Computer Science
Scientific paper
Jul 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982kosis..20..552a&link_type=abstract
Kosmicheskie Issledovaniia, vol. 20, July-Aug. 1982, p. 552-559. In Russian.
Computer Science
Anisotropy, Energetic Particles, Magnetic Storms, Particle Precipitation, Auroral Zones, Cosmos Satellites, Electron Precipitation, Particle Flux Density, Proton Precipitation, Spatial Distribution, Temporal Distribution
Scientific paper
Cosmos-900 data are used to compare the space-time variations of the precipitation of electrons with energies ranging from 50 to 80 keV with those of the precipitation of protons with energies ranging from 210 to 320 keV during the magnetic storm of July 29, 1977. In contrast to the proton precipitation, the electron precipitation occurs as short bursts and is most intense in the morning-daytime sector. The anisotropy of electrons decreases as their flux increases, and the magnitude of the fluxes is limited by a critical level. The magnitude of fluxes of precipitating electrons was often found to exceed that of quasi-trapped electrons in the auroral zone.
Altyntseva V. I.
Dronov V. A.
Kovtiukh A. S.
Panasiuk M. I.
Polekh Nelya M.
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