Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991azh....68..853b&link_type=abstract
Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 68, July-Aug. 1991, p. 853-862. In Russian.
Astronomy and Astrophysics
Astronomy
Decametric Waves, Jupiter (Planet), Planetary Radiation, Plasma Waves, Radio Emission, Cerenkov Radiation, Electron Beams, Io, Wave Generation
Scientific paper
A novel mechanism is proposed for the generation of Jovian decametric S-emission based on the Cerenkov instability of an electron beam that is capable of arising inside the Io-Jupiter flux tube. It is shown that the proposed mechanism explains fairly well such experimental findings as the cone-like radiation pattern, the anomalous angle-frequency dependence, and the dynamic drift of S-bursts over a wide frequency range. Estimates made for Jupiter's intrinsic parameters demonstrate that the mechanism is able to provide the observed values of emission energy fluxes.
Boev A. G.
Lukyanov M. Y.
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