spirit-lamp newly trimmed and largely dosed with a supply of moistened salt ( op .
cit. p. 146 ) .
The idea of a diminutive fireball containing the solid mass , although diminutive itself , surrounded by a luminous gaseous case , including a vacuum , till the force of the movement is spent in heat and light , may not be considered inadequate to the subject .
In a most interesting memoir entitled c " Contributions to the Knowledge of Falling Stars " * , by Dr. Edmond Weiss , of Vienna , that able astronomer ( the representative , together with Dr. Oppolzer and Lieut. Reziha , of the Austrian Navy , of our Austrian expedition for the eclipse of 18th of August at Aden , where they were so hospitably welcomed and kindly supported by the Governor-General , J. Russell , in behalf of the British Government , along with the North-German expedition , composed of Drs. Vogel , Fritsche , Zenker , and Thiele ) considers among other subjects the influence of the earth 's attraction upon shower-meteors , independently of Schiaparelli 's disquisitions relative to the same subject , and points out also the circumstance that some of them may receive such a direction as to leave our solar system altogether , while Dr. Gall insists upon the fact that the Pultusk swarm must have entered it with an independent force of at least from 4 , to 7 English miles ( 1 to 1 !
geographical miles ) .
My original design was only to offer some appropriate remarks on the subject of the phenomena of light , heat , and sound generated in and accompanying the arrival of meteorites on the earth through our terrestrial atmosphere ; but the different departments of natural science referring to meteors and meteorites are of so manifold a nature , that I frequently was obliged to advert to some of them in regard to which I should rather have kept more on the reserve .
But the whole range of meteorand meteoritescience , continually enlarging , more and more clearly presents itself in these four grand sections:-lst , the original formation of meteorites ; 2nd , their movement through cosmic space ; 3rd , their arrival through the atmosphere upon our earth ; and , 4th , the studies instituted on the objects themselves , which fall into our hands and are preserved in our museums .
To the third of these sections it is that my particular attention was directed .
ei Beitrage sir Kenntniss der Sternschnuppen , von dem c. M. Dr. Edmund Weiss .
Vorgelegt in der Sitzung am 16 .
Janner 1868 , " Sitzungsberichte der Math.-nat .
Class der Kais .
Akademie der Wissenschaften , lvii .
Band ii .
Abth .
5 .
pp. 281-342 .
[ Dec. 10 ,
|
112370 | 3701662 | On the Solar and Lunar Variations of Magnetic Declination at Bombay.--Part I. [Abstract] | 161 | 163 | 1,868 | 17 | Proceedings of the Royal Society of London | Charles Chambers | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 54 | 1,046 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112370 | null | http://www.jstor.org/stable/112370 | null | null | Meteorology | 91.012154 | Tables | 7.108635 | Meteorology | [
46.42936706542969,
7.341024875640869
] | II .
" On the Solar and Lunar Variations of Magnetic l)eclination at Bombay."-Part I , By CHARLES CHAMBERS , Esq. , Superintendent of the Colaba Observatory .
Communicated by B. STEWART , LL. D. Received June 30 , 1868 .
( Abstract .
) The hourly observations of magnetic declination at the Government Observatory , Bombay , have extended over a period of nearly a quarter of a century , but the present discussion is confined to the observations made in the seven years 1859 to 1865 .
After describing the instrument with which the observations were made and the method of ' reducing them , the writer exhibits , by means of Tables and curves , the following results:1st .
The agreement of the diurnal variation of the aggregate of easterly disturbances when different separating values are adopted .
2nd .
The same for the aggregate of westerly disturbances .
3rd .
The diurnal variation of the aggregate of easterly disturbances , exceeding 1'4 in amount , in the period of seven years .
4th .
The same for westerly disturbances .
5th .
The disturbance-diurnal variation , or the excess at each hour of the aggregate of easterly over the aggregate of westerly disturbances .
6th .
The aggregates of easterly , westerly , and easterly and westerly disturbances , and the numbers of disturbed observations in each month of the year .
7th .
The aggregates of easterly , westerly , and easterly and westerly disturbances , and the numbers of disturbed observations , in each of the years 1859 to 1865 , and in the period of seven years .
8th .
The solar-diurnal variation of declination in each month of the year , and for the whole year .
9th .
The excess of the diurnal variation of declination for each month over the mean diurnal variation for the year .
10th .
The mean diurnal variation of declination for the half-years April to September and October to March , in each of the years 1859 to 1865 .
11 th .
The semiannual inequality in the mean diurnal variation of declination .
12th .
the mean diurnal variation of declination for each of the years 1859 to 1865 .
13th .
The calculated values of the coefficients A. , B , A2 , B2 , A3 , and B3 in the equation h =A1 cos n +B1 sin +A2 cos 2n +B2sin2n+A3 , cos3n+B 3 sin 3n + &c. . .
, which expresses the mean diurnal variation of declination for each month of the year , for the whole year , and for different half-years .
14th .
The same for the half-years April to September and October to March , in each of the years 1859 to 1863 .
15th .
The solar-diurnal inequality of declination , in the calculation of which all disturbances are included .
16th .
The variation from year to year in the range of the mean diurnal variation of declination 17th .
The secular change and semiannual inequality of absolute declination .
The diurnal variations of disturbance , both easterly and westerly , are found to be of definite and systematic character , and to be comparable with the same variations for other places ; the annual variation is not very regular , but the progression in the amounts of disturbance in different years accords well ( with exception as to the incomplete year 1861 ) with the known character of the decennial variation .
The mean diurnal variation of declination , as well as its semiannual inequality , is of the general character due to the latitude in which Bombay lies ; the progression from month to month in the annual variation of the diurnal variation is also distinctly marked in all months except July .
A semiannual inequality is shown to exist in the diurnal variation of declination whose times of opposition are the equinoxes .
It is found that this inequality not only exists , but has the same general character at five widely separated stations in the northern magnetic hemisphere , and also , with some modifications as to character , at two stations having south magnetic latitude .
Its special characteristics are : 1st .
That , as in the typical mean diurnal variation of declination , there is scarcely any change during the night hours , and that the main variation occurs during half the day , in this case between 18 hours and 6 hours , local astronomical time .
2nd .
That the range of variation differs from about half a minute to nearly a minute of arc .
3rd .
That the hour of noon is that about which the deviations due to this variation pass through zero , and on each side of which the inflexions of the representative curve are inversely , but , in respect to north latitude stations , symmetrically disposed .
4th .
The turning-points are 21 hours and 3 hours , the former being a maximum , and the latter a minimum for north latitude stations from January to June , and for south latitude stations from July to December ; and vice versa , for north latitude stations from July to December , and for south latitude stations from January to June .
The solar-diurnal inequality of declination , in the calculation of which all disturbances are included , differs at no hour of the day by more than 0'061 from the mean diurnal variation , which is calculated after the rejection of all observations disturbed to the extent of more than 1 ' 4 .
The range of the diurnal variation of declination in different years is shown to be subject to a periodical variation , whose times of maxima and minima approach nearly to those of the maxima and minima of the decennial period in the amount of yearly disturbance .
The secular change of absolute declination is found for the years 1859 to 1865 to be an annual increase of easterly declination of 3"017 ; the semiannual inequality to be an excess of 0'"227 of easterly declination in the months October to March over its value in the months April to September .
|
112371 | 3701662 | On the Diurnal and Annual Inequalities of Terrestrial Magnetism, as Deduced from Observations Made at the Royal Observatory, Greenwich, from 1858 to 1863; Being a Continuation of a Communication on the Diurnal Inequalities from 1841 to 1857, Printed in the Philosophical Transactions, 1863. With a Note on the Luno-Diurnal and other Lunar Inequalities, as Deduced from Observations Extending from 1848 to 1863. [Abstract] | 163 | 165 | 1,868 | 17 | Proceedings of the Royal Society of London | George Biddell Airy | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 3 | 46 | 1,468 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112371 | null | http://www.jstor.org/stable/112371 | null | null | Meteorology | 75.520522 | Tables | 14.269051 | Meteorology | [
45.32904815673828,
10.667115211486816
] | III .
" On the Diurnal and Annual Inequalities of Terrestrial Magnetism , as deduced from observations made at the Royal Observatory , Greenwich , from 1858 to 1863 being a continuation of a communication on the Diurnal Inequalities from 1841 to 1857 , printed in the Philosophical Transactions , 1863 .
With a Note on the Luno-diurnal and other Lunar Inequalities , as deduced from observations extending from 1848 to 1863 .
" By GEORGE BIDDELL AIRY , Astronomer Royal .
Received July 27 , 1868 .
( Abstract .
) The author states that the instruments employed are precisely the same which were used in the second part of the former investigation , from 1848 to 1857 , mounted in the same place , and treated in the same manner .
In describing the treatment of the photographic curves , he first gives the number of days which have been omitted in different years ; because the character of the observations or curves was too disturbed to permit the usual treatment of the observations , or the drawing by hand of a pencil curve that would fairly represent the general course of the curve .
The greatest numbers of omitted days occur in the years 1846 , 1847 , 1848 ; 1851 , 1852 , 1853 , 1854 ; 1859 , 1860 .
As the estimate of the amount of irregularity has been made throughout by the same person , he considers that these years may be accepted as those in which the disturbances were the greatest .
If they point to any cycle at all , it is one of 6 or 6years .
These days being omitted , the ordinates of the pencilled curves on the other days were used as basis of ' all the following investigations .
For the solar inequalities , they were treated by collecting the measures for every complete solar day , or for every solar hour bearing the same ordinal number , according as the annual or diurnal inequalities were the subject of inquiry ; but in all cases these quantities were next grouped by months , and the monthly means were taken .
In the further treatment , the means of the monthly means of every complete day for all the months of the same name in the different years were taken and corrected for secular change ; the corrected numbers do not appear to indicate any sensible annual equation .
Then the means of the monthly means of every solar hour for all the months of the same name in the different years were taken , giving the diurnal inequalities on the mean of years for the twelve separate months ; and these present , for the declination ( north to west ) and horizontal force , for the period 1858 to 1863 , sensibly the same differences between the summer months and the winter months as those for the period 1848 to 1857 .
For the vertical-force -163 curves also , the nodal passage in both periods is earliest in the summer months ; but it is not quite certain whether the curves in autumn , in the period 1858 to 1863 , are quite so bold as those in 1848 to 1857 ; the difference , however , if any , is inconsiderable .
After this , the monthly means of every solar hour are taken through each year , giving the mean diurnal inequality of each year ; and here a very remarkable change is observable .
To explain this , it is necessary to refer to the former paper , where it is shown that the curves for diurnal inequality of the horizontal forces had very slightly increased from 1841 to 1847 , but had rapidly diminished from 1848 to 1857 , giving the smallest and most winter-like curves in 1856 and 1857 .
Now it is found that from 1858 to 1863 the curves have increased , with a little irregularity in 1861 , till they are sensibly as large as they were at first .
Thus1858 nearly resembles 1856 1859 , , , 1851 1860 , , , 1850 1861 , , , , 1851 1862 , , , , 1847 1863 , , , 1841 With regard to the diurnal inequality of vertical force , it appears that the curves gradually increased in boldness to 1855 , and have gradually diminished to 1862 .
The nodal passages , it was remarked in the former paper , had been much accelerated in the hour of the day , from 1842 to 1857 .
Now , from 1858 to 1863 , the hours of nodal passages have been retarded , till in 1863 they are again nearly the same as in 1848 .
In all these remarkable changes there is no appearance of cycle .
The author then proceeds to the treatment of lunar inequalities from 1848 to 1863 .
The bases of their treatment were thus obtained : the exact time of moon 's transit was laid down on the time-scales of the photographic sheet , and the intervals were divided into lunar hours , and a new system of ordinates , corresponding to the lunar hours , was measured to the pencil curves .
The system of grouping was precisely similar , mutatis mutandis , to that for the solar inequalities .
First , for the menstrual inequalities .
The declination seems to exhibit a distinct lunar menstrual inequality , with + maximum about the fifth day of lunation ; the horizontal force seems to show a lunar semimenstrual equation with maximum about the second day ; the vertical force shows nothing certain , proving only that , if there is anything , it is very small .
Secondly , for the lunodiurnal inequalities .
The luno-diurnal inequalities in declination and horizontal force on the mean of 1858 to 1863 agree so closely with those on the mean of 1848 to 1857 , as to leave no doubt of their existence and law as luno-semidiurnal inequalities , with no trace of luno-diurnal or other inequality .
Remarking the singular difference for different years which has presented 164 [ Dec. 10 , itself in the discussion of the solar inequalities , it appeared to the author very desirable to examine whether there is any discoverable difference in the lunar inequalities for the same years .
The years were accordingly thus divided : Large solar curves. .
1848 to 1852 , 1859 , 1860 , 1862 , 1863 .
Small solar curves. .
1853 to 1858 , 1861 .
On discussing these , it was found that in all cases the lunar horary epoch for the inequality was sensibly the same for years of large solar curves and for years of small solar curves ; but the coefficient was different .
The value of the fraction lunar semidiurnal inequality in years of large solar curves lunar semidiurnal inequality in years of small solar curves is For declination ... ... ... .
1 35 For horizontal force ... . .
125 The author remarks that it would seem possible to suggest two conjectural reasons for this remarkable association in the time-law of changes of solar effect and lunar effect .
One is , that the moon 's magnetic action is really produced by the sun 's magnetic action ; and a failure in the sun 's magnetic power will make itself sensible , both in its direct effect on our magnets and in its indirect effect through the intermediation of the moon 's excited magnetism .
The other is that , assuming both actions ( solar and lunar ) to act on our magnets indirectly by exciting magnetic powers in the earth , which alone or principally are felt by the magnets , the earth itself may have gone through different stages of magnetic excitability , increasing or diminishing its competency to receive both the solar and the lunar action .
