Three excitation bands of whistlers in Jupiter's radiation belts

Details Three excitation bands of whistlers in Jupiter's radiation belts Three excitation bands of whistlers in Jupiter's radiation belts

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13.1094b&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, Dec. 1987, p. 1094-1099. In Russian. In Russian.

Other

Cyclotron Resonance, Jupiter Atmosphere, Radiation Belts, Wave Excitation, Whistlers, Electron Distribution, Gyrofrequency, Relativistic Velocity, Spectral Bands

Scientific paper

Instability of Jupiter's radiation belts to the excitation of whistler waves at cyclotron resonance is studied. It is shown that for the experimentally observed dumb-bell-shaped distributions of energetic electrons the instability is possible in three spectral bands. One is below the relativistic gyrofrequency, ωB/γ. The other two are centred round the half of the nonrelativistic gyrofrequency (ωB/2).

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