Fluxes of solar and galactic cosmic rays at satellite orbits

Details Fluxes of solar and galactic cosmic rays at satellite orbits Fluxes of solar and galactic cosmic rays at satellite orbits

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kosis..23..944g&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 23, Nov.-Dec. 1985, p. 944-946. In Russian.

Mathematics

Probability

Galactic Cosmic Rays, Magnetospheric Instability, Satellite Observation, Satellite Orbits, Solar Cosmic Rays, Circular Orbits, Elliptical Orbits, Energy Spectra, Flux Quantization, Solar Protons

Scientific paper

A method is developed for comparing fluxes of solar and galactic cosmic rays at satellite orbits and in interplanetary space. The energy spectra of particles on various L-shells can be determined when there is information about cosmic rays outside the magnetosphere. The energy spectra of cosmic-ray particles encountered by a satellite can be determined if the probability of the satellite staying on an L-shell is known.

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