Generation of hydrogen and helium isotopes and gamma radiation in solar flares

Details Generation of hydrogen and helium isotopes and gamma radiation in solar flares Generation of hydrogen and helium isotopes and gamma radiation in solar flares

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975izssr..39q.287i&link_type=abstract

(Mezhdunarodnyi Seminar po Uskoreniiu Chastits i Iadernykh Reaktsii v Kosmose, 6th, Leningrad, USSR, Aug. 19-21, 1974.) Akademii

Physics

Gamma Rays, Helium Isotopes, Hydrogen Isotopes, Particle Production, Solar Flares, Lunar Soil, Neutron Physics, Positron Annihilation, Solar Cosmic Rays, Solar X-Rays

Scientific paper

The theory of nuclear reactions in solar flares is analyzed, and calculations are made of the yield of the secondary nuclei H-2, H-3, and He-3 in the low-energy range. It is suggested that the large amount of He-3 in some flares may be due to the presence of primary He-3 in flare regions, and the role of He-3 in neutron capture on the sun is calculated. It is shown that the excess of H-3 in lunar soil may be provided by nuclear reactions in flares. The dynamics of the formation of the 0.511-MeV gamma line by positron annihilation is thoroughly analyzed.

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