Energy spectrum of particles accelerated in solar flares

Details Energy spectrum of particles accelerated in solar flares Energy spectrum of particles accelerated in solar flares

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984izyak..48.2246k&link_type=abstract

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

Physics

Energy Spectra, Particle Acceleration, Solar Flares, Solar Protons, Gamma Ray Spectra, Interplanetary Space, Solar Cosmic Rays, Solar Neutrinos

Scientific paper

A large volume of data concerning the energy spectrum of flare particles as measured in the stratosphere and interplanetary space is analyzed. Particular consideration is given to nuclear gamma-lines and the in situ energy spectrum of particles; the effect of coronal propagation on the shape of the energy spectrum of particles with energies less than 100 MeV/nucleon; and solar neutrinos and the energy spectrum of accelerated particles in the high-energy region. It is shown that different approaches to the determination of the energy spectra give similar results, which supports the hypothesis that the shape of the spectrum of flare-accelerated particles remains constant in the 10-1000 MeV range; the power-law spectrum is considered to be the most probable.

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