The statistical characteristics and mechanisms of solar flare gamma-ray emissions.

Details The statistical characteristics and mechanisms of solar flare gamma-ray emissions. The statistical characteristics and mechanisms of solar flare gamma-ray emissions.

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pabei...9....3x&link_type=abstract

Prog. Astron., Vol. 9, No. 1, p. 3 - 14

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Scientific paper

During the 21st solar activity cycle, about two hundred solar γ-ray flares were observed by the γ-ray spectrometer on SMM and the γ-ray detector on the Hinotori satellite. Analyses of these observational data give a number of statistical characteristics concerning solar flare γ-ray emission. The author presents several characteristics, i.e. distribution of the occurrence rate for flares, time structure, distribution of event size, directivity, the relation of γ-ray continuum with other kinds of emissions, "MeV excess", as well as solar flare γ-ray line emissions. Finally, emission mechanisms of solar flare γ-rays are briefly described.

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