The role of superthermal electrons in the formation of the anomalous component of solar cosmic rays

Details The role of superthermal electrons in the formation of the anomalous component of solar cosmic rays The role of superthermal electrons in the formation of the anomalous component of solar cosmic rays

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980izssr..44.2480k&link_type=abstract

(Seminar po Vzaimodeistviiu Kosmicheskikh Luchei so Sredoi, Leningrad, USSR, Nov. 30-Dec. 2, 1979.) Akademiia Nauk SSSR, Izvesti

Physics

Atmospheric Turbulence, Chromosphere, Hot Electrons, Ion Acoustic Waves, Solar Cosmic Rays, Solar Electrons, Helium Isotopes, High Energy Electrons, Magnetohydrodynamic Turbulence, Solar Atmosphere, Solar Flares, Solar X-Rays

Scientific paper

The generation of ion-acoustic turbulence during the penetration of hot electrons with energy exceeding 10 keV into the solar chromosphere is examined. It is shown that this phenomenon leads to conditions that favor the injection of He-3 in the acceleration regime; i.e., energetic electrons, accelerated during flares and producing hard X-rays, can create conditions that explain observed enrichment coefficients.

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