Relativistic protons in the solar flare of September 24, 1977

Details Relativistic protons in the solar flare of September 24, 1977 Relativistic protons in the solar flare of September 24, 1977

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980kosis..18..801b&link_type=abstract

Kosmicheskie Issledovaniia, vol. 18, Sept.-Oct. 1980, p. 801-804. In Russian.

Physics

Particle Acceleration, Relativistic Particles, Solar Flares, Solar Protons, Electron Acceleration, Prognoz Satellites, Solar Atmosphere

Scientific paper

Prognoz-6 data on the solar flare of September 24, 1977 are examined. The results confirm Lin's hypothesis (1974) according to which two types of acceleration processes can exist in large flares. In one process, electrons are accelerated to energies of several tens of keV and protons are accelerated to energies of several hundred keV. In the second process, relativistic electrons and protons are produced.

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