Relaxation oscillations in the source of S-bursts of Jovian decametric radio emission

Details Relaxation oscillations in the source of S-bursts of Jovian decametric radio emission Relaxation oscillations in the source of S-bursts of Jovian decametric radio emission

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..644s&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, July 1988, p. 644-650. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

3

Decametric Waves, Jupiter (Planet), Planetary Ionospheres, Planetary Radiation, Radio Bursts, Radio Emission, Cyclotron Resonance, Flux (Rate), Plasma Waves, Wave Excitation

Scientific paper

A mechanism is proposed by which long-period (tens of milliseconds) trains of S-bursts of Jovian decametric radio emission are produced. Those trains of S-bursts are caused by pulsed diffusion in momentum space of fast electrons. The diffusion is due to plasma waves generated by fast electrons under the cyclotron reasonance conditions. Conditions for appearance of a periodic regime are specified. Dependence of the period on the electron flux in the source is found. It is shown that a periodic regime with periods consistent with the observations is possible in the Jovian ionosphere environment.

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