2.2 MeV gamma-ray line observed during two SN solar flares

Astronomy and Astrophysics – Astronomy

Scientific paper

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Gamma Ray Astronomy, Gamma Ray Spectra, Solar Flares, Solar Neutrinos, Solar Spectra, Energy Spectra, Galactic Nuclei, Gamma Ray Spectrometers, Line Spectra

Scientific paper

The 2.2 MeV line flux was monitored during airborne omnidirectional gamma-ray detector observations in the 0.3-10 MeV range of several solar flares of importance SN and SF. The observations were conducted around noon time, at 23 deg S latitude, on Dec. 15, 1978. Statistically significant line fluxes of 0.0155 plus or minus 0.005 photons/sq cm per sec and 0.00997 plus or minus 0.00485 photons/sq cm per sec were observed within a few minutes of the optical maxima for the cases of two long duration SN flares, while only upper limits were obtained for SF flares.

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