It has previously been suggested that the energy for the optical emission of solar flares was provided by ionization losses of accelerated particles in the flares. We show that nuclear interaction of these particles would also produce fluxes of secondary neutrons and gamma rays detectable at the ear
Solar flare neutrons and their capture gamma ray emission
โ Scribed by X M. Hua; R. E. Lingenfelter
- Publisher
- Springer
- Year
- 1987
- Tongue
- English
- Weight
- 412 KB
- Volume
- 113
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
We briefly describe our recent Monte Carlo calculations of the energy and angular distributions of neutrons escaping from the solar atmosphere. Comparing the calculation results with measurements of the neutron flux from the flares, we determined the angular distribution and energy spectrum of the accelerated ions. We also describe our calculations of the time dependence of the 2.223 MeV line emission, which provide a sensitive measure of the photospheric ZHe abundance. We find that the SMM measurements of the time dependence of the 2.2 MeV line emission from the flare of 1982 June 3 imply a ZHe/H ratio of (2.3:t:1.2)x10 -s at the 90% confidence level.
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