Beaming structures of Jupiter's decametric common S bursts observed from LWA1, NDA, and URAN2 radio telescopes
On 2015 February 21, simultaneous observations of Jupiter's decametric radio emission between 10 and 33 MHz were carried out using three powerful low frequency radio telescopes: Long Wavelength Array Station One (LWA1) in USA; Nan\c{c}ay Decameter Array (NDA) in France; and URAN2 telescope in Ukraine. We measure lag times of short bursts (S bursts) for 105 minutes of data over effective baselines up to 8460 km by using cross correlation analysis of the spectrograms from each instrument. Of particular interest is the measurement of the beaming thickness of S bursts, testing if either flashlight or beacon like beaming is emanating from Jupiter. We find that the lag times for all pairs drift slightly as time elapses, in agreement with expectations from the flashlight like beaming model. This leads to a new constraint of the minimum beaming thickness of 2.66" Also, we find that most of the analyzed data abound with S bursts, whose occurrence probability peaks at 17 18 MHz.