Data on the energy spectrum of solar cosmic rays with energies of 100-500 MeV according to stratospheric measurements

Details Data on the energy spectrum of solar cosmic rays with energies of 100-500 MeV according to stratospheric measurements Data on the energy spectrum of solar cosmic rays with energies of 100-500 MeV according to stratospheric measurements

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983izssr..47.1779b&link_type=abstract

(Seminar po Solnechnoi Aktivnosti i Solnechnym Kosmicheskim Lucham, Leningrad, USSR, Nov. 1982) Akademiia Nauk SSSR, Izvestiia,

Physics

Radiation Measurement, Solar Corona, Solar Cosmic Rays, Solar Protons, Spectral Energy Distribution, Stratosphere Radiation, Interplanetary Space, Particle Emission, Proton Energy, Solar Flares, Solar Physics, Solar Terrestrial Interactions

Scientific paper

The experimental energy spectrum of solar protons in the stratosphere is used to calculate the spectrum of solar protons in the source in the framework of diffusion models with instantaneous and prolonged injection. It is shown that prolonged injection causes a change in the character of the solar-cosmic-ray (SCR) spectrum in the source, and that this change should evidently be taken into account in the development of the theory of SCR acceleration, coronal propagation, and emission into interplanetary space. It is noted, however, that experimental data on SCR intensity are insufficiently sensitive to the duration of injection.

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