Solar flare neutrons and gamma ray lines

Details Solar flare neutrons and gamma ray lines Solar flare neutrons and gamma ray lines

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....4..101l&link_type=abstract

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

Physics

Energy Spectra, Gamma Ray Spectra, Interplanetary Medium, Neutron Emission, Particle Acceleration, Solar Flares, Solar Neutrons, Anisotropy, Bessel Functions, Charged Particles, Photosphere

Scientific paper

Energy spectrum of accelerated protons and nuclei at the site of the June 21, 1980, limb flare is derived by a new technique, using observations of the time-dependent flux of high-energy neutrons at the earth. This energy spectrum is very similar to the energy spectra of seven disk flares for which the accelerated particle spectra have been previously derived (Lingenfelter et al., 1965; Lingenfelter and Ramaty, 1967) using observations of 4-7-MeV to 2.223-MeV fluence ratios.

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