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Abundances from solar-flare gamma-ray line spectroscopyElemental abundances of the ambient gas at the site of gamma ray line production inthe solar atmosphere are deduced using gamma ray line observations from a solar flare. The resultant abundances are different from local galactic abundances which are thought to be similar to photospheric abundances.
Document ID
19850026481
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Murphy, R. J. (Maryland Univ. College Park, United States)
Ramaty, R. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Forrest, D. J. (New Hampshire Univ.)
Kozlovsky, B. (Tel Aviv Univ.)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 4
Subject Category
Solar Physics
Report/Patent Number
SH-2.1-13
Report Number: SH-2.1-13
Accession Number
85N34794
Funding Number(s)
CONTRACT_GRANT: NAS5-28609
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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