High-energy neutrons and gamma quanta and the characteristics of flare particles

Details High-energy neutrons and gamma quanta and the characteristics of flare particles High-energy neutrons and gamma quanta and the characteristics of flare particles

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984izyak..48.2212k&link_type=abstract

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

Astronomy and Astrophysics

Astronomy

Energetic Particles, Gamma Ray Astronomy, Solar Corpuscular Radiation, Solar Flares, Solar Neutrons, Angular Distribution, Energy Spectra, Helium, Particle Acceleration, Pions

Scientific paper

It is argued that existing experimental data concerning high-energy neutrons and gamma quanta in solar flares can be interpreted using the model of Kocharov and Mandzhavidze (1983). It is shown that the energy spectrum and angular distribution of flare-accelerated particles in a wide energy range can be established by measuring the energy spectrum and flux of neutrons and gamma quanta.

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