Physical Sciences: Fine Structure of the Jupiter Radio Bursts

Details Physical Sciences: Fine Structure of the Jupiter Radio Bursts Physical Sciences: Fine Structure of the Jupiter Radio Bursts

Feb 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973natur.241..387e&link_type=abstract

Nature, Volume 241, Issue 5389, pp. 387-389 (1973).

Physics

9

Scientific paper

SHORT pulses with a time scale of milliseconds and fractions of a millisecond have been observed in the radio emissions of Jupiter at wave frequencies near 20 MHz since 1956 (refs. 1 and 2). Little is known about these ``S'' bursts, however, although it has been established3 that their occurrence depends strongly on the orbital position of the satellite Io. Further, Gordon and Warwick4 were able to show from a small set of observations that the bursts may have a relatively narrow radio frequency bandwith (<50 kHz) and that their centre frequency may change rapidly with time at the rate 25-35 MHz s-1, at least near 26 MHz.

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