Energetic electron components at geosynchronous orbit

Details Energetic electron components at geosynchronous orbit Energetic electron components at geosynchronous orbit

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989georl..16..147c&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 16, Feb. 1989, p. 147-150. Research sponsored by DOE.

Other

34

Geosynchronous Orbits, High Energy Electrons, Magnetospheric Instability, Satellite Observation, Earth Magnetosphere, Electron Density (Concentration), Energy Distribution, Magnetic Storms, Spectral Energy Distribution

Scientific paper

Energy distribution functions have been derived from energetic (30-2000 keV) electron fluxes observed simultaneously by three geosynchronous orbit satellites throughout the year 1986. These distributions, as well as others derived from empirical models of outer magnetospheric electron fluxes, can be resolved into two distinct relativistic Maxwellian components which are each fully parameterized by a density and a temperature. A four-parameter characterization is presented which provides a new, simplified procedure for the interpretation of energetic electron data in the outer magnetosphere.

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