Abstract
Elemental abundances of the ambient gas at the site of gamma-ray production in the solar atmosphere are deduced using gamma-ray line observations of a solar flare. The production site is most likely the chromosphere. The resultant abundances are different from local galactic abundances which are thought to be similar to photospheric abundances.
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Resident Research Associate at the Naval Research Laboratory, under the NRC Associateship Program.
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Murphy, R.J. (1989). Solar Abundances Using Gamma-Ray Line Spectroscopy of a Solar Flare. In: Shapiro, M.M., Wefel, J.P. (eds) Cosmic Gamma Rays, Neutrinos, and Related Astrophysics. NATO ASI Series, vol 270. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0921-2_23
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DOI: https://doi.org/10.1007/978-94-009-0921-2_23
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