Generation of neutrinos in solar flares

Details Generation of neutrinos in solar flares Generation of neutrinos in solar flares

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981izssr..45.1151k&link_type=abstract

(Evropeiskii Simpozium po Kosmicheskim Lucham, 7th, Leningrad, USSR, Sept. 15-19, 1980.) Akademiia Nauk SSSR, Izvestiia, Seriia

Physics

2

Nuclear Reactions, Particle Flux Density, Solar Flares, Solar Neutrinos, Spectral Energy Distribution, Stellar Models, Particle Acceleration, Reaction Kinetics, Solar Protons

Scientific paper

The spectra of neutrinos generated in solar flares have been calculated for accelerated protons with R0 = 100, 200, and 300 MV (where R0 is characteristic hardness). Results are presented in a graphical form. It is shown that for flares with Np (greater than 30 MeV) equal to or greater than 10 to the 34th and R0 equal to or greater than 200 MV, the flux of the flare neutrinos is predominant for energies below 300 MeV; for energies below 14 MeV, the predominant neutrinos are those from the interior of the sun.

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