Quasilongitudinal approximation for whistler-mode waves in the magnetospheric plasma

Details Quasilongitudinal approximation for whistler-mode waves in the magnetospheric plasma Quasilongitudinal approximation for whistler-mode waves in the magnetospheric plasma

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990p%26ss...38.1551s&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 38, Dec. 1990, p. 1551-1553. Research supported by NERC.

Physics

2

Earth Magnetosphere, Refractivity, Space Plasmas, Wave Dispersion, Whistlers, Electron Distribution, Equatorial Regions, Gyrofrequency, Maxwell-Boltzmann Density Function

Scientific paper

The range of applicability of an improved quasi-longitudinal
approximation for whistler-mode waves in the equatorial magnetosphere is
specified. It is pointed out that this approximation can be used at
frequencies less than but not close to the electron gyrofrequency and
wave normal angles less than but not close to the resonance cone angle.

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