The epochs of lunar inequality in western declination from north and in horizontal force to magnetic north are sensibly the same ; and the coeffi .
cients expressed in terms of horizontal force on the mean of all the years are sensibly the same , and equal to 0'000061 .
The direction of the composite disturbing force is therefore sensibly N.W. and S.E. magnetic , or ( roughly ) in the direction of a line from the Red Sea to the south of Hudson 's Bay .
It may be remarked in opposition to this that the solar diurnal action is mainly in the S.W. direction .
The luno-diurnal inequality of vertical force on the mean of all the years appears to consist of a luno-diurnal and a luno-semidiurnal term .
|
112372 | 3701662 | On the Measurement of the Luminous Intensity of Light. [Abstract] | 165 | 167 | 1,868 | 17 | Proceedings of the Royal Society of London | William Crookes | abs | 6.0.4 | null | null | proceedings | 1,860 | 1,850 | 1,800 | 2 | 34 | 1,097 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112372 | null | http://www.jstor.org/stable/112372 | null | 112,416 | Optics | 56.085542 | Measurement | 16.494728 | Optics | [
9.019428253173828,
-20.467262268066406
] | I. " On the Measurenent of the Luminous Intensity of Light .
" By WILLIAM CRooKEs , F.R.S. &c. Received June 27 , 1868 .
( Abstract .
) The measurement of the luminous intensity of a ray of light is a problem the solution of which has been repeatedly attempted , but with less satisfactory results than the endeavours to measure the other radiant forces .
The problem is susceptible of two divisions , the absolute and the relative measurement of light .
A relative photometer is one in which the observer has only to ascertain the relative illuminating powers of two sources of light , one of which is kept as uniform as possible , the other being the light whose intensity is to be determined .
It is therefore evident that one great thing to be aimed at is an absolutely uniform source of light .
In the ordinary process of photometry the standard used is a candle , defined by Act of Parliament as a " sperm of six to the pound , burning at the rate of 120 grains per hour .
" This , however , is found to be very variable , and many observers have altogether condemned the employment of test-candles as light-measures .
The author has taken some pains to devise a source of light which should be at the same time fairly uniform in its results , would not vary by keeping , and would be capable of accurate imitation at any time and in any part of the world by mere description .
The absence of these conditions seems to be one of the greatest objections to the sperm-candle .
It would be impossible for an observer on the continent , ten or twenty years hence , from a written description of the sperm-candle now in use , to make a standard which would bring his photometric results into relation with those obtained here .
Without presuming to say that he has satisfactorily solved all difficulties , the writer believes that he has advanced some distance in the right direction , and pointed out the road for further improvement .
A glass lamp is taken of about 2 ounces capacity , the aperture in the neck being 0 25 inch in diameter ; another aperture at the side allows the liquid fuel to be introduced ; this consists of alcohol of sp. gr. 0-805 , and pure benzol boiling at 81 ?
C. , which are mixed together in the proportion of five volumes of the former and one of the latter .
The wick-holder consists of a platinum tube , and the wick is made of fifty-two pieces of platinum wire , each 0-01 inch in diameter .
The flame of this lamp forms a perfectly shaped cone , the extremity being sharp , and having no tendency to smoke ; without flicker or movements of any kind , it burns when protected from currents of air at a uniform rate of 136 grains per hour .
There is no doubt that this flame is very much more uniform than that of the sperm-candle sold for photometric purposes .
Tested against a candle , considerable variations in relative illuminating power have been observed ; but on placing two of these lamps in opposition , no such variations have been detected .
The instrument devised for measuring the relative intensities of the standard and other lights is next described ; it has this in common with that of Arago described in 1833 , as well as with those described in 1853 by Bernard , and in 1854 by Babinet , that the phenomena of polarized light are used for effecting the desired end* .
But it is believed that the present arrangement is quite new , and it certainly appears to answer the purpose in a way which leaves little to be desired .
The instrument cannot be described without the aid of drawings which accompany the original paper , but its mode of action may be understood by the following description .
The standard lamp being placed on one of the supporting pillars which slide along a graduated stem , it is moved along the bar to a convenient distance , depending on the intensity of the light to be measured .
The light to be compared is then fixed in a similar way on the other side of the instrument .
On looking through the eyepiece two brightly luminous disks will be seen , of different colours .
One of the lights must now be slid along the scale until the two disks of light , as seen in the eyepiece , are equal in tint .
Equality of illumination is easily obtained ; for , as the eye is observing two adjacent disks of light which pass rapidly from red-green to green-red , through a neutral point of no colour , there is no difficulty in hitting this point with great precision .
Squaring the distance between the flames and the centre will give inversely their relative intensities .
The delicacy of this instrument is very great .
With two lamps , each about 24 inches from the centre , it is easy to distinguish a movement of one of them to the extent of one-tenth of an inch to or fro , and by using the polarimeter an accuracy exceeding this can be attained .
The employment of a photometer of this kind enables us to compare lights of different colours with one another .
So long as the observer , by the eyepiece alone , has to compare the relative intensities of two surfaces respectively illuminated by the lights under trial , it is evident that , unless they are of the same tint , it is impossible to obtain that absolute equality of illumination in the instrument which is requisite for a comparison .
By the unaided eye one cannot tell which is the brighter half of a paper disk illuminated on one side with a reddish , and on the other with a yellowish light ; but by using the photometer here described the problem becomes practicable .
When the contrasts of colour are very strong ( when , for instance , one is a bright green and the other scarlet ) there is difficulty in estimating the exact point of neutrality ; but this only diminishes the accuracy of the comparison , and does not render it impossible , as it would be according to other systems .
|
112373 | 3701662 | Preliminary Report of Dredging Operations in the Seas to the North of the British Islands, Carried on in Her Majesty's Steam-Vessel Lightning | 168 | 200 | 1,868 | 17 | Proceedings of the Royal Society of London | William B. Carpenter|Dr. Carpenter|Wyville Thomson | fla | 6.0.4 | http://dx.doi.org/10.1098/rspl.1868.0026 | null | proceedings | 1,860 | 1,850 | 1,800 | 35 | 509 | 19,609 | http://corpora.clarin-d.uni-saarland.de/surprisal/6.0.3/?id=112373 | 10.1098/rspl.1868.0026 | http://www.jstor.org/stable/112373 | null | null | Geography | 44.7134 | Biography | 19.429866 | Geography | [
58.30256652832031,
11.912785530090332
] | II .
" Preliminary report , " by Dr. WILLIAm B. CARPENTER , V.P.R.S. , " o of Dredging Operations in the Seas to the North of the British Islands , carried on in Her Majesty 's Steam-vessel 'Lightning , ' by Dr. CARPENTER and Dr. WYVILLE TIIOMSON , Professor of Natural History in Queen 's College , Belfast .
" Received October 22 , 1868 .
In accordance with the request of the President and Counlcil of the Royal Society , conveyed in the Letter written by their direction to the Secretary to the Admiralty on the 18th of June ( Appendix ) , the Lords Commissioners of the Admiralty were pleased to give their sanction to the scheme for Deep-sea Dredging therein proposed , and to furnish the means of carrying it out as effectively as the advanced period of the season might permit .
2 .
The Surveying-ship 'Lightning ' was assigned for the service , and was furnished with a " donkey-engine , " and with all other appliances iequired for the work , together with the most approved Sounding-apparatus* and Thermometers .
The vessel was placed under the charge of Staff-Comnmander May , who had been much erngaged in exploratory service elsewhere ; and the instructionis given to him were so framed as to enable him to carry out my wishes in every practicable way .
3 .
I was accompanied by my fiiend Professor Wyville Thomson , with whom the idea of this inquiry had originated , and to whose zealous and efficient cooperation I have been greatly indebted in the prosecution of it .
His large previous experience in Dredging-operations , and his extensive knowledge of the Marine Fauina , not merely of Great Britainl , but of the Scandiniavian and Boreal provinices , have supplied much that would otherwise have been deficient on my own part ; and hie has shown hinmself ever ready to relieve me of the more laborious part of the work we had jointly undertaken .
Although it has beenl deemed fitting that , as it was by rue that the proposal for this inquiry was brought before the Royal Society , and as I was enttrusted by the Admiralty withi the direction of it , this IReport of its proceedings should proceed from myself , I have the satisfaction of saying that it has the fuill conicuLrrence of my able Coadjutor.-I was permitted to take with me one of my sonls as an Assistant ; and we were all three considered as in the Public Service , and liberally providled for accordingly .
4 .
It is with great pleasure that I am able to state that the results of 12* 310 e 30 ' : o 30 tt 0 tl§ 3 ' 73 6.5 ) Clhart to rieeompany l^:-@#4r > *:| ~18681Y rL a t.t~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~u .
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2w 6v a.42i 234 238 .
78 VIE ... ... ... ... . .
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50ODr .
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70 A 27 40 2 68 78 52 30 4,50 50 27.2 40 06 23 AM.86 0 80 06 _tB-mL 42 43 W.0 40 48 20 87 iffRENEY IV '24 as a 42 60 4Z .
ii 40 'OS .
" 40 2I-'-46 40 , 4g , ; , v 4w,.V 36 42 42 227.94 ' 42 47 46 M ?
.W 39.0 4.3 -43 40 J7 40 4o 48 r2 as 40 40 22 40 44 27 Jo so 54 %_ " .70 21 2 " 40 43 20 ' ( 33 49 !
-.30 ' e-a Jo 26 3M6 .
87.62 48. .
N. , Nortk46 jo se F5 'M IIEBRIDYS za , S. 70 80 28 30 27 63 66 20 __J.W .
306* 3030,.110 ' 30 ' Eugrwn & by Mal'oy So= our inquiries have been , in all essential particulars , fully as satisfactory as we had ventured to anticipate .
The lateness of the date at which the Expedition started ( its departure from Stornoway having beeni necessarily delayed until August 11 th ) , and the consequent limitation of the time during which deep-sea dredging would be likely to be practicable , precluded the idea that the present inquiry could be more than tentative , anything like a systematic exploration of the Marine Zoology of the area we proposed to traverse being scarcely to be expected .
In poilnt of fact , during the four weeles which elapsed between our first departure from Stornoway and our return to it on September 9th , only nine days were available for dredging in the open ocean ; and on onlyfour of these were we on a bottom exceeding 500 fathoms [ 914 metres ] in depth ; and in our second cruise of a week 's duration , we only dredged once .
Yet , as will hereafter appear , we have been enabled , by this very limnited amount of work , not only to add many new and interesting facts to science , in regard both to the Physics and the Animal Life of the Ocean ; but also to correct serious errors which have been sanctioned by high authority , and to lay a definite foundation for mxiore extended inquiries directed towards the solution of various genleral questionis of the highest importance .
5 .
On the day after our first departure from Stornoway ( August 12 ) we were met by a breeze from the N.E. , so strong that , although a sounding was obtained in lat. 590 20 ' N. and long .
70 5 ' W. , which indicated a depth of at least 500 fathoms [ 914 matres ] , with a minimnum temperatuire of 49 ?
[ 90.4 Cent. ] , the temperature of the surface-water being 5420 [ 12'-5 Cent. , any attempt to dredge was out of the question .
6 .
This breeze lasted with considerable force for three days , dturing which , being compelled to lie-to under canvas , we drifted to the northward of the deep water ; ouir first soundi:lgs after its abatement ( Auguist 15th ) giving depths of 229 and 164 fathoms [ 419 and 300 metres ] respectively , with a minimunm temperature of 480 [ 80.9 Cent. ] , the temperature of the surface-water being 54 [ 12 ` 2 Cent. ] .
As we were then approaching the Faroe Banks , we considered it expedient to devote a couple of days to the examination of the distribution of Animal Life at these comparatively moderate depths , and then to proceed to the Faroe Islands , reserving the deeper water for our retuirn voyage .
7 .
The average depthi of the Faroe Banks is about 60 fathoms [ 110 m'tres ] , and their miniminum temperature was found to be about 50 ?
[ 100.0 Cent. ] when the temperature of the surface was 530 [ 1 ` 6 Cent. ] .
The character of the Marine Invertebrate Faun-a of this region exhibited the admixture of British and of Boreal types , which might be expected from its temperature and geographical position , the former decidedly predominating .
The comu-mon Ophiocomna rosula of our own shores ( Ophiothrix fragilis of Miiller and Trroschel ) presents itself in very great abunldance , and probably furnishes an importanit part of the food of the Cod which frequent these balnks .
8 .
We reached Thorsaven on the morning of August 17th ; and , as the weather was then fine , we applied ourselves without delay to the exploration of the Fiords in its vicinity , using for this purpose the boats of the country , with native boatmen , whose knowledge of the tides and currents was indispensable to us .
Unfortunately the weather again became so unfavourable as to prevent us from extending our inquiries to more distant localities , at the same time that the low state of the barometer rendered it inexpedient to put to sea again for the prosecution of our special object * .
We found , however , that the Shells of the straits and fiords of the Faroes had been carefully collected by Sysellman Muller , who has long been in the habit of availing himself of the opportunities for dredging afforded by his official visits to different parts of the group ; and that a List of the Mollusea found in them has been recently published by Dr. 0 .
A. L. Mdrch t. The result of our own dredgings , taken in connexion with the in-formation obtained from these sources , leads us to believe that furthec exploration in this locality is not likely to bring out facts of any special interest .
The tides and currents in the Straits between the islands are so strong as to render the deepest parts of the mid-channels ( in which alone could any novelty be anticipated ) an unsuitable habitation for Marine Invertebrata ; and in the long narrow fiords which extend from these between the elevated ridges of Trap that traverse the interior of the islands the water is seldom of any considerable depth , and probably contains a large admixture of fresh water from the almost continuous rainfall which here prevails .
The general character of the Marine Zoology of the Faroes , as of their adjacent banks , seems to be just what might be expected from their position on the border between the British , Scandinavian , and Boreal provinces .
9 .
