Analyses Of Jovian Decametric Radiation S-Bursts Interacting With N-Bursts

Details Analyses Of Jovian Decametric Radiation S-Bursts Interacting With N-Bursts Analyses Of Jovian Decametric Radiation S-Bursts Interacting With N-Bursts

Aug 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002em%26p...88..187o&link_type=abstract

Earth, Moon, and Planets, v. 88, Issue 4, p. 187-209 (2000).

Physics

Dam, Jupiter, N-Burst, S-Burst, Tilted-V

Scientific paper

Dynamic spectra of S-bursts of Jovian decametric radiations are obtained by using a high time resolution radio spectrograph which has a time resolutionof 2 msec and the bandwidth of 2 MHz.Within occurrence of 65 S-burst events observed in the period from 1983 to 1999, 26 events have been identified as the S-N burst events, which are characterized by the interaction between the S-burst emissions and the Narrow band emissions. In the dynamic spectra of the S-N burst, the trend of emissions with negative and slower frequency drift named as “Trailing Edge Emission” are often observed shortly after the appearance of the S-burst.Detailed analyses of these phenomena revealed that the Trailing Edge Emission is not a manifestation of S-burst with slower drift rate but a variation ofN-burst. The results suggested that S-burst and the associated Trailing Edge Emission are formed simultaneously started from a common region with different drift rates. It has been further suggested that the appearance of the S-burstsis not controlled by the geometrical effect between the source region and theobserver, but directly reflects the generation of the source region widelydistributed in an altitude range from a few thousands km to 30,000 km, alongthe Io flux tube.

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