Energetic electrons near the earth's quasi-perpendicular bow shock

Details Energetic electrons near the earth's quasi-perpendicular bow shock Energetic electrons near the earth's quasi-perpendicular bow shock

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988baicz..39..308v&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 39, no. 5, 1988, p. 308-314.

Astronomy and Astrophysics

Astronomy

6

Bow Waves, Earth (Planet), High Energy Electrons, Shock Waves, Anisotropy, Distribution Functions, Electron Acceleration, Pitch (Inclination), Time Dependence

Scientific paper

The fast Fermi mechanism can, in general, explain the origin of energetic electrons upstream of the quasi-perpendicular bow shock and give reasonable levels of their fluxes. A more detailed analysis, however, shows that energetic electrons (Ee > 10 keV) have a harder spectrum and lower anisotropy than predicted values and they are also observed at pitch angles close to 90° where reflected electrons could not be present.

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