At the first indicationi of improvement in the weather , we left Thorsaven on the 26th of Auigust , with the intenition of reaching the deep channel which we expected to find lying E. and W. , between the North of Scotland and the Faroe Banks , as soorn as possible , and of exploring this channel as completely as we might be able .
At the end of our first day of steaming southwards , however , we encountered a gale from the S.W. , in the course of which the barometer fell to 29 inches , and which was severe enough to do much damage to our ship ; and it was not until the afternoon of August 29th that , after lying-to for nearly three days under canvas and drifting to the N.E. , we were able to obtain a Sounding in lat. 60§ 451 and long .
4049 ? .
This gave us a depth of 510 fathoms [ 933 mnetres ] ; and the two thermometers sent down with the lead gave a minimum of 330 [ 0§ 5 Cent. ] and 34Y ' [ P14 Cent. ] respectively , the temperatuire of the surface-water being 52 ?
[ 110 1 Cent. ] .
10 .
This very remarkable indication was fully colnfirmed the next morning , when we sounded again in lat. 60§ 71 and long .
50 21 ' , and found the depth to be 500 fathoms [ 914 mretres ] , and the minimum temperature , as giveni by the mean of three thermometers* ( showing 31 ?
[ 0 2 Cent. ] , 320 [ 0 " Cent. ] , and 330 [ 00.5 Cent. ] respectively ) , to be 32§ 2 [ 0 ?
1 Cent. ] , the temperature of the surface-water being 510 [ l0`5 Cent. ] .
11 .
We here for the first time had an opportunity of working our Dredge at this great depth , and found no difficulty in doing so .
The bottom consisted of sand and stones ; and it is important to remark that the same kind of bottom was met with in all our subsequent soundings and dredgings in the " cold area " ( §§ 12-14).-As might have been anticipated from the extraordinary reduction of the Temperature , there proved to be a comparative scantiness of Animal life ; and of the forms which did present themselves , several belonged to the Boreal Fauna .
Still there were examples of several different groups ; and there was not that predominance of low forms which some have supposed to characterize the Fauna of great depths .
Indeed the Rlizopoda , of which we afterwards encountered an extraordinary development at the like depth , but in a much warmer temperature , were almost entirely absent .
It is worthy of note that a specimen of Astropecten of a bright red colour came up adherent to the dredge-line at a distance of 250 fathoms [ 457 metres ] from the dredge , about 1200 fathoms [ 2195 metres ) of line being out .
As this animal is entirely unprovided with swimming-organs , and was found to be of such specific gravity as to sink immediately when placed in a jar of sea-water , it can scarcely have been taken up anywhere else than from the sea-bottom ; and if this be admitted , it is obvious that at least 250 fathomns [ 457 metres ] of the dredge-line must have been lying oln that bottom .
Not only on many subsequent occasions did Ophiurida come up on the like part of the dredge-line , but in our last dredging ( § 19 ) , from a depth of 65.0 fathoms [ 1189 metres ] , there came up attached to it , at a distance of abouit 50 fathoms [ 92 mretres ] from the dredge , two pieces of a Siliceous Sponge , which most assuredly could not have been drawn from any other source than the sea-bottom t , and which included many small living Ophiurida .
e It had been our intention to make a careful comparison of each of these Thermometers with an accurate standard on our return , and thus to have determined with greater pre .
cision the temperatures they respectively indicated ; but two of them were unfortunately lost in a subsequent Sounding ( § 19 ) .
t From this it is obvious that the Dredge-rope , so far from buioying up the Dredge , must effectually assist in sinking it , especially when the rope has been solidified by previous repeated immersions at great de-pths .
I find the specific gravity of a portion of our dredge-rope , which has been thus subjected to a pressure of 118 atmospheres , to be 1347 , that of Sea-water being about 1029 .
In our earlier dredgings , we attached one or two couples of 12-lb .
shot to the dredge-line at a short distance from the dredge , so as 12 .
The weather again interfered with the prosecution of our irnqu'iry , which had now become of most unexpected interest ; but we were able on the morning of September 1st to obtain a Sounding , in lat. 60§ 10 ' and long .
5 ' 59 ' , which ftully confirmeed our previous observations .
The depth was here 550 fathoms [ 1006 metres ] , and the minimum temperature indicated by the mean of two thermometers* ( which stood at 3 1i7 and 32 ?
` 5 respectively ) was 32 ?
[ 0 ?
Cent. ] , the surface-temperature being 530 [ 11`6 Cent. ] .
There was , however , too much wiind for dredging on that day .
13 .
On the following day ( Sept. 2 ) , in lat. 60§ 24 ' and long .
6§ 38 ' , our Sounding gave us a depth of oiily 170 fathoms [ 311 metres ] ; but even at this depth we found , with a surface-temperature of 52 ?
[ 11.l1 Cent. ] , a minimum temperature , indicated by the mean of two thermometerst ( which stood at 41k0 and 420 respectively ) , of 41 [ 50.4 Cent. ] , -that is , about 6 ?
[ 30.3 Cent. ] lower than the minimutm temperature we had found at a like depth when approaching the Faroe Banks ( § 6 ) , and 8 ?
[ 40.4 Cent. ] lower than tnat we subsequently encountered at the like depth when approaching the inorth coast of Scotlanid ( § 17 ) .
Our Dredgings here aforded evidence of a great abundance and variety of Animal life , Norwegian forms being mingled in a very marked manlner with British .
In particular we obtained a large number of specimens of Terebratula cranium of uniusual size , a beautiful delicately moulded arenaceous triradiate Foraminifer+ , and very large examples of a coarsely arenaceous Rhizopod closely correspondirig with the Lituola Soldanii of the Silurian Tertiaries .
14 .
On the following day ( Sept. 3 ) we again found ourselves in deep water , our Sounding , taken in lat. 600 28 ' and long .
60 55 ' , giving a depth of 500 fathoms [ 914 metres1 .
The mninimum indicated by the mean of three thermometers ( which registered 31 4 ?
, 33 ?
0 , and 340 respectively ) was 330 [ LO ?
5 Cent. ] , the temperature of the surface being 51 [ 100.5 Cent. ] .
I-Here , again , our Dredgings gave the same general results as those of previous dredgin , gs at the like depth and temperature ( § 11 ) ; and not only was our previous conclusion confirmed , that a pressure of 100 atmospheres is not incompatible with the existenice of num'ierous and varied forms of Animal life , but we had the gratification of obtaining a specimen of the remarkable Echinoderm Bri & inya ( one of the Norwegian types specially mentioned in Prof. Wyville Thomson 's letter ) , part of the arms of which to ensure its , handles being kept down upon the ground , in the position requisite for the ' biting ' of its edge ; but we soon becamne satisfied that this is effectually done by the weight of the dredge-rope itself , when it has once been deeply submerged .
A third Thermometer had been sent down ; but as it registered a minimum of 36§ 2 [ 2§ 3 Cent. ] , we thought it fair to presutme that its index had not been carried down as far as the real miniimum-a circumstance of frequenit occurrence .
t Our third Thermoineter stood on this occasion at 450 [ 70`2 C. ] ; and its reading has not been taken into account , for the reason stated in the preceding note .
+ This we believe to be the Rhabdammniga cabyssorum of Sars ; but as no description of the type has yet ( so far as we can learn ) been published by him , we are unable to identify it with certlainty .
came up on the dredge-rope , whilst other portions , with the body ( apparently belonging to one and the same individual ) , were found in the dredge .
15 .
The weather again occasioned for two days an interruption in our dredging ; and it did not even permit the use of the proper deep-sea sounding-apparatus .
But a sounding was taken on Sept. 5th , in lat. 60§ 30 ' and long .
70 16 ' , with the ordinary deep-sea lead , which showed that there was no bottom at 450 fathoms [ 822 metres ] , and gave a minimnum temperature , indicated by the mean of two thermometers ( which marked 330 and 352k respectively ) , of 334 ?
[ 0§ 7 Cent. ] , the surface-temperature being 500 [ 10 ?
0 .
Cent. ] .
16 .
It was then considered expedient to shape our course in a southerly direction ; and on the morning of September 6th we found ourselves in lat. 590 36 ' and long .
7§ 20 ' .
lIere a very careful Sounding gave a depth of 530 fathoms [ 969 mectres ] ; and the minimum temperature indicated by the mean of three thermometers ( which registered 47 ?
, 47k , ?
and 472 ?
respectively ) was 4730 [ 8§ 5 Cent. ] , the surface-temperature being 522 ?
[ l 104 Cent. ] .
This result fully confirmed that obtained by our first less satisfactory sounding in nearly the same locality ( § 5 ) , which the low ternperatures subsequently obtained with such uniformity in like depths elsewhere had led us to doubt.-We were able on this day to obtain several good casts of the Dredge , the results of which proved of extraordinary interest .
The bottom consisted of a bluish-white tenacious mud , containing but a small admixture of the Glo6igerince so abundantly obtained by previous soundings from various parts of the sea-bottom of the North Atlantic .
Imbedded in this mud there came uip an extraordinary collection of Siliceous Sponges , of new and most remarkable forms ; and with these was associated the Hyalonema Sie6oldii , which appeared to us clearly referable to that Family .
The Rhizopods found in this mud were scarcely less interesting ; for besides numerous specimens of the typically triradiate Rhabidammina alyssorum ( ?
) , presenting a varied range of forms , another large group of gigantic coarsely arenaceous bodies presented themselves , of the most varied shapes , apparently referable to the Astrorhiza limicola * as their fundamental type , together with a large and perfect living specimen of Cristellaria , closely resembling that common in the Siciliani Tertiaries , and a CGorniuspira of extraordinary size .
With these lower forms , our dredgings on this bottom brouight uip a considerable vrariety of higher tie pes , Zooplhytes , Eckizoderms , MIollusks , and Crustaceans ; amongwhich may be mentioned , as of special interest , two specimens of Rhiz-ocrigns , the small Apiocrinoid whose recent discovery by M. Sars on the coast of Norway ( see Appendix ) may be considered as having furnished a principal " ; motive " of our expedition , and a living Oculina prolhfera , of which we had on previous occasions brought up only dead and worn specimelns.-We thus obtained evidence of the existence , not of a degraded or starved-ouit residuum of Animal life , but of a rich and varied Fauna , including elevated as well as humble types , at a depth of 530 fathoms [ 969 metres ] .
This Fauna was essentially British in its general character , but included several types hitherto found only near the coast of Norway .
Since it presented itself on the southern border of the deep channel intervening between the North of Scotland and the Faroe Banks , these types must henceforth be considered to appertain equally to the British province .
17 .
As it was necessary for us to continue our course towards Stornoway , we were not able to prosecute further inquiries in this interesting locality , as we should otherwise have been most glad to do ; and on the morning of September 7th , in lat. 590 5 ' and long .
70 29 ' , a Sounding gave the comparatively small depth of 189 fathoms [ 345 mretres ] .
We found the minimum temperature , indicated by the mean of three thermometers ( respectively marking 49 O , 49 30 , and 49 I ' ) , to be here 49 ?
0 [ 9§ 8 Cent. ] , the surface-temperature being 520 [ 110 1 Cent. ] .
Here our Dredge brought up almost exclusively the ordinary types of the northern shores of Scotland , the chief features of interest being the great abundance of Cidaris papillata , and the occurrence of Antedon celticus ( Comatula celtica of Barrett ) , numerous specimens of which had been previouisly obtained off the coast of Ross-shire by Mr. J. Gwyn Jeffreys .
As we approached the land , the contents of the dredge became altogether barren of animal life , probably on account of the " scour of the strong currents and tides of this locality , and the stony character of its bottom .
In the Minch ( the channel between the Island of Lewis and the mainland ) the dredge again brought up a considerable number of well-known North British forms ; and at one of our casts it came up full of mud , sticking in which was an extraordinary number of livinog specimens of Pennatula .
18 .
We arrived at Stornoway on the afternoon of September 9 ; and here Prof. Wyville Thomson was obliged to leave us , in order to attend the Meetings of the Commission on Science and Art Instruction , of which he is a member .
As , however , the weather presented an uniusually settled aspect , and as the results we had already obtained led me strongly to desire an opportunity of examining both the Temperature and the Animal life of waters still deeper than any we had hitherto sounded , it was thought by Captain May and myself that , notwithstanding the lateness of the season , it would be worth while to venture another short cruise in a westerly direction , where we knew , from soundings previously taken , that a depth exceeding 1000 fathomxs ( 1829 metres ) is to be met with.-After refitting our ship and our dredging-apparatus at Stornoway , we left that harbour for a second t'ime on September 14 , and proceeded in a N.W. course , with the view of finding , in the latitude of the region which had given us a temperature of 320 [ 0 ?
Cent. ] at a depth of 500 fathoms [ 914 me'tres ] , but at some distance to the westward , still deeper water , and possibly a still lower temperature ( the freezing-point of sea-water being 270.4 [ -20.55 Cent. ] ) , and of then running southwards until we should find ourselves over the deep valley between the Western Hebrides and the Rockall Bank .
In this valley we hoped , from our previous success in working the Dredge at upwards of 500 fathoms , to be able , if weather should permit , to demonstrate the practicability of examining by its means the distribution of Animal life at twice that depth .
19 .
After a very fine run of 140 miles in a N.W. direction from the Butt of Lewis , we took a Sounding on the morning of Sept. 15 in lat. 590 59 ' , long .
90 15 ' , and found at 650 fathoms [ 1189 inetres ] a bottom of bluishwhite unctuous mud , very like that from which we had brought up the Siliceous Sponges ( § 16 ) .
The minimum temperature here indicated by the mean of three thermometers ( registering 450 , 46 ' , and 47 0 respectively ) was 460 [ 70.7 Cent. ] , the surface-temperature being 530 [ 110.6 Cent. ] .
As it was thus evident that we were in the warm , not in the cold area of bottom-temperature , we proceeded about 60 miles still further to the N.W. , and on the morning of Sept. 16 we sounded in lat. 60 ' 38 ' and long .
