Generation of VLF HISS and chorus in Jupiter's magnetosphere

Details Generation of VLF HISS and chorus in Jupiter's magnetosphere Generation of VLF HISS and chorus in Jupiter's magnetosphere

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ijrsp..20..438s&link_type=abstract

Indian Journal of Radio and Space Physics (ISSN 0367-8393), vol. 20, Dec. 1991, p. 438-443.

Physics

Space Physics

Dawn Chorus, Hiss, Jupiter Atmosphere, Planetary Magnetospheres, Plasma Waves, Very Low Frequencies, Electron Distribution, Gyrofrequency, Whistlers

Scientific paper

Using the plasma and field parameters corresponding to L = 8 temporal growth rates of VLF waves are computed for a non-Maxwellian electron-distribution function in the Jovian magnetosphere. It is found that the presence of bi-Maxwellian electron distributions leads the generation of VLF chorus just below one-half of the electron gyrofrequency and that the presence of a nonthermal drifted Maxwellian tail leads the instability below one-fourth of the electron gyrofrequency. The computed results are in good agreement with those reported by the Voyager 1 and 2 plasma-wave experiments.

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