Studying travelling ionospheric disturbances from near-vertical ionosphere sounding with high temporal resolution
In this study, we analyze the near-vertical ionospheric sounding data obtained with a multipurpose digital chirp ionosonde. The ionosonde was recording ionograms once each minute. We analyzed the results of processing the datasets over three observational years from 2010 to 2012. Obtaining ionograms with a high temporal resolution allowed us to trace the dynamics and evolution of additional traces referred to as “cusps”, and also to combine ionograms with such traces into sequences. The percentage of ionograms containing cusps proved to be more than 10% of the overall number of ionograms. Thus, during daytime, the rate surpasses 30%, whereas, during nighttime, such ionograms are practically absent. The typical cusp lifetime proved to be 4-15 min, therefore, disturbed ionograms are much more rarely detected with standard vertical sounding ionosondes. The presence of such traces unambiguously evidences significant electron density horizontal gradients caused by travelling ionospheric disturbances (TIDs) with scales up to 50 km.
The effects of travelling ionospheric disturbances on ionograms
Abstract The numerical synthesis of ionograms by ray-tracing in an analytic two-dimensional ionosphere is simplified by a technique which avoids the usual wastage of ray tracings. The technique is particularly suitable for obtaining ionogram sequences corresponding to a moving ionospheric disturbance. It is applied firstly to a moving tilted ionisation increase, which gives the familiar travelling-cusp records. Ionograms do not give a good measure of the vertical distribution of ionisation, and in the case considered lead to an overestimate of the horizontal size of the increase by a factor of about 2. For a travelling ionisation decrease or trough, the ionograms show an additional U-shaped trace overlapping the main trace. Calculated ionograms agree closely with some observations. It is difficult to obtain any measure of the size of the electron-density decrease; critical frequency scalings may give no indication of the passage of an intense disturbance. Similar results are obtained for a wavelike perturbation in an exponential topside ionosphere. Topside ionograms then show multiple ‘nose’ traces, following in general the curve for the unperturbed ionosphere. It is suggested that the multiple echoes frequently observed on topside ionograms may, in some cases, be due to refraction in large disturbances rather than the commonly-assumed ducting mechanism.
An ionospheric ray tracing technique
The method of Jones used for the ray tracing of internal gravity waves has been applied to radio waves in the ionosphere. This method avoids problems usually encountered near a reflection point and, consequently, may be used to trace both reflected and refracted rays. The method is particularly efficient when the propagation effects of the magnetic field are neglected.