110 7 ' .
The depth'was here 570 fathoms [ 1043 metres ] ; and the scoop of the Sounding-apparatus brought up an almost pure Globigerina sand .
The minin'mum ' temperature indicated by two thermometers ( registering 46- ?
and 47'0 respectively ) was 470 [ 8 ?
03 Cent. ] , the surface-temperature being 52'.-Still looking for deeper water and a lower temperature , we proceeded about 50 miles further in the same direction ; and on the afternoon of that day took another Sounding in lat. 61§ 2 ' and long , .
120 4 ' , which gave a depth of 650 fathoms [ 1189 metres ] .
On this occasion our Sinker and three Thermometers were unfortunately lost by the parting of the line in winding-up , so that we did not ascertain either the nature of the bottom or the minimum temnperature ; but as we had now reached a latitude far north of that of the cold depths we had previously traversed ( being nearly that of the southern end of the Faroe group ) , we deemed it inexpedient to proceed further in this direction ; and a cast of the Dredge was therefore taken at this point , the depth being greater by 120 fathoms than any at which we had previously worked it .
We found no difficulty in this operation , notwithstanding that the dredge was loaded with about 2cwt .
[ 127 kilog .
] of whitish grey mud , of peculiar viscidity , brought up from a depth ( 3900 ' feet ) nearly equal to the height of the highest mountains in Great Britain .
At some 50 fathoms [ 92 metres ] from the dredge , two whitish tufts were seen on the dredge-rope ; and these proved to consist of portions of a Siliceous Sponge , quite free from the mud with which all the specimens previously obtained had been infiltrated .
As it is obvious that these specimens must have been detached by the dredge-rope in its passage over the surface of the mud ( § 11 ) , it seems clear that these Sponges , in part at least , project above that surface , which the infiltrated condition of those previously obtained had caused us to doubt .
On separating the different parts of the large mass of mud brought up by the dredge , we found it to be everywhere traversed by fibres , which proved to be long siliceous Sponge-spicules ; and our subsequent examination of these has shown them to be the root-fibxres of Sponges , the bodies of which have a siliceous framework of very different structure .
As it thus appears that these Siliceous Spongoes , when growing on the surface of the mud , send root-fibres ( so to speak ) far and wide into its substance , the idea previously suggested by Prof. Love'n , that the elongated flint-rope of HIyalonenza Sieboldii is in reality the mud-imbedded stem , supj)orting the Sponge with which it is connected , instead of beingo imp)llanted in the Sponge and supported by it ( which is the commonly received opinlioIn ) , seems the more likely .
This idea is thought probable by Prof. WVyville Thomson , who has already paid great attenition to the whole group , and by whomi all the niew forms we lave obtained will hereafter be fully described .
-Entangled among the fibres of the Sponge were found several small Opltiocomce , Polyzoa , Grustacea , and tubicolar Annelidt7a , the tulbes of the last being for the most part compose-d of Globigerine cemented together , frequenitly in a most regular and beautiful manlner .
The only living testaceous Mollusk that presented itself was a small specimen of Te elbraldla cr aniun .
Imbedded in the mud were found a specimnen of Kophobelemnnon Miulleri ( a type allied to Pennatula ) in full life , and two headless stems of Ruizocrinus , the perfectly fresh aspect of which leads me to believe that they must have growiv on the spot , and have been munutilated in .
the sifting of the mudl in which they were imbedded .
This mud contained a considerable proportioni ( about 60 per cent. ) of Glo6igerinio , together with some remarkably large Biloculince and other M31ilioline forms .
The general character of this Fauna obvionsly bore a close relationi to that of our previous dredging in a similar bottom ; and though we caninot positively affirm the Temperature of that bottom to be the same , yet we have not merely the evidenlce of a previous Sounding in a locality not far removed from it , but also that of a Sounding subsequently takenl in another locality further to the south , but nearly in the same longitude ( § 20 ) , to this effect .
20 .
Being anixious now to proceed as quickly as possible to the region in which we knew that we slhouled find much deeper water , we steered nearly due south , and on the morning of Sept. 17 reached lat. 590 49 ' and long .
12§ 36 ' .
Ilere a Souniiding gave us a depth of 620 fathoms [ I 134 mretres ] , with a bottom of white mud very similar to that of our last dredging .
The minimumn temperature , as showni by the meain of two there * See his description of Hyolnmerl boreale inI 'U fversigt af K. Veteiuslkaps Alademiens F6rbandlingar , ' 1808 , p. 105 ; translated inI 'Annals of Natural History , ' Fourth Series ( 1808 ) , vol. ii .
p. 8l.-Dr .
J. E. Gray , whilst still maintaining that tho " flint-rope " is a Zoophytic product , and that the Sponge with which it is connected is parasitic , has also com-le to the conelusionthat the brulsh-like terminiation serves as tho root implanted in imiud , above which the Spolnge is borneo .
( See Ann. of Not .
list .
, Fourth Series , vol. ii .
p. 272 .
) t See his Paper on the Vitreous Sponiges , in ' Annals of Natural History , ' Fourti Series , vol. i. ( 1868 ) , p. 114 .
mometers ( registering 45-k0 and 46-IO respectively ) , was 46 ?
[ 70.7 Cent. ] , the temperature of the surface being 52 ?
[ 110 1 Cent. ] .
21 .
Still proceeding southwards , we reached in lat. 58k0 the locality in which we hoped , from soundings previously made and recorded , to be able to extend our inquiries to greater depths ; but unfortunatelv a breeze had now set in from the N.E. , which was strong enough to prevent us not only from dredging but even from sounding ; and this breeze freshened on the night of Sept. 19 to a gale , which made it prudeint to seek the shelter of the land by running to the eastward .
Notwithstanding a partial abatement on the afternoonl of the next day , it was considered by Capt. May that , having due regard to the uncertain aspect of the weather , to the state of the barometer , and to the season of the year , as well as to the fact that the time assignied by the Admiralty for our remaining at sea was on the point of expiring , it would not be prudent to hold on as we were , for the slight chance of being able to accomplish our object .
Our course was therefore directed to Oban , which we reached on the afternoon of Sept. 21 * .
General -Results .
Before proceeding to sum up the general results of our inquiries , and to indicate the conclusions to which these seem to point , I think it desirable to give a brief notice of the researches of those who had preceded us in the same line of inquiry .
The earliest instance I have been able to find in which living Animals were brought up from great depths in the Ocean , occurred in the Arctic Expedition ( 1818 ) of Captain ( afterwards Sir John ) R:oss , and is mentioned in the narrative of his ' Voyage of Discovery ' t. General Sabine , who was a member of that Expedition , has been kind enough to furnish me with the following more ample particulars of this occurrence:- " The ship sounded in 1000 fathoms , mud , between one and two miles off shore ( lat. 730 37 ' N. , long .
750 25 ' W. ) ; a magnificent Asterias caput-medusce was entangled by the line and brought up with very little damage .
The mud was soft and greenish , and contained specimens of Lumbricus tu6icola .
' So far my written journal ; but I can add , from a very distinct recollection , that the heavy deep-sea weight had sunk , drawing the line with it , several feet into the very soft greenish mud , which still adhered to the line when brought to the surface of the water .
The Starfish had been entangled in the line so little above the mud , that fragments of its arms , which had been broken off in the ascent of the line , were picked ouit from amongst the muid .
" It hence seems indubitable that the Asterias ( Astrophyton ) and the Tubicolar Annelids were brought upfromz the bottom ; and the only doubt that can fairly be thrown upon the value of this observation has reference to the precise depth indicated by the Sounding , this having been made according to the old method now abandoned as unreliable .
The circumstances under which this sounding was taken , howeever , render it probable that the actual depth was not much less than that recorded .
In another Sounding , in calm water , and with a smooth sea ( lat. 720 23 ' N. , long .
730 7 ' W. ) , a depth of 1O05 fathoms was obtained with great precision ; and a small Starfish was found attached to the line below the point marking 800 fathoms .
The subsequent explorations of Prof. Edward Forbes* , on which he founded the opinion that a zero of animal life would be found at 300 fathoms [ 548 metres ] , did not themselves go deeper than 230 fathoms [ 420 metres ] ; vet his bigh authority on questions of this nature caused his opinion to be very generally adopted , alike by Zoologists , Physical Geographers , and Geolo0lists .
The fallacy of Prof. E. Forbes 's assumption , however , was demonstrated by the results of Dredgings carried on in Sir James Ross 's Antarctic Expedition , at depths of from 270 to 400 fathoms , which yielded evidence of great abundance and variety of Animal life between those depths .
Dr. J. 1D .
Hooker has kindly placed in my hands some extracts from his Journal , which give much fuller particulars of these results than are to be found in Sir James Ross 's Narrative t. On the 28th of Jurne , 1845 , the ill-fated Mr. Iharry Goodsir , who was a member of Sir John Franklin 's expedition , obtained in Davis 's Straits , from a depth of 300 fathoms , " a capital haul , -Mollusca , Crustacea , Asterida , Sptangi , Corallirtes , &c. " " The bottomn was composed of very fine green mud , apparently corresponding to that mentioned by General Sabine .
I am not aware that between this date and that at which the researches of MM .
Sars commenced , any Dredging was carried on at depths exceeding those now specified ; and the additions to our knowledge of the Life of the deep sea , with one remarkable exceptioni to be presently noticed ( p. 182 ) , were made through the instrumentality of the improved Sounding-apparatus , which brings up a specimen of the superficial deposit ( of whatever nature this may be ) covering the sea-bottom , with such Animals as it may meet " , 11 Report on the Miolluisca and Radiata of the Egean Sea , and on their distribution considered as bearing on Geology ; " in Report of the British Associationi , 1843 , p. 130 .
t 'Voyage of Discovery and Research in the Southern and Antarctic Regions , during the Years 1839-1843 , ' vol. i. p. 207 , and Appendix , p. 334.-It is much to be regretted that the specimenis obtained should never have been systematically catalogued , and that the many novelties which presented themselves ( among them a Pyonoogobid twelve inches across ) shouldr not have been described .
The specimens , with drawings made at the ime by Dr. Hooker , were kept by Sir Jamnes Ross , with a view to their publication ; but he died without carrying that intention inlto efect ; and neither specimens nor drawings are now recoverable .
t See the ' Natural History of the European Seas , ' by Prof. E Forbes and R. Godwin-Austen 1859 , p. 51 .
with on the spot on which it drops .
This method of examination must obviously be very inferior to Dredging in collecting-power ; nevertheless it has yielded some very important results .
In the year 1855 , Prof. Bailey ( of West Point , U.S. ) published a " Microscopic Examination of Deep Soundings from the Atlantic Ocean " * , between lat. 42§ 4 ' and 540 17 ' North , and long .
90 8 ' and 29 ?
0 ' West , and at depths of from 1080 to 2000 fathoms .
He stated that " none of these soundings contain a particle of gravel , sand , or other recognizable Mineral matter ; and that they are all made up of the shells of Globigerine and Orbulince , with a fine calcareous mud derived from the disintegration of those shells , containing a few siliceous skeletons of Polycystina and spicules of Sponges .
" Connecting these results with those furnished by previous Sounidings in the western portions of the Atlantic , Prof. Bailey inferred that with the exception of a spot near the bank of Newfouindland , in which the bottom at 175 fathoms was found to be made up of quartzose sand without any traces of organic forms , " the bottom of the North Atlantic Ocean , so far as examined , from the depth of about 60 fathoms to that of 2000 fathoms , is literally nothing but a mass of microscopic shells ; " and he explicitly likened this deposit to the Chalk of England and the Calcareoiis MaPls of the Upper Missouri .
After stating that examination of samples of ocean-water , taken at different depths in situations in close proximity to the places where the sounidings were made , yielded no trace of Foraminifera , he concludes with the following questions:- " Do they live on the bottom at the immense depths where they are found , or are they borne by submarine currents from their real habitat ?
Has the Gulf-stream any connexion , by means of its temperature or its current , with their distribution ?
" Upon these questions Prof. Bailey does not seem ever to have given a decided opinion ; although he inclined to the belief that the Globigerinaw and Orbulint ?
had not lived on the bottom where they were found , but had either been transported thither by currents , or had lived nearer the surface of the sea , and had fallen to the bottom after death .
On the other hand , Prof. Ehrenberg , to whom specimens of these Soundings were forwarded .
, expressed his conviction ( based on the condition of the organic substance contained in the cavities of the shells ) that these Foraminifera had lived on the bottom from which they were brought up .
Similar conclusions regarding the extensive diffusion of Globigerince over the deep-sea bottom of the North Atlantic were drawn by Prof. Huxley from his examination of the Soundings brought up by Lieut.-Commander Dayman , from depths of from 1700 to 2400 fathoms t. Of the whole mass of the fine mudldy sediment of which these soundings consisted , it is estimated by Prof. Huxley that 85 per cent. conisisted of Globigerine ; 5 per cent. of other Forarninifera , of , at most , not more than four or five species ; and the remaining 10 per cent. partly of Siliceous organisms ( D)iatom8 and Polycystina ) , partly of mineral fragments , and partly of the very minute granular bodies designated by Prof. HEuxley Coecoliths .
These granules he described as appareretly consisting of several concentric layers su-rrounding a minute clear cenitre , and looking at first sight somewhat like single cells of the plant Pr-otococcus ; but as thby are rapidlv and co-mpletely dissolved by dilute acids , their composition cannot be organic .
With referenice to the question whether the Giohigerince actually live at these depths , Prof. H-Iuxley says , " The balance of probabilities seems to me to incline in that direction .
And there is one circumstance which weighs strongly in my mind .
It may be taken as a law that any genus of animals which is found far back in time is capable of living under a great variety of circulmstances as regards light , temperatuire , and pressure .
Now the genius Globigerina is abundantly represented in the Cretaceous epoch , and perhaps earlier " ( op .
cit. p. 67 ) .
