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

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

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985rpspr...6...32k&link_type=abstract

In its USSR Rept.: Space (JPRS-USP-85-005) p 32-33 (SEE N86-14111 04-88) Transl. into ENGLISH from Kosmich. Issled. (Moscow),

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 to 1000 and 100 to 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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