Computer Science
Scientific paper
Oct 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ge%26ae..17..820b&link_type=abstract
Geomagnetizm i Aeronomiia, vol. 17, Sept.-Oct. 1977, p. 820-825. In Russian.
Computer Science
Electromagnetic Radiation, Solar Flares, Solar Protons, Solar X-Rays, Solar Cosmic Rays, Solar Radio Emission, Solar Spectra
Scientific paper
The information content of parameters that characterize electromagnetic radiation from solar flares is studied. A response function is obtained which distinguishes flares accompanied by high-energy proton injection from flares not accompanied by such injection. A regression equation is derived for predicting the integrated proton flux at energies in excess of 60 MeV. The results obtained indicate that the characteristics of solar X-ray emission are the most informative for the diagnostics of high-energy solar-cosmic-ray protons.
Bezruchenkova T. M.
Frolov S. G.
Mikriukova N. A.
Pereiaslova N. K.
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