Observation of protons with energies not less than 100 MeV and electrons with energies not less than 20 MeV on the oriented satellites Cosmos-208 and Cosmos-228

Details Observation of protons with energies not less than 100 MeV and electrons with energies not less than 20 MeV on the oriented satellites Cosmos-208 and Cosmos-228 Observation of protons with energies not less than 100 MeV and electrons with energies not less than 20 MeV on the oriented satellites Cosmos-208 and Cosmos-228

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ge%26ae..23..894b&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 23, Nov.-Dec. 1983, p. 894-900. In Russian.

Physics

Electron Energy, Galactic Cosmic Rays, Proton Energy, Satellite-Borne Instruments, Solar Cosmic Rays, Cerenkov Counters, Cosmos Satellites, Energy Spectra, Radiation Distribution, Scintillation Counters

Scientific paper

The use of scintillation-Cerenkov spectrometers (SEZ-1) on the oriented low-apogee satellites Cosmos 208 and 228 made it possible to observe galactic and solar cosmic rays as well as related albedo radiation in a wide time range (from a few minutes to the 11-year cycle). Using the latitude effect of cosmic rays in the geomagnetic field, it was possible to determine the energy spectrum of variations in the range from the threshold energy of the detector (Ep = 100 MeV) to the geomagnetic cutoff threshold energy at the equator (15 GeV). Readings of the instrument are shown to differ significantly in the case of the orientation of its axis toward the zenith and toward the nadir.

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