Solar cosmic rays in the source according to observations of high-energy particles, hard X-rays, and radio emission

Details Solar cosmic rays in the source according to observations of high-energy particles, hard X-rays, and radio emission Solar cosmic rays in the source according to observations of high-energy particles, hard X-rays, and radio emission

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984izyak..48.2158d&link_type=abstract

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

Computer Science

Energetic Particles, Interplanetary Medium, Solar Cosmic Rays, Solar Flares, Solar X-Rays, Type 3 Bursts, High Energy Electrons, Solar Electrons, Solar Protons, Venera Satellites

Scientific paper

An analysis is made of Venera 13 and 14 measurements of electrons with an energy of 0.025-1.6 MeV, protons with an energy of 1-60 MeV, and X-rays with an energy of 0.05-0.75 MeV. The study involved the consideration of 138 solar-cosmic-ray bursts for the period from November 1981 to April 1982. The results are used to determine the characteristics of solar flares that are accompanied by the ejection of accelerated particles into interplanetary space.

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