Generation and propagation of high-energy solar cosmic rays

Details Generation and propagation of high-energy solar cosmic rays Generation and propagation of high-energy solar cosmic rays

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988izssr..52.2368k&link_type=abstract

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

Other

High Energy Interactions, Proton Energy, Radiation Distribution, Solar Cosmic Rays, Solar Protons, Diffusion Theory, Particle Acceleration

Scientific paper

The generation and propagation of high-energy solar cosmic rays (SCRs) are investigated on the basis of neutron-monitor and satellite data, as well as on the basis of numerical solutions of an equation for the propagation of flare-accelerated particles. Among other findings it is shown that the SCR drift has a significant effect on the space-time intensity and anisotropy characteristics of high-energy solar protons. In addition, the shape of the SCR energy spectrum can change significantly during the propagation of flare SCRs from the source to the detection point.

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