Some features of solar-flare electromagnetic and corpuscular radiation production

Details Some features of solar-flare electromagnetic and corpuscular radiation production Some features of solar-flare electromagnetic and corpuscular radiation production

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979izssr..43..749b&link_type=abstract

(Seminar po Iadernoi Kosmicheskoi Fizike, 10th, Leningrad, USSR, Oct. 1978.) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskaia

Computer Science

Electromagnetic Radiation, Particle Production, Solar Corpuscular Radiation, Solar Flares, Solar Protons, Distribution Functions, Microwave Frequencies, Solar Activity, Solar Electrons, Solar Radio Bursts

Scientific paper

The intensity distribution functions at maximum of 87 solar proton events with proton energies greater than 10 MeV and of 323 solar microwave radio bursts are studied. The results show that the number of accelerated protons is roughly equal to the number of accelerated electrons raised to some power in the range from 2 to 2.5. It is concluded that proton acceleration to energies up to 10 MeV occurs only in some flares accompanied by radio bursts at frequencies of 2695 and 8800 MHz.

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