The basic characteristics of solar cosmic ray fluxes during the period from September 1 to 16, 1971

Details The basic characteristics of solar cosmic ray fluxes during the period from September 1 to 16, 1971 The basic characteristics of solar cosmic ray fluxes during the period from September 1 to 16, 1971

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977kosis..15..566n&link_type=abstract

Kosmicheskie Issledovaniia, vol. 15, July-Aug. 1977, p. 566-572. In Russian.

Physics

Earth Magnetosphere, Proton Flux Density, Solar Cosmic Rays, Solar Protons, Energy Spectra, Polar Regions, Solar Flux Density

Scientific paper

During the first half of September, 1971, proton fluxes with energies of
5, 15, 25, 40, and 65 MeV were recorded at heights of 650 km in the
high-latitude regions of the magnetosphere. The proton energy spectrum
is described by a power function whose exponent varies with time from
0.6 to 2.0 at energies between 5 and 65 MeV and between 1.3 and 3.4 MeV.

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