Solar flare neutron production and the angular dependence of the capture gamma-ray emission

Details Solar flare neutron production and the angular dependence of the capture gamma-ray emission Solar flare neutron production and the angular dependence of the capture gamma-ray emission

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..107..351h&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 107, no. 2, 1987, p. 351-383.

Physics

103

Capture Effect, Gamma Ray Bursts, Monte Carlo Method, Neutron Emission, Solar Atmosphere, Solar Flares, Solar Neutrons, Angular Distribution, Computerized Simulation, Energy Spectra, Heavy Ions, Nuclear Reactions, Particle Acceleration

Scientific paper

The depth dependence of the production of neutrons and capture gamma-ray line emission are calculated by Monte Carlo simulation of the nuclear processes taking place when flare-accelerated ions interact with the solar atmospheres. The calculations also give the heliocentric-angular dependence of the 2.223 MeV neutron capture line emission as a function of accelerated-ion energy spectrum and angular distribution. These results are compared with observations to determine the energy spectrum shape and total ion number for various flares.

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