The results obtainied by Prof. Bailey and Prof. I-Iuxley , in regard to the prevalence of Glo6igerin6e over a la.rge part of the sea-bottom in the North Atlantic Ocean , were confirnmed and extended by the observations of Dr. Wallich , made during the voyage of the ' Bull-dog ' in 1860 ; and as he was able to examiine the condition of the Globigerince when freshly brought up , his testimony furnishes any important corroboration of Prof. Ebrei berg 's conclusion .
" The Globigerince , " he says * , " have never been detected free-floating in any number in deep , or forming deposits in shallow waters ; a considerable proportion of those met with in deep-sea deposits exhibit every appearance of vitality ; and their maximuim developmeylt is associated with the presence of the Gulf-stream , but only through the operation of collateral conditions prevailing at great depths below the current itself .
" But in addition , the ' Bull-dog ' sounding-line brouLght uip a cluster of Opphiocownce attached to a portion of it which had lain on the bottom at a depth of 1260 fathoms ; and Globigerince were found , with other matters , in their stomachs .
Further , in various localities , at depths ranging from 871 to 1913 fathoms , tubes of small Tubicolar Annelids were brought up ; and some of these were found to be composed of Globigerina-shells cemented together , whilst others were made up of aln admixture of Spongespicules and minute Calcareous debris .
Lastly a living Serpula , Spirorbis , and a group of Polyzoa were brought up from a depth of 680 fathoms , and a couple of living A 2phip)od Crustaceec from a depth of 445 fathoms .
Taking into consideration the arguments adduced to prove that the conditions which prevail on the deep-sea bed are not incompatible with the maintenance of animal life , and the extreme improbability that the creatures heretofore discovered at great depths are merely exceptional or accidental examples , it will , I think , be conceded that the presence of a living Fauna in the deeper abysses of the ocean has been filly established " t. Dr. Wallich 's just conielusions have not by any means commanded the universal assent of Naturalists .
It is still urged* that the Globigerinee lived at or near the suirface , and that they only fell to the bottom after death .
Anid it has been thouight by many to be more probable that the Ophioeomce had been entangled by the Sounding-line during either its descent or its ascent through the water , than that they had lived on the bottoml .
Our Dredge , however , having brought up , from depths of 530 and 650 fathoms , abundance of living Globigerine and Ophiocornce entangled in the recesses of Sponges , with Rotalice attached by shell-substance to the spicules of these Sponges , the statements of Dr. Wallich with regard to these animals , which I had always myself regarded as probable , may now be considered as put beyond reasonable question t. The general bearings of the facts thus brought to light , together with those furnished by the earlier observations of Sir John Ross and others , are fully and ably discuissed by Dr. Wallich ; but I must content myself with the following citation of his conclusions , referring to his Treatise for the arguments on which they rest : " Basinog my arguments , then , on two facts which I venture to hope are unequivocally proved in the preceding pages , namely that h-ighly organized creatures have been captured in a living condition at depths vastly exceeding those to which animal life had previouslv been supposed to extenid , and that their presence , when captured , cannot be regarded as an accidental or exceptional phenomenon , it has been my endeavour to establish the following important propositions : " I. The conditions prevailing at great depths , although differing materially from those which prevail near the suirface of the ocean , are not incompatible with the maintenance of animal life .
" II .
Assuming the doctrine of single specific cenitres to be correct , the occurrence of the same species in shallow water and at great depths proves that it must have undergone the transition from one set of conditions to the other with impunity .
" III .
There is nothing in the nature of the conditions prevailing at great depths to render it impossible that creatures originally , or through acclimatization , adapted to live under them should become capable of living in shallow water , provided the transition be sutfficiently gradual ; and hence it is possible that species now inihabiting shallow water may at some anterior period have been inhabitants of great depths .
" IV .
On the one hand the conditions prevailing near the surface of the ocean render it possible for organisms to subside after death to the greatest depths , provided every portion of their structure is freely pervious to fluid .
On the other hand , the conditions prevailing at great depths render it impossible for organisms still constituted to live under them to rise to the surface , or for the remains of these organisms after death to make their appearance in shallow water .
" 'V .
The discovery of even a single species living normally at great depths warrants the inference that the deep sea has its own special fauna , and that it has always had it in ages past ; and henice that many fossiliferous strata , heretofore regarded as having been deposited in comparatively shallow water , have been deposited at great depth " * .
In 1861 the very importanit fact was made public by M. Alphonse Milne-Edwards t , that when the Submarinie Telegraph-cable between Sardinia and Algiers was taken up for repair , several living Polyparies and Mollusks were attached to portionis of it which had been submerged to a depth of from 2000 to 2800 mictres , or from 1093 to 1577 fathoms .
Of these , some had been previously considered very rare , or had been altogether unknown ; whilst others were only known in a fossil state as belonging to the Fauna of the later Tertiaries of the Mediterraniean basin .
In the Swedish Expedition to Spitzbergen in 1861 , a compact mass of clay was brought up from 1400 fathoms by the " M'Clintock apparatuis , " the temperature of the interior of which was fonind to be 320.5 [ 00.3 Cent. ] , the temperature of the surface-water being 390.2 [ 40 Cenit ] .
" Notwithstanding this low degree of warmth , there were found several marine animals of different types and classes-amongst others a moderately large Polyparium , probably belonging to the Ilydroid class , a bivalved Mussel , some Tunicata attached to the Polyparium , and one Crustacean of bright colours " T. Of the very important researches which have been subsequently carried on by Prof. Sars of Christiania and his Son , we knew little more , whenl we proceeded on our own cruise , than is stated in Prof. Wyville Thomson 's letter ( Appendix ) .
But I have since learned from the recently published Report ?
, which Prof. Sars has been good enough to transmit to me , that their Dredgings have ranged between 200 and 450 fathoms , and that no fewer than 427 species have been collected within this range , which he classifies as follows : Protozoa .
{ Rhizopoda ... ... . .
68 Sponge .
5 Coelenterata ... ... Anthozoa ... ... ... ... 20 Hydrozoa .
2f Crinoidea ... ... ... ... . .
2 Echinodermata.* .
Echinida..5 Holothurida .
8 Vermes.f Gephyrea .
6 Annelida. .
51 rPolyzoa .
35 Tunicata .
4 Mollusca .
- .
Brachiopoda. .
41 Conchifera 37 tCephalophora 53 fArachnida.1 ... ... Arthropoda .
Crustacea.105 427 Of these , 20 species of Rhizopoda , 3 of Echinodermata , 8 of Conchifera , 3 of Cephalophora , and 4 of Crustacea-in all 42-are recorded as having been found at 450 fathoms .
Shortly after our return , I learned that an exploration of the deep sea by means of the Dredge had been very successfully commenced by Count Pourtales , in connexion with the United States Coast Survey ; and I have since received from Mr. Alexander Agassiz the following account of its results:- " He has dredged to 500 fathoms along quite a line of sections betweeni Florida and Cuba ; and under this pressure of nearly 100 atmospheres he has found Echini , Starftshes , Ophiuridans , Crinoids , Corals , many kinds of Crustacea,.4nnelids , Moliusca , Molluscoids , and , in fact , a Fauna as plentifully represented as along the most populous of our marine shore-fauna .
It has been decided to send Mr. Pourtales again this winter ; and with his former experience and additional equipment , we may look for grand results .
The facilities placed at his disposal are very great ; as his dredging-work is done in connexion with regular soundings carried on by the Survey of the Gulf-stream commnenced by Mr. Bache and prosecuted by his successor Prof. Pierce " .
Our own Dredgings , which have extended to a depth of 650 fathoms , are still the deepest of which I have any knowledge .
They were accomplished without any serious difficulty , and with results fully as satisfactory as those of ordinary shore-dredging .
And I have no doubt that similar dredges , worked by adequate enigine-power , would answer equally well at those far greater depths , our knowledge of the living inhabitants of which has beeni hitherto limited ( with the notable exception of the Mediterranean cable , p. 182 ) to the few forms that have beeni brought up by the Soundingapparatus* .
I , The collective results of these recent Dredgings have conclusively established the justice of the inference formerly drawni by Dr. Wallich from the more restricted data he had collected , as to the existenice of a varied and abundant submarine Fauna , at depths which have beeni generally supposed to be either altogether azoic , or occupied only by Animals of very low type .
And a complete disproof has thus been furniished of the doctrine , against which Dr. Wallich argued with great force , that a cert ; ain amouint of bathymetric pressu:-re must be prejuidicial , if not absolutely fatal , to highier forms of Animnal life .
In much that has been put forward upon this subject , two important considerations have been altogeth-er ignlored:-first , that pressure will not act upon an Animnal whose body entirely consists of solid and liquid parts , in the same mannaer as it acts nipon one that includes air-cavities ; and second , that as fluids press equally in all directions , an Animal i-milmersed at any depth is just as free to move one part upon another , as it would be if living near the surface .
The right point from which to look at this subject has long appeared to me to be the conClition of a drop of water , conceived as carried downi from the surface to a depth ( say ) of 1100 fathoms [ 2012 mzetres ] , at which the pressure will be about 200 atmospheres , or 3000 lbs. [ 1360 kilogr .
] upon the square inen .
Let it be coniceived that this drop is enclosed in a pellicle of the thinnest possible membrane , fitted only to separate it from the surrounding mnediumn , but having in itself no power of resistance .
Now it is obvious that this drop would maintain its form , whatever this may have originally been , entirely unchanged , being neither flattened-out into a planie , nor reduced to a sphere , by pressure to any amotunt which acts uponI it equally in all directions ; while its bhlk will only undergo r eduction , under a pressuire of 200 atmospheres , to the extent of less than one-hundredth .
Next , let us suppose , inistead of a drop of water conitained within a pellicle , a particle of the semiflutid " sarcode " of which the body of a 1 ?
/izopod is composed ; in which the more liquid interior ( endosarc ) is contained by a more tenacious external layer ( ectosarc ) , the contractility of which gives rise to continual changes of form , that are subservienit to the movement of the creature from place to place , and also to the ing- , estion of its food .
Now , it will be obvious to any one who follows out the law of flutid pressure in its application to any Animnal of this sirnple constitution , that so long as these changes of form do not involve a change of bellk , pressure to any amouint exerts no anitagonizing itnfluLence ; so that its movements can be performed with the same freedom on the ocean-bottom as they can be niear the surface .
And , further , even when the bulk of the body is augmented by the ingestion of solid or liquid particles ( say the reception of a zoospore of a Protophyte as food , or the filling of the " contractile vesicle " with water from without , which seems to be a sort of respiratory process ) , just as much pressure will be exerted by the superincumbent liquid in forcing those particles into the body as is exerted upon the exterior of the body in resisting its distension ; so that here , again , the influence of that pressure will be practically nil.-If the actions of any purely aquatic Animal of more complex structure be looked at from the same point of view , I am persuiaded that it will be fotund that they are not practically interfered with by fluid pressure to any amount , such pressure not having any tendency to alter either the general form of the body , or the shape of its softest and most delicate parts , and not interfering in the least either with the movements of these parts one upon the other , or with the circulation of fluid in their interior , or with those molecular chaniges which are concerned in their nutrition .
II .
The results we have obtained fully justify the consident expectation we had formed and expressed ( see Appendix ) , on the basis afforded by the observations of M. Alphonse Milne-Edwards on the Mediterranean Cable , and by the results of the dredgings of M. Sars , jun .
, that the systematic exploration of the Ocean-bottom , at depths much greater than are usually to be found near lauid , would bring to light many forms of Animal life , either altogether new to science , or hitherto supposed to be limited to particular localities , or known only as belonging to a Geological epoch supposed to have terminated .
For one and the same cast of the dredge , in the singularly productive locality specified in § 16 , brought up specimens of the highest interest belonging to each of these categories ; so that if we had been able , .
by remaining there even for a few days , to work this ground thoroughly , a much larger addition might have been fairly expected from this one spot , -stiLl more , therefore , if the inquiry should be extended over that much wider area in which , as will presently appear , the like conditions prevail .
For it must have been a strangely fortunate accident that brought together into ouLr drecdge so remarkable a collection of Vitreous S9ponges and gigantic Rhizopods ( many of them altogether new , and the rest known only as inhabitants of very distant localities , -with the Rhizocrinus previously obtained only in one spot more than 600 miles off ) , if these were not diffused tolerably abundantly as well as widely ; and the probability that they are so rises almost to a certainty , when it is borne in mind that the next dredgefull that was obtained from a bottom similar both in character and in temperature , though at a depth of 120 fathoms greater , and at a distance of 200 miles in a straight line , showed distinct evidence of the prevalence of similar types ( § 19 ) .
111 .
Our researches have conclusively established the existence of a minimum Temperature* at least as low as 3 20 [ 00 Cent. ] over a considerable area , where the depth was 500 fathoms [ 914 metres ] and upwards ; notwithstanding that the surface-temperature varied little from 52 ?
[ 110 1 Cent. ] , alike in this region and in neighbouring areas of similar depth , in , which the minimum temperature was only a few degrees beneath that of the surface .
The current doctrine in regard to deep-sea temperatures may be considered to be that expressed by Sir J. Herschel ( Physical Geography , 1861 , p. 45 ) in the following terms:- " In very deep water all over the globe a uniform temperature of 390 Fahr. [ 40 Cent. ] is found to prevail , while above the level , when that temperature is first reached , the ocean may be considered as divided into three great regions or zones-an equatorial and two polar .
In the former of these , warmer , in the latter colder , water is found at the surface .
The lines of demarcation are of course the two isotherms of 390 mean annual temperature .
" This doctrine , which is more fully and explicitly set forth by Dr. Wallich ( The North-Atlantic Sea-bed , ' 1862 , pp. 98 , 99 ) , rests , I believe , chiefly on the temperature-observations mad'e in Sir James Ross 's Antarctic Expedition , which were not inconsistent with the prevalent belief that sea-water , like fresh water , has its maximum density at this temperature , and that consequently water at 32 ?
or 330 cannot underlie water at 39 ? .
