Formation of secondary high-energy electrons in the low-density medium at high altitudes

Details Formation of secondary high-energy electrons in the low-density medium at high altitudes Formation of secondary high-energy electrons in the low-density medium at high altitudes

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984kosis..22..947k&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 22, Nov.-Dec. 1984, p. 947-949. In Russian.

Computer Science

Sound

Geophysics, High Energy Electrons, Secondary Emission, Upper Atmosphere, Earth Albedo, Flux Quantization, Pitch (Inclination), Satellite Sounding, Scintillation Counters

Scientific paper

The formation of a high-energy secondary electron halo at high altitudes (approximately 500 km) in the upper atmosphere is examined on the basis of Cosmos-225 scintillation-counter data for electron energies of 70-1000 and 100-1000 MeV. This secondary-electron flux is shown to be roughly equal to the flux of albedo electrons, which serves as a confirmation of Grigorov's (1977) model concerning the existence of a radiation belt formed of electrons with energies exceeding 100 MeV.

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