Energy and pitch-angle characteristics of high-energy solar cosmic rays

Details Energy and pitch-angle characteristics of high-energy solar cosmic rays Energy and pitch-angle characteristics of high-energy solar cosmic rays

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988izssr..52.2396k&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Alma-Ata, Kazakh SSR, Sept. 13-15, 1988) Akademiia Nauk SSSR, Izvestiia, Ser

Physics

High Energy Interactions, Proton Energy, Solar Cosmic Rays, Solar Protons, Earth Magnetosphere, Energy Spectra

Scientific paper

The paper presents an analysis of the pitch-angle and energy characteristics of solar cosmic rays in the highly anisotropic event of May 7, 1978. The investigation is based on neutron-monitor data and a numerical solution of the particle-propagation equation. It is shown that, in this event, the generation of protons on the sun and their escape into the interplanetary medium took place over a time period of less than 0.05 h.

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