Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983izssr..47.2066d&link_type=abstract
(Seminar po Solnechnoi Aktivnosti i Solnechnym Kosmicheskim Lucham, Leningrad, USSR, Nov. 1982) Akademiia Nauk SSSR, Izvestiia,
Astronomy and Astrophysics
Astronomy
Radio Astronomy, Solar Flares, Solar Radio Emission, Proton Energy, Solar Protons, Statistical Distributions
Scientific paper
An analysis was made of the statistical distributions of fluxes of protons with energies exceeding 10 MeV recorded in the orbit of the earth in 1967-1973 after about 600 radio bursts at 3-5 GHz. The results of the analysis show that nonproton events dominate in the case of low-intensity (with respect to the radio flux) flares or flares that are unfavorably located with respect to the earth. Conversely, in the case of high-intensity bursts and favorable position of the flare with respect to the earth, nonproton events are almost completely absent. The mechanisms thought to be responsible for the U-shaped spectra of some of the events are discussed.
Dianov G. A.
Molchanov A. P.
Pogodin I. E.
Stupishin A. G.
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