Nuclear processes and neutrino production in solar flares

Details Nuclear processes and neutrino production in solar flares Nuclear processes and neutrino production in solar flares

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985aipc..126..121l&link_type=abstract

IN: Solar neutrinos and neutrino astronomy; Proceedings of the Conference, Lead, SD, August 23-25, 1984 (A86-37626 17-93). New Y

Astronomy and Astrophysics

Astronomy

2

Particle Production, Solar Flares, Solar Neutrinos, Energy Spectra, Flux Quantization, Gamma Ray Astronomy, Particle Acceleration, Time Response

Scientific paper

The determination of flare neutrino flux is approached from the standpoint of recent observations and theoretical results on the nuclear processes in solar flares. Attention is given to the energy spectra and total numbers of accelerated particles in flares, as well as their resulting production of beta(+)-emitting radionuclei and pions; these should be the primary sources of neutrinos. The observed 0.511 MeV line flux for the June 21, 1980 flare is compared with the expected from the number and spectrum of accelerated particles.

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