Flux limit of electrons with energies exceeding 0.7 MeV at heights of about 900 KM

Details Flux limit of electrons with energies exceeding 0.7 MeV at heights of about 900 KM Flux limit of electrons with energies exceeding 0.7 MeV at heights of about 900 KM

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980kosis..18...79g&link_type=abstract

Kosmicheskie Issledovaniia, vol. 18, Jan.-Feb. 1980, p. 79-82. In Russian.

Physics

Atmospheric Models, Electron Flux Density, Magnetospheric Electron Density, Satellite Observation, Capture Effect, Diurnal Variations, Electron Energy, Electron Precipitation, Magnetic Fields, Magnetic Variations

Scientific paper

Data from the Meteor satellite are used to construct an averaged model of electron flux limits for the magnetosphere at energies exceeding 0.7 MeV; the model agrees well with theories of the structure of the stationary magnetic field in the capture region. Variations of flux limits on the nightside of the magnetosphere are mainly determined by magnetic variations. The main cause of flux limit variations on the dayside is the augmentation or reduction of electron precipitation in the near-equatorial regions.

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