Flux dynamics and spectra of protons in a series of solar proton events in July 1985 according to Prognoz-10 satellite measurements

Details Flux dynamics and spectra of protons in a series of solar proton events in July 1985 according to Prognoz-10 satellite measurements Flux dynamics and spectra of protons in a series of solar proton events in July 1985 according to Prognoz-10 satellite measurements

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988izssr..52.2377a&link_type=abstract

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

Physics

Proton Beams, Solar Protons, Energy Bands, Particle Telescopes

Scientific paper

Prognoz-10 data on four solar proton events observed in July 1985 are analyzed. Preliminary results indicate that the isotropic diffusion approximation cannot be used to describe the time profiles of the fluxes, that the solar-cosmic-ray spectra in all the events are hard, and that particle arrival in all the events (including the distant beyond-the-limb flares) was fast.

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