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Solar Abundances Using Gamma-Ray Line Spectroscopy of a Solar Flare

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Book cover Cosmic Gamma Rays, Neutrinos, and Related Astrophysics

Part of the book series: NATO ASI Series ((ASIC,volume 270))

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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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© 1989 Kluwer Academic Publishers

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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

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-6903-8

  • Online ISBN: 978-94-009-0921-2

  • eBook Packages: Springer Book Archive

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