Field-aligned precipitation of greater than 30-keV electrons

Details Field-aligned precipitation of greater than 30-keV electrons Field-aligned precipitation of greater than 30-keV electrons

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976jgr....81.2927w&link_type=abstract

Journal of Geophysical Research, vol. 81, June 1, 1976, p. 2927-2930.

Physics

2

Auroral Zones, Electron Precipitation, High Energy Electrons, Magnetic Effects, Electron Flux Density, Geomagnetic Latitude, Magnetically Trapped Particles, Ogo-6

Scientific paper

A search through 2-3 months of data from Ogo 6 has revealed about 10 cases of field-aligned precipitation of electrons at energies greater than 30 keV. Brief descriptions are given of the four most spectacular of these events, in which the ratio between precipitated and trapped fluxes reached about 100 in one case. Preliminary indications are that such events occur mainly in the evening and midnight sectors and at high geomagnetic latitudes (usually at or above the trapping boundary for electrons with energies greater than 30 keV).

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