Some comments on the whistler mode instability at Jupiter

Details Some comments on the whistler mode instability at Jupiter Some comments on the whistler mode instability at Jupiter

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976jgr....81.1787s&link_type=abstract

Journal of Geophysical Research, vol. 81, Apr. 1, 1976, p. 1787-1790. Research supported by the TRW Systems Independent Researc

Physics

1

Jupiter (Planet), Planetary Radiation, Radiation Belts, Whistlers, Electron Distribution, Magnetospheric Instability, Modulated Continuous Radiation, Planetary Magnetospheres

Scientific paper

The paper considers the possibility that electrons with energies exceeding 21 MeV at Jupiter interact resonantly with obliquely propagating whistler mode waves. The equatorial pitch angle distributions are deduced from the Pioneer 10 and 11 data points of Van Allen et al. (1975). For the L shell subgroup 7, there is observed a 'hat-shaped' pitch angle distribution which is similar to that found within the earth plasmasphere.

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