Several instances , however , had been previously recorded , in which temperatures below 390 had been observed .
Thus Lieut. S. P. Lee , of the United States Coast Survey , in August 1847 found 370 below the Gulf-stream , at the depth of 1000 fathoms [ 1809 mnetres ] , in lat. 350 26 ' N. and long .
730 12 ' W. ; and Lieut. Dayman found the temperature at 1000 fathoms [ 1829 metres ] in lat. 51 ?
N. and long .
40 ' W. to be 320 7 ' [ 00 4 Cent. ] , the surface-temperature being 540.5 [ 120.5 Cent.]* .
" At the very bottom of the Gulf-stream , " says Lieut. Maury ( Physical Geography of the Sea , 1860 , p. 58 ) , " when its surface-temperature was 80 ' [ 260.6 Cent. ] , the deep-sea thermometer of the Coast Survey has recorded a temperature as low as 350 [ 1.'6 Cent. ] .
These cold waters doubtless come down from the north to replace the warm waters sent through the Gulfstream to moderate the cold of Spitzbergen ; for within the Arctic Circle the temperature at corresponding depths off the shores of that island is said to be only one degree colder than in the Caribbean Sea , while on the shores of Labrador and in the Polar Sea the temperature of the water beneath the ice was invariably found by Lieut. De Haven at 280 [ -20.2 Cent. ] , or 40 below the melting-point of freshwater ice .
Capt. Scoresby relates that on the coast of Greenland , in latitude 720 , the temperature of the air was 42 ?
[ 50.5 Cent. ] , of the water 340 [ 01 ?
i Cent. ] , and 290 [ -1l06 Cent. ] at the depth of 118 fathoms " t. That there is no Physical improbability in the 100 atmospheres to which their bulbs were subjected , would prevent them from recording a minimnum as low as the aclual minimum ; and it seems to us not at all improbable that the actual minimurum may have been from 2 ?
to 4 ?
lower than the recorded minimum .
In any renlewal of the inquiry , it will be of course desirable that the Thermometric apparatus used should be specially protected from this source of error .
existence of a stratuim of sea-water at a temperature of 32 ?
or even 280 below a stratum at 390 , is evident from the fact ( whichhas been experimentally established beyond question t ) that Sea-water , in virtue of its salinie impregnation , contracts continuously down to its or dinar ?
y freezing-point , which is bellow 280 Falir .
And the existence of such strata , even in Equiatorial regions , has beea regarded by high scientific authorities t as proving the existeine of deep currents bringing cold water from Polar Regions to replace the warmer water that is continually flowing , as ( notably ) in the Gulf-stream , from the Equiatorial towards the Polar Regions , as well as to make good the immenSe losS which is constantly taking place by evaporation from th surface of Tropical seas .
To such an under-current , probably proceeding from the North or North-east , the low temperatures we Journial of Capt. Ross 's Voyage , which , if there was no error in the instrument employed , gives a lower temperature than any yet recorded : laving sounded , on Sept. 19 , 1818 , in 750 fathoml-s , the registeriu0Thermometer was senit down to 680 fathoms ; and on coming up , the index of greatest cold was at 250 75 .
Niever having known it lower than 280 in former instances ( even at a depth of 1000 fathoms , and at other times when close to the bottom .
) , I was very careful in exaamining the Thermiiometer ; but could discover no other reason for it than the actual coldness of the water .
" * It is stated by M. Despretz , as the result of a series of carefully conducted experiments , that the maxiiztmn density of Sea-water cooled down coniiitnuously without agitation is at -3 67 Cent. , or 250.4 Falir .
; the freezing-point of Sea-water which is a(ritated being -2 ?
55 Cent. , or 270.4 Fahr. See his 'H Recherches sir le Maximumr .
de Densite des Dissolutions Aqueuses , " in Assnales de Cliimie , 1.833 , tom .
lxx .
p. 54 .
t This doctrine , long sinice explicitly stateed by I-IHumboldt ( Cosmos , vol. i. p. 296 ) , is thuls set forth by Prof. Buff in his I Physics of the Earth ' ( p. 194):- " The water of the ocean at great depths lias a temperature , even unider the equtator , nearly approaching to the freezing-point .
Thiis low temperature cannot depend on aly influence of the sea-bottom ... The fact , however , is explained bly a continual cuirrent of cold water flowing from the Polar regions toNvar(ds the Eqtuator .
The following wellkniowin experiment clearly illustrates the manner of this movement .
A glass vessel is to be filled with water with which some powder has been mixed , and is then to be heated at bottom .
It will sooIn be seen , fromii the motion of the particles of powder , that currenlts are set up in opposite directions through the water .
Warmii water rises from the botton , up through the middle ol the vessel , and spreads over the surface , wlsile the colder and therefore heavier liquid falls down at the sides of tlse glass .
Currents like these mrust arise in all water-basins , and eveni int the oceans , if differenit parts of their surface are uniequally heated .
Tlhc water that is cooled in the polar regions sinks and travels frotmi the poles towards the equator , puislhing away the warimer and lighter liquid from the bottom of the sea ; itself to give way in turn , as it gets warm , to the colder water that follows after it .
This continual fw olf the water from the cold zones is replaced in a twofold manner .
The w^arsi water of the tropical seas , since it is the lightest , must spread itself north and soutlth over the surface of the ocean , and thus graduially losing its heat , be carried to the polar regions .
Between the tropics , too , evaporation goes on lllost vigorously , and( a great part of the Vap6UrS formaed fall again in raini and snow only in highler latitudes .
" A. iV set of deep sonudiuc s , takeni across the Arabiasa Sea , between Adeni and Bomlbay , by Capt. Shortland , in I-I.M.S .
' hydra , ' has lately )ee.n received by the IJydrograplier to tlse Admniralty , which give a line of bottom-temnperature of 331-0 [ 00.8 Cent. ] at depths observed between lat. 60§ 45 ' and 60§ 7 ' , as shown in the followin , Table and the accompanying Map ( for which I am indebted to the kindness of the H-vdrographer to the Admiralty ) , may be pretty certainly attributed .
TABLE OF PLACES , DEPTHS , AND TEMPERATURES OF SOUNDINGS .
Warmn rea .
No. LatituLde , N. LongiDepth , in Temperature tude , W. Fathoms .
at surface .
at bottom .
1 59 20 75 At least 500 545 490 2 60 32 0 10 104 54 485 3 60 31 9 18 229 54 48 4 60 44 8 45 72 54 49 5 61 17 48 02 53 50 12 59 36 7 20 530 52 5 47*3 13 59 57 29 189 52 49-3 14 59 59 9 15 050 53 40 15 60 38 11 7 570 52 47 16 61 2 12 4 ( 350 17 59 49 12 36 60 52 46 Gold A4rea .
No. Latitude , N. LonlgiDepth , in Temperature tude , W. Fathoms .
at surface .
at bottom .
6 60 4i5 4 49 510 52 33-7 7 60 75 21 500 51 32-2 8 60 10 5 59 550 53 32 9 60 24 6 38 170 52 41 7 10 60 28 6 55 500 51 33 11 60 30 7 16 At least 4,50 50 33-2 Of its northern limit we are not able to give any account ; but about 50 miles to the southward we found the temperature at the same depth to be 150 higher [ 8§ 3 Cent. ] ; and since the like temperature showed itself at even greater depths to the westward , between lat. 590 59 ' and 600 38 ' , and inferenitially ( § 19 ) as far north as 610 2 ' , at a distance of 175 miles from the most westerly point to which we traced this cold area , it may be presumed that this area was as limited in a westerly as we found it to be in a southerly direction .
HIere , therefore , within a short distance of the Northern Coast of Scotland , an opportunity is piresented for determining with great precision the physical conditions of two opposing currents , having a difference of temnperature of at least 150 .
In such determination it of 1800 fathoms and uipwards , the surface-temperature being 75 ? .
It seems impossible to account for this fact on any other hlypothesis than that of a deep currenit from the Antarctic Polar region , which must have maintainied this extremely low temuperature throughout the vast course it has had to tr'averse .
would be very desiratble to ascertain whether the minimum temperature is that of the botto , n ( a point of fundamental importance as regards the distributioni of Animal life ) , or whether it is that of some intermediate stratum .
The deep-sea Sounding-apparatus with which we were provided only allowed the attachment of the Thermometers to the extremity of the line ; and it is possible , of course , that their minimum may represent , not the temperature of the sea-bottom , but that of some higher stratum .
Independently , however , of the physical improbability ( for the reason already stated ) that Sea-water at 320 should overlie water of any higher temperature , which would be specifically lighter than itself , we have the evidence afforded by our Sounding in 170 fathoms ( § 13 ) within the cold area , that the temperature descends progressively with the depth ; at first ( as elsewhere observed ) more rapidly , afterwards more slowly .
And as this shallow bank is of very limited extent , and the bottom in its neighbourhood must become rapidly deeper , a careful examination of the bottom-temperature of its inclined sides at different depths would furnish satisfactory data on this point .
IV .
A general comparison of the Faunae of the different localities which we had the opportunity of examining seems to warrant the conclusion that the distribution of the Animal life of the seas beyond the Littoral zone* is more closely related to the temperature of the water than to its depth .
The predominance of North British types , not merely on the southern but on the northertn side of the deep valley which separates the Faroe Banks from the coast of Scotland , and in the warm areaof the valley itself , the slight admixture of exclusively Scandinavian or Boreal forms e-ven as far north as the Faroe Islands , the larger admixture of these on the shallow bank in the cold current , the still greater proportion of Boreal forms in the deeper and yet colder waters of that current , and ( in most striking contrast with this ) the presence of forms hitherto known only as inhabitants of the warmer temperate seas at the like depth in the war m area not many mniles off , -all indicate the intimacy of the relationship between Geographical distribution and Temperature .
The existence of Boreal types in the midst of an area whose surface-temperature is 52 ?
[ 1 P1 Cent. ] , and whose bottom-temperature , even at 500 fathoms ' [ 914 metres ] depth , is generally 470 or 48 ' [ 8 ?
` 3 or 80.8 Cent. ] , is obviously a phenomenon parallel to the occurrence of Alpinie plants at a high elevationl on -mountains within the tropics ; and as every Botanist would regard such occurrence as having no relation to elevationper se , but only to eleva* The distribution of marine Aniimal life in the Littoral zone is affected by a great number of conditionis , which place it in altogether a different category from that of the deeper seas .
I aim very glad to find outr views on this point in harmony with those of my friend Mr. J. Gwyn Jeftreys .
" The bathiymetrical zones have been too much divided by Risso and subsequent authors .
There are two pr-incipal zones , littoral and sumauerine ; the nature of the habitat and the supply of food influence the residence and migiration of ta .
, nimals , not the comparative depth of water."-Annals of Natural History , 4th ser. vol. ii .
( 1-868 ) p. 303 .
p tion as affecting Temnper ature , so it is obvious that , with the evidence we are enabled to present of an abundant and varied Fauna at a depth of even 650 fathomns [ 1189 muetres ] , the Zoologist is fully justifned in attributing the far different characteer of the Fauna we encounLtered at 500 fathoms [ 914 mnetres ] with a Temperature of 32 ?
[ 00 Cent. ] to that remarkable reduction .
Further , although the nature of the bottom has doubtless an important influence on the Animal life which it suistains , yet this very condition , as will presently appear , is itself dominated in great degree by Temperature .
V. The results of ouir D3redgings fully confirm the indications afforded by the specimens of the bottom previously brought up by the Soundings already noticed , in regard to the existence , on the sea-bottom of large areas of the North Atlantic , of a stratum of " calcareous mud , " partly composed of living Globigerince , partly of the disintegriated materials of the shells of form-er generationis , and partly of the " coccoliths ' of Prof. Huxley ( loc. cit. ) and the " coccospheres " of Dr. Wallich * , with a greater or less admixture of other constituents .
And they fuLrthier indicate that the prevalence of this deposit is connected with a bottom-temperature of 450 and upwards , which , in latitudes above 560 , can scarcely be attributed to any other influence than that of the Gulf-stream .
The examination which Prof. I-nuxley has been good enough to make of the peculiarly viscid muid brought up in our last dredging at the depth of 650 fathoms [ 1189 mi'tres ] , has afforded him a remarkable confirmation of the concluision he announiiced at the recenit Meeting of the British Association , that the coccoliths and coccosplhieres are imibedded in a living expanise of pirotoplasnic substance , to which they bear the same relation as the spicules of Sponges or of Radiolaria do to the soft parts of those alnimals .
Thus it would seem that the whole myass of this mud is penetrated by a living org-anism of a type even lower , because less definite , than that of Sponges and Rlizopods ; and to this organism Professor huxley has given the name of PBIathybius 1 .
In what manner the materials for its protoplasm , as for that of the Globigerinw which usually , accomnpany it itn larger or sm-naller proportion , are obtained , is a most perplexinproblem .
All the evidence we at present possess in re , ard to the alimentation of Rhizopods , leads to the belief that , in coilmmon with higolher Animals , they depend upon the Organiic Comnpoundcs previously elaborated by Vegetative agency ulnlder the influielnce of the light andi heat of the Sun .
But every form of Vegetable life that is visible to the n-aked eve seems entirely wanlting at great depths in the ocean : and although this deposit is found by the Microscope to contain the siliceous lori-ee of Diatoms , yet these do not present thiemselves in : anything like the abunrdance that would be reouired for the nutrition of so larme a mass of Animal life as that " Remarks on some niovel Phases of Organic Lift at great depth s in the Sea , " ill 'Ann .
of Not .
list .
' ser. 3 , vol. viii .
( 1861 ) p. 52 .
P " On somnfe Organisms ' living at Great Deptls in thLlle North Atlan-tic Ocea-L ; " in Quart , Journi .
of Microse .
