The limb darkening of neutron capture line at 2.22 MeV and gamma-ray line emission model in solar flares

Details The limb darkening of neutron capture line at 2.22 MeV and gamma-ray line emission model in solar flares The limb darkening of neutron capture line at 2.22 MeV and gamma-ray line emission model in solar flares

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....4...89y&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Conference Papers. Volume 4 (A85-2

Astronomy and Astrophysics

Astronomy

Gamma Ray Astronomy, Limb Darkening, Neutron Emission, Solar Flares, Solar Neutrons, Solar Protons, Nuclear Capture, Particle Acceleration, Photosphere, Positron Annihilation, Solar Atmosphere

Scientific paper

Ratios between the intensity of neutron capture line at 2.22 MeV and
that of C deexcitation line at 4.44 MeV for eight large flares observed
by the Hinotori satellite were analysed. The results show clear evidence
of the limb darkening of 2.22 MeV line. From this results, the site of
nuclear reactions and the interaction model in solar flares are studied.

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