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Solar flare gamma-ray line spectroscopyThe techniques and the results of solar elemental abundance determinations using observations of gamma ray lines from the April 27 1981 olar flare were outlined. The techniques are elaborated on and observed and the best-fitting theoretical spectra are presented. Numerical values for the photon fluences and the total number of protons involved in the thick-target production of these gamma rays are derived.
Document ID
19850026482
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Murphy, R. J. (Maryland Univ. College Park, United States)
Forrest, D. J. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Ramaty, R. (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-2.1-14
Report Number: SH-2.1-14
Accession Number
85N34795
Funding Number(s)
CONTRACT_GRANT: NAS5-28609
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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