The energy spectrum of cosmic rays in the range from 1 MeV to 20 GeV

Details The energy spectrum of cosmic rays in the range from 1 MeV to 20 GeV The energy spectrum of cosmic rays in the range from 1 MeV to 20 GeV

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976izssr..40..543a&link_type=abstract

(Vsesoiuznaia Konferentsiia po Fizike Kosmicheskikh Luchei, Samarkand, Uzbek SSR, Oct. 29-31, 1975.) Akademiia Nauk SSSR, Izvest

Astronomy and Astrophysics

Astronomy

Energy Spectra, Interplanetary Space, Solar Cosmic Rays, Anisotropic Media, Astronomical Models, Correlation, Diffusion Coefficient, Energy Dissipation, Energy Transfer, Interstellar Gas, Proton Flux Density, Steady Flow

Scientific paper

The propagation of the steady solar cosmic ray flux in interplanetary space is analyzed. It is shown that changes in the exponent of the spectrum occur only in the energy range below 1 MeV. At higher energies, the changes are insignificant over the paths from the sun to the earth and from the earth to Jupiter. The anisotropy is approximately 30%, while the gradient exceeds 100% per 1 AU. The model proposed is capable of explaining the observed properties of the steady solar particle flux.

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