Time structure of gamma rays from the solar flare of 26 March 1991

Physics

Scientific paper

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Gamma Ray Bursts, Gamma Ray Telescopes, Solar Flares, Gamma Ray Spectra, Radio Emission

Scientific paper

The paper presents results of a time analysis of gamma-ray fluxes with
energies exceeding 30 MeV recorded by the Gamma-1 orbital telescope
during the solar flare of 26 March 1991. The observed quasi-periodicity
of the radiation peaks with characteristic times of 50 sec and 3-4 min
may reflect the temporal characteristics of the acceleration process.

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