Effects of the coronal propagation of solar protons with an energy exceeding 100 MeV

Details Effects of the coronal propagation of solar protons with an energy exceeding 100 MeV Effects of the coronal propagation of solar protons with an energy exceeding 100 MeV

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984izyak..48.2171b&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, July 1984) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskai

Physics

Energy Spectra, Proton Energy, Solar Corona, Solar Cosmic Rays, Solar Protons, Energetic Particles, Interplanetary Medium, Propagation Velocity, Proton Energy, Proton Flux Density, Time Lag

Scientific paper

It is shown that the energy spectrum of solar protons with energies of 100-1500 MeV, integrated over the injection time, is not significantly sensitive to coronal effects and has an average exponent (in the power spectrum) of 3.08 + or - 0.11. The coronal effects for fast solar proton events are manifested in the ejection delay of the first particles (which does not depend on particle energy) and in prolonged injection with a characteristic time that depends on energy.

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