Gamma-radiation from the solar flare of 15 June 1991 as evidence of long-term acceleration of protons up to 10 GeV

Details Gamma-radiation from the solar flare of 15 June 1991 as evidence of long-term acceleration of protons up to 10 GeV Gamma-radiation from the solar flare of 15 June 1991 as evidence of long-term acceleration of protons up to 10 GeV

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993roizf..57..138k&link_type=abstract

Rossijskaya Akademiya Nauk, Izvestiya, Seriya Fizicheskaya (ISSN 0367-6765), vol. 57, no. 7, p. 138-141.

Computer Science

Gamma Ray Bursts, Particle Acceleration, Solar Flares, Solar Protons, Energetic Particles, Solar Atmosphere

Scientific paper

The power spectrum of gamma-radiation up to 2 GeV observed during the flare of 15 June 1991 indicates that the primary protons had a power spectrum extending at least to 10 GeV. Comparing the time profiles of centimeter-wave emission, gamma-radiation in nuclear lines in the 0.8-8 MeV range, and high-energy gamma-radiation from pion decay, their coincidence is found, indicating the simultaneous long-term acceleration of particles after the impulsive phase of the solar flare.

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