Equatorial gyroresonance between electrons and magnetospherically reflected whistlers

Details Equatorial gyroresonance between electrons and magnetospherically reflected whistlers Equatorial gyroresonance between electrons and magnetospherically reflected whistlers

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990georl..17.1865j&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 17, Oct. 1990, p. 1865-1868.

Physics

12

Earth Magnetosphere, Equatorial Atmosphere, Gyrofrequency, Plasma Waves, Whistlers, Electron Energy, Space Plasmas, Spectrograms

Scientific paper

Magnetospherically reflected whistlers resonantly interact with energetic (of order 100 keV) electrons in a relatively narrow energy range during multiple equatorial crossings over a wide range of L-shells (L between 1.5 and 4). Results indicate that wave energy that enters the magnetosphere at a fixed location can potentially contribute to the loss of particles over a wide range of latitudes.

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