Society , vol. viii ; .S .
p 203 .
represented by the GloNigerina-shells ; and there appears good reason to regard them as rather representing Diatom-s which have lived at or niear the surface , and have only subsided to the bottom after death , than organiisms which habitually live and grow in the ocean-depths .
It may be that the Bathybius ( which bears a very striking resemblanice to the iRhizopod-like rnycelitrn of the Myxogastric Fungi ) has so far the attributes of a Vegetable , that it is able to elaborate Or-ganic Compounds out of the materials supplied by the mediumni in which it lives , and thius to provide sustenance for the Animals imbeddedl in its muidst .
But to whichlever of these two Kingdoms we refer it , there seems adequiate reason for regarding this Bakthybius as onie of thie chief instruments whereby the solid material of the Calcareous mud which it perv , ades is separatedc from its solution in , the oceani-waters-@ In colnlnexion with this subject it may be suggested , as a suibject well worthy of experimental inquiry , to wwhat depth the Adetinic rays pen-etrate Sea-water in sufficient intenisity to produce an appreciable effect on a hiighly sensitive surface .
Certain it is that among the Ainimals broug , ht up from great depths , bright colours are not wanting .
This was noticed by Dr. Wallich in the case of the Ophiocoren brought up from 1260 fathoms .
And not only did the Astropecten , which came up on our dredige-linle from.500 fathoms , at once attract attention by its bright orange-red hue , but the small Annelid & which inhabited the Siliceous Sponge brouoht up from 650 fathoms were distian-uished1 by the vividness of their red or gre u colorationi .
VI .
Our researches have brought out with remarkable force the resemblance between this Calcareous deposit and the great Chalk-formation , which had been previously pointed out by Prof. Bailey , Prof. Huxley , and Dr. Wallich , but more particularlv by 1ir .
Sorby t , who identified the * Tle discovery of this indefinito plasmoclium , covering a wide area of the existing Sea-bottom , should afford a remiarkable confirmation , to sicch ( at least ) as still think confirnation necessary , ol the doctrine of the Organiie origin of the Serpentine-Limestono of the Laurentian Formation .
For if Bathlybiius , like the testaceous Rhizopods , could form for itself a sheolly elnvelope , that en-velope would closely resemable Diozoon .
Further , as Prof. Huxley has proved the existence of Beihybiies through a great range not merely of depth but of tenvpereture , I cannot buLt thinlk it probable that it has existed continuouLsly in the deep secs of elI Gcological Epochs .
And so far , therefore , from conisidering that the discovery of Eozoo2dl RPoc in the Liassic or evell in Tertiarry Strata , would ( as asserted by Profs .
Kinog:nd Rowney in a Paper recenitly presenited to the Geological Society ) be a conclesive disproof of its Organ-ie origin , I am fLilly prepared to believe thait Dozoo , as well as Bai'blecs , may have maintained its oxistenice th.rough the whole duration of Geological Time , from its first appearanee to the present Epoch ; and should be not in the least suprisped at bring , ing it up from 1000 or 2000 fathoms , if I should be enabled to dredge at thiose depths .
There must have been deep sects at all periods ; and the , coinsiderLcuions stated in Par. IX .
chow that the coaticlcity of Organic types is perfectly consistent with greet local chaniges .
Of such conitinutity there is niow ample evidence .
O " On the Organic Origin of the so-called Crystalloids of the Chalk , " in I Ann , of Not .
1-list .
' ser. 3 , vol. viii .
( 1861 ) p. 52 .
cc coccoliths " of Prof. Hluxlev and the " coccospheres " of Dr. 'Wallich with bodies observed in Chalk .
While the soundings , on the nature of which this conclusion was based , could Inot inidicate more thau the existence of a mere surface-layer of this material , the fact that our large dredges came up completely filled with it , and the maniier in which massive Siliceous Sponges had obviously been imbedded in it , clearly prove it to possess considerable thickness .
The existeniee of this deposit over a very large area was marked out by our Dredgings at the extreme distance of 200 mniles , and by several intermediate Soundings ; and the variations in its character corresponded closely with those which present themselves in different parts of the same stratum of Chalk .
VIT .
But besides confirming the views already pronmulgated , as to the complete dependence of this Calcareous deposit on the enormous development of low forms of Organic Life , our researches also show that the area over which this deposit is being formed is peopled by a variety of higher types of marine A-nimals , many of which carry us back in a most remarkable manner to the Cretaceous epoch .
Thus among Mollusca we have two Terebratulidee , of which one at least ( Tere6ratulina caput-ser entis ) may be certainly idenitified with a Cretaceous species , whilst the seconld ( 7aldheinia cranium ) may be fairly regarded as representing , if not lineally deseended from , another of the types of that family so abundant in the Chalk .
Among Echinoderms we have the little Rhizocrinus , that carries us back to the Apiocrinite tribe which flourished in the Oolitic period , and was intil lately supposed to have had its last representative in the Bourgetticrinus of the Chalk , to which the Rhizocrinus presents many points of remarkable correspondence e. Among Zoophytes , the OCQeliaza we met with in a living state seems generically allied to a Cretaceous type ( 0 .
explanata of Michelin ) .
Anid the remarkable abundanice of Sponges , which not improbably derive their nutriment from the protoplasmic substance that enters largely into the composition of the calcareous mud wherein they are imbedded ( p. 190 ) , is a preeminently conspicuous feature of resemblance.-We can scarcely doubit that a more systematic examination of the remarkable Formation at present in progress would place in a still stronger light the relationship of its Fauna to that of the Cretaceous period , since the specimens which our few dredgefuls contained can only be considered as a mere sample of the varied forms of Animial life which this part of the Ocean-bottom sustains .
And if ouir notion of the intimacy of ' this relationship should be confirmed by further inquiry , it would go far to prove , what seems on general groLunds highly probable , that the deposit of Globigerina-mud has beeni going on , over some part or other of the North-Atlantic sea-bed , from the Cretaceous epoch to the present time ( as there is niich reason to thinik that it did elsewhere in anterior Geological periodls ) , this mud beig , not merely a Chalk-formation , but a continuation of the Chalk* See the recently pujblished " Memoires pour servir a la coiinaissance des Crinoides vivants , ' by Prof. Sars ( Christiania , 1868 ) .
formation ; so that we may be said to be still livingg in the Cretaceous Epoch * VIII .
It can be scarcely riecessary to point out in detail those various important applications of the foregoing conclusions to Geological Science , whicn will at once occur to every Geologist who endeavours to interpret the past history of our globe by the light of the changes it is at present undergoing .
Bult this Report would not be complete without some notice of these .
In the first place , it may , I think , be conisidered as proved that no valid inference can be drawn from either the absence or the scantiness of Organic Remnains in any unmetamorphosed sedimentary rock , as to the depth at which it was deposited .
So far from the deepest waters being aZoic , it has been shown that they may be peculiarly rich in Animal life .
On the other hand , comparatively shallow waters may be almost azoic , if their temperature be low or their currents be strong ; and thus even littoral fornationis may show but few traces of the life that might be abundant on a deeper bottom at no great distance.-Again , it has been shown that two depqsits may be taking place within a few miles of each other , at the same depth and on the same geological horizon ( the area of one penetrating , so to speak , the area of the other ) , of which the Mineral character and the Fauna are alike different , -that difference being duie on the one hand to the direction of the current which has furniished their materials , and on the other to the temperature of the water brou(ght by that current .
If our " 'cold area " were to be raised above the surface , so that the deposit at present in progress upon its bottom should become the subject of exanmination by some Geologist of the futuire , he would find this to consist of a barren Sandstone , including fragments of older rocks , the scanty Fauna of which would in great degree bear a Boreal character ( ?
H. ) ; whilst if a portion of our " warm area " were elevated at the same time with the " ' cold area , " the Geologist would be perplexed by the stratigraphical continuity of a Cretaceous formation , including not only anl extraordinary abundalnce of Sponges ) but a great variety of other Animal remains , several of them belonging to the warmer Temperate region , with the barren Sandstone whose scanty Faunia indicates a widely different climatic condition , which he would naturally suppose to have prev ailed at a different period .
And yet these two conditions have been shiown to exist simultaneously , at corresponding depths , over wide contigvtons areas of the sea-bottom X in virtue solely of the fact that one area is traversed by anl Equatorial and the other by a Polar current t. Further , in the midst of the land formed by the elevation of the " cold area , " ori Geologist would find a hill somrne 1800 feet high , covered with a Sandstone continuous with that ol the land from -hich it rises , but rich in remains of Animals belonging , to a more temperate province ( § 13 ) and might easily fall into the mistake of supposing that two such differenit Fauna , occurring at differenit levels , must incdicate two distinct climlates separated in time , inistead of indicating , as they have beenl shown to do , two contemporanieous but dissimrilar climates , separated only by a few miles horizontally , and by 300 fathoms verticnlly.-It seems , searcely possible to exa-gerate the inportance of thaese facts , in their Geological and Palseontological relations , especially in regard to those more localized Formation 's which are especially characteristic of the later Geological epochs .
But eveni in regard to those older Boucks , N ; hose wicle rang , e in space and time would seem to indicate a general prevalence of similar coniditions , it may be suggested whether a diicrecilee of bottomn-temiperature , depending upon deep oceanic currenits , was not the chief determining cause of that remarkable contrast betweern the Faumn.e of dinf-erent areas in .
the same Formation , which is inldicated by the abundlance and variety of the Fossils of oue locality , and their scantin:ess and limitation of type in another ; as is seen , for exAample , wleln the " Primordial Zone " of Barrande is compared with its equivalent in North Wales.-Further , in the case of those Calcareous deposits which o we their very existence to the vast development of Organisms that possessed the power of separatinog Ca-rbonatUe of Lime from the ocean-waters , temnperature may be pretty certainly assumed to be the chief conlition , not merely of the character of the Animal remains which those formations may ihclude , but of the very production of their solid material .
IX .
Ilow important a light is thrown by the facts we have brought into view on those changes in .
the Marinie Fauna of any particular area , which cannot be referred to changes in its own geological condition , i neecl scarcely be pointed out .
As there must have been deep seas in all Geological epochs , so there must have been varieties in S'u6nrihne Climante at least as great as tbose we have discovered , depending upon those Equatorial and Polar Currents whose existence Las been shmown to be a Physical necessity .
Hence it is obvious that sinie change s in the direction of slch opposing currents must have been producedl by any upward or downward movement of the sea-bottom ( as , in the areas of clevation and subsidence marked out by Mr. Darwin in our existing seas ) a considerable inodification , or eveni a complete reversal , of the Subrrmaririe Climates of adjacent aireas miglt have beein conseqluent upon alterations in the cointour of the lanid , or in the level of the sea-bottomn at a gry-eat distance .
The effect of such a modification of Temperature upon the respective Paunim of these areas would probably depend upon the rate and degree of the cliange .
If neessary coiise'uience of the difference of surface-tcsnperaturc between Equatorial anicl Polar waters ; and those who raise the objection aro consequently bound to orier some other conceivable bypothesis oln w , , , hich the facts above stated can be accoulnited for .
rapid and considerable , it might cause the extinction over those areas of a large proportion of the species which inhabited them ; whilst others would mnigrate in the direction of the temperature most congenial to them , and transfer to new localities those types which could no longer exist ill their previous habitats , -thus establishing the Colonies of M. Barrande .
If , on the other hand , such a change of Temperature were more gradual , the greater part of the species constituting the Faunie of the areas over which it occurred might adapt thenmselves to it , undergoing such modifications in their structure and habits as might be considered sufficient to differentiate them specifically , whilst retaining so maniy characters of general similarity as to constitute " representative species " @ .
X. The ingenious suggestion of Dr. Wallicht that the nature of the Animal life found on the sea-bottom may not unifrequently afford some clue to the history of its changes of level , -his discovery at great depths of a type ( the Ophioeowa gr agntlata ) which is essentially littoral being indicative of slow progressive subsidence , -may be extenided with some probability to changes of submarine climate ; for where any species is found abulndaantlly as a littoral form , its presence at great depths in the same region wotild seem to inidicate that the suibsidence of the bottom has not been attended with any considerable alteration of tetmperature , whilst its absence on nieighboulring parts of the same area may be fairly taken as evidelnce of such a chan , e. The preparation of a detailed list of , the Species found in each locality , with the depths from wzvhich they were broug , ht up , furnishing the justification of the geiieral statenients imade in this Report , has been kiildly unidertaken by Professor Wyville Thomsoni , who will present it at the earliest practicable dlate ; and he will also describe the new and very remarkable forms of Vitr eous Sponges we have obtainied , this being a group to which he has already given special attention.-I .
shall myself lose no time in , preparing anaccount of the Piizopods we have collected , availing myself of the kinld assistance of Professor I-Huxley , who has undertaken to examine and describe the Organic components of our various specimenis of Chalk-mud , and of Professor Frankland , who will deterimine their Chemical comiposition .
Wecannot but hope that when ourReport shall have been thus completed , it may be found not unlworthy of the Royal Society by which our inquiry was promoted in the first instance , and of the Government which provided the meanls for its prosecution , and that the results we have obtained may be reg , arded as sufficienitly important to justify its extension bot ; h in range * It will be obvious to every one who is conversant with Sir Charles Lyell 's ' Principles , ' that in the views above staLted I have sim)ply extleded the doctrines long since promulgated by that great Mlaster of the Philosophy of GO-cology .
t The North-Atlantic oea-Bed , pp. I19-155 .
and objects .
