Interpretation of solar flare γ-Ray continuum observations

Details Interpretation of solar flare γ-Ray continuum observations Interpretation of solar flare γ-Ray continuum observations

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993adspr..13..259a&link_type=abstract

Advances in Space Research, Volume 13, Issue 9, p. 259-262.

Physics

1

Scientific paper

The γ-ray spectrometer on board the Solar Maximum Mission detected a large number of solar flares with γ-ray emission in the 10-100 MeV range. A smaller number of these events displayed evidence of a hardening of the photon spectrum around 70 MeV indicating the presence of neutral pion decay γ-rays. We consider thick-target calculations of the interaction of accelerated protons with the ambient solar atmosphere to address the production of this pion decay radiation.

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