For we cannot but believe that Pllysicists , Physical Geographers , Naturalists , and Geologists will alike desire such a careful and detailed exploration of the Sea-bottom between the North of Scotland and the Faroe Islands ; as may determinie with precision , -(I ) the depth in every part of that area ; ( 2 ) the temn perature , not merely of every part of the bottom , but also at variotus depths of the water that lies upon it , say , at every 50 fathoms vertically ; ( 3 ) the precise boundaries of the cold area of bottom-temperature which separates the northern and southerni portions of the warm area ; ( 4 ) the direction and rate of any current that may be detected in either or each of these areas ; ( 5 ) the relative composition of the water in these areas respectively ; ( 6 ) the relative proportions of gases contained in the sea-water at different depths , and in the same depth at different temperatures ; ( 7 ) the penetrating power ?
of the Actinic rays in their passage through Sea-water ; ( 8 ) the nature , composition , and sources of the deposits in progress over the several parts of the sea-bottom , especially distinguishing those of its warm and those of its cold tracts , as well as those along the line or band of demarcation between the two ; and ( 8 ) the distribution of Animal and Vegetable Life throughout the whole region , as complete a collection as possible being made by repeated dredgings in every part of it , so as to furnish materials for valid inferences as to the relations of its several forms to the depth , temperature , and character of the sea-bottom on which they respectively occur .
The near proximity of this area to our own shores , and the consequent facility with which a vessel may be kept at sea during the whole of the season most suitable for work of this kind , by runining for supplies to Stornoway , Lerwick , or Kirkwall ( as may be most convenient ) , renclers it peculiarly fitting for such an investigation ; for just as the limited area of the British Islands presenits an epitonme of the whole Geological series , so does this limited Oceanic area presenit such varieties of depth and temperature , and probably of currents , as are only likely to be met with elsewhere at a far greater distance from land , and over a much wider Geographical range.-But it is also greatly to be desirect that these inquiries should be prosecuted at still greater depths ; and such may be reached with no less facility by proceeding westwards from the West of Scotland or the North-west of Ireland , a depth of at least 1300 fathoms being known to exist between these C(oasts and Rockall Batnks .
It only remains for me to tender the grateful acknowledgments of Professor Wyville Thomson and myself to Her Majesty 's Governiment for the readiness with which they acceded to the recommendation of the Presidenit and Council of the Royal Society , and for the liberality with which the means of prosecutingo , ou-r inquivies were furnished by the Admiralty ; and we would in particular express our obligations to the Hydrographer to the Admiralty for the earnestness with which he took up the idea of this Expedition in the first inistaniee , the perseveranice with which he subsequently carried through every arrangement that could promote its scientific efficiency , and the colnsiderate kindness with which he provided all that was needfiul for our welfare and comfort .
Our cordial thaniks are also due to Staff-Commander May for the heartiness with which he threw himself into the work , and the thoughtful considerationi he uniformly showed , alike for the objects of the Expedition and for our personal convenience ; and to Sub-Navigating-Lieutenant Tooker , by whom Captain May 's exertions in both these respects were zealously and efficiently seconded .
We would also record our sense of the friendly reception which we met with on the part of Ilis Excellency the Governor of ' the Faroe Islauds , who , althouogh we were not in any way accredited to him , did his utmost not only to promote the Scientific objects of our visit , but also ( with the aid of his accomplished Ladv ) to render our stay at Thorshaven agreeable to us .
APPENDIX .
From the Minutes of the Council of tke Royal y Society , Jftne 18 , 1868 .
FPromit Dr ) .
Carpenter , V.P.R.S. , to the Pr-esidezt of the Royal Society .
University of London , Burlington House , W. June 18th , 1868 .
DE3AR GE]3NTERAL SABINE , -During a recent visit to Belfast , I had the opportunity of examining some of the specimens ( transmitted by Prof. Sars of Christiania to Prof. Wyville Thomson ) which have been obtained by 1 .
Sars , jun .
, Inspector of Fisheries to the Swedish Governlment , by deep-sea dredgings off the coast of Norway .
These specimens , for reasons stated in the enclosed letter from Prof. Wyville Thomson , are of singular interest alike to the Zoologist and to the PalTontologist ; and the discovery of them can scarcely fail to excite , both among Naturalists and among Geologists , a very strong desire that the zoology of the deep sea , especially in the Northern Atlantic region , sholuld be more thoroughly and systematically explored than it has ever yet beenl .
From what I ktnow of your own early labours in this field , I cannot entertain a doubt of your fuLll concurrence in this desire .
Such an exploration cannot be undertaken by private individuals , even when aided by grants from Scientiric Societies .
For dredging at great depths , a vessel of considerable size is requisite , with a trained crew , such as is only to be found in the Government service .
It was by the aid of such an equipment , furnished by the Swedish Government , that the researches of M. Sars were carried on .
Now as there are understood to be at the present time an unusual nuiLmber of gun-boats and other cruisers on our northern and western coasts , which will probably remain on their stations until the end of the season , it has occurred to Prof. Wyville Tlhomson and ml-yself , that the Admiralty , if moved thereto by the Countcil of thb Royal Society , might be iniduiced to place one of these vessels at the disposal of ourselves and of any other Naturalists who might be willing to accomipany us , for the purpose of carrying on a systematic course of deep-sea dredging for a mnonth or^ six weeks of the present summier , commnencin , early in August .
, Though we desire that this inquLiry should be extended both in geographical range and in depth as far as is proposed in Prof. Wvyville Thon1iso 's letter , we think it preferable to limit ourselves on the present occasion to a request which will not , we believe , inlvolve the extra expense of sending out a coaling-vessel .
We should propose to imake Kirkwall or Lerwick otur port of departure , to explore the sea-bottom between the Sh-etland and the Faroe Islands , dredging aroLnd the shores and in the fiords of the latter ( which have not yet , we believe beenl scienitifically exax ' ined ) , and then to proceed as far north-west into the deep water between the Faroe Islands and Icelanid as may be founid practicable .
It would be desirable that the vessel prov7ided for such a service should be onie capable of umaking way under canlvas , as well as by steam-power ; but as our operationis must necessarily be slow , speed would not be rlecuired .
Considlerable labour would be spared to the crew if the vessel be provided with a " donkeyeng , in " that could be used for pulling up the dredoe .
If the Council of the Royal Society should deem it expedienit to prefer this requLest to the Admiralty , I trust that they may further be willing to place at the disposal of Prof. WAyville T1hom11 , son11 and myself , either from the Douation Fund or the Government-Granllt Funld , a suns of ?
100 for the expenises wAe0 must incur in providing an amiiple supply of spirit and of jars for the preservation of specimens , witn other scientific appliances .
Ve would undertake that the choicest of suLch specimens shotuld be deposited in the British Museum .
I shall be obliged by your bringing this subject before the Council of the Royal Society , and remaini , Dear General Sabine , you1rs faithfully , The Ptresldenlt of the Royal Society .
WILLIAM 13 .
CAi .
PriNTER .
Fro ?
n Prof. TVyville T1tooisonl Belfast , to Dr. Opcnter , T.P.B.S. May 30 , 1868 .
MvY PEA & R C2VR .
PnNrnu,2-WClVeui I last saw you , I suggesteed how very importeant it would be to the advancement of science to determilne with accuracy the conditions and distribLution of Animial Life at great depths in the ocean ; I iow resuume the facts and consideratfions which lead me to believe that rescareises iss this direction promise valuable results .
All recent observations telnd to negative Edward Forbes 's opinion that a , ero of animal life was to be reachled at a depth of a few hundred fiathoms .
Tw\vo years ago , Al .
Sars , Swedish Goverume'n Tns -eto'r of Fisheries had an oppostulnity isl his official capacity of dredgino ofi the toffoden Islahids at a depth of 300 fathosuis .
I visited Norway shortly after his retusrn , a"nd ha ' an opportuniity ' of studyinog with his father , Prof. Sas , r some Oc hiiresLlts Aniisal foriss were abandant ; many of them wet newx to science ; and anmong them was onie of surpassing interest , the snmall Criinoid of welish 0ou0 nave a specimnen , and which we at onice recoonized as a degraded type of the A1piodrhidac , na order lli-therto egca.rdedas extinc7t which attained its naxiusam in the Pear-escerinites of the Jurassic Period , and whose latest represesitative Ihitherto knowsi was the Boo1guctticrfnus of the Clialk .
Somue years previously , M. Absjorusen , dredging in 200 fathomns in the Tlardelnger:rjoid , procured several exalispLes of a Stasfiis ( Brisinga ) wNvhich seems to fisid its nearest ally isi the fossil genus Protester .
These observe , ations place itbeyonid a doubt that assisual life is abundtant in the ocean at depths varying from 200 to 300 fathoms , that the forms at these great depths differ greatly from those met with in ordinary dredg , ings , and that , at all events in some cases , these animals are closely allied to , and wouLld seem to be directly descended from , the fauna of the early Tertiaries .
I think the latter result might alimost have been anticipated ; an probably further investigation will add largely to this class of data , and will give us an opportunity of testin(g ouLr determination of the zoological position of some fossil types by an examination of the soft parts of their recent representatives .
The meain cause of the destruction , the migration , and the extreme modification of Animal types , appears to be change of climate , chiefly depending upon oscillations of the earth 's crust .
These oscillations do not appear to have ranged , in the northern portion of the Northern Hemisphere , much beyond 1000 feet since the commencement of the Tertiary epoch .
The temperature of deep water seems to be constant for all latitudes at 390 ; so that an immnense area of the North Atlanitic iu-st have had its coinditions unaffected by Tertiary or Post-tertiary oscillations .
One or two other quLestions of the highest scienltific interest are to be solved by the proposed investioations : Ist .
The effect of pressure upon Animal life at great depths .
There is great mnisapprehension oln this point .
Probably a perfectly equal pressure to anzy amo-unt would have little or no effect .
Air being highly compressible , and water compressible only to a very slight degree , it is probable that under a pressure of 200 atmospheres , w"ater may be even more a6rated , and in that respect more capable of supporting life , than at the surface .
2nd .
The e-ffect of the great diminution of the stimulus of Light .
From the condition of the Cave Faunia , this latter agent probably affects only the development of colour and of the organs of sight .
I have little doubt that it is quite practicable , with a small heavy drecdge , and a couple of miles of stouIt -Manilla rope , to dredge at a depth of 1000 fathoms .
Such , an undertakino would , however , owingo to the distance , and the labour involved , be quite beyoned the reach of private enterprise .
What I am therefore anxious for is , that the Admiralty may be induceld , perhaps at the instance of the Council of the Royal Society , to send a vessel ( such as one of those which accompanied the Cable EExpedition to take soundings ) to carry out the researclL .
I sho-uLld be ready to go any time after July ; and if you Lwould take part in the investigation , I cannot but believe that it would give good results .
I woould propose to start from Aberdeen , and to go first to the Rockall fishing-bankls , where the depth is moderate , and thence north-westward , towards the coast of Greenland , rather to the north of Ca pe Farewell .
We should thus keep pretty nearly alongw the isotherm of 390 , shortly reaching 1000 fathoms depth , where , allowing 1000 feet for oscillations in level , and 1000 feet for influence of surface-currents , smumrner h-eat , &c. , we should still have 4000 feet of wate-r whose colnditions have probably not varied greatly since the commilelncement of the Eocene epochl .
Your most truly , WYVIILLE Tsro-rseN .
These letters having been considered , it was Resolved , -That the proposal of Drs. Carpeniter and W\yville Thomisona be approved , and recommended to the favourable consideration of the authorities of the Admiiralty ; and that a sum , of not exceeding ?
100 , be advanceed from the Donation Fund to meet the expenses referred to in Dr. Carpenter 's letter .
The following draft of a letter to be written by the Secretary to the Secretary of the Admiralty was approved : MY LoRD , Iam directed to acquiaint youi , for the information of the Lords Commissioners of the Adlmiralty , that the President and Council of the Royal Society have had under their consideration a proposal by Dr. Carpenter , VicePresident of the Royal Society , and Dr. Wyville Tholllson , Professor of Natural IHistory in Queen 's College , Belfast , for conducting dredging operations at greater depths than have heretofore been atteml'pted in the localities wNvhich they desire to explore the miiain purpose of such researchles being to obtain inforlmlation as to the existence , miode of life , and zoological relations of marine animials living at great depths , with a view to the soluition of variotus questions relatin to animal life , and having an important bearing ; on Geology and PaLeontology .
The objects of the operations which they wislh to undertake , and the course which they would propose to follow , as well as the aid they desire to obtain fiem the Admiralty , are lmlore ftully set forth in the letter of Dr. Carpenter to the President , and that of Professor Thomson , copies of which I herewith enclose .
The President and Council are of opinion that important advantages may be expected to accrue to science from the proposed undertaking ; accordingly they strongly recommend it to the favourable consideration of I-Ter Majesty 's Government , and earniestly hope that the Lords Commissioners of the Admiiiralty may be disposed to grant the aid requested .
In such case the scientific appliances required would be provided for from fnlds at the disposal of the Royal Society .
Iam , &c. , W. SHIARPEY , Sec. R.S. Lord H. Lennox , MAP .
, Secretary of the Achnirialty .
Fromn the Minutes of the Council of the Royal Society for October 20 , 1868 .
Admiralty , 14th July , 1868 .
SIn1 In leply to your letter of the 22nd ultimo , submitting a proposition from Dr. Carpenter and Professor Thomson to investigate , by means of dredging , the bottom of the sea in certain localities , with a view to ascertain the existence and zoological relationis of marine animals at great depths , -a research which you and the Coulncil of the Royal Society strongly recommend in the interests of science to the favourable consideration of 17e1r Majesty 's Government , for aid in furtherance of the undertaking , -I am commanded by My Lords Coimmissioners of the Admiralty to acquaint you that they are pleased to meet your wishes so far as the Service will admit , and have given orders for ITher M < ajesty 's steam-vessel ' Lightning ' to be prepared immediately , at Pembrolke , for the purpose of carrying out such dredg , ing operations .
I am , Sir , Youir obedient Servant , WV .
G. ROirAINE .
To the iPresident of the ioyel Society .
The Society then a(djourined over the Christmas PRecess to 'T'hursday , January 7 , 1869 .
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