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Gamma ray line production from cosmic ray spallation reactionsThe gamma ray line intensities due to cosmic ray spallation reactions in clouds, the galactic disk and accreting binary pulsars are calculated. With the most favorable plausible assumptions, only a few lines may be detectable to the level of 0.0000001 per sq. cm per sec. The intensities are compared with those generated in nuclear excitation reactions.
Document ID
19850025692
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Silberberg, R. (Naval Research Lab. Washington, DC, United States)
Tsao, C. H. (Naval Research Lab. Washington, DC, United States)
Letaw, J. R. (Severn Communications Corp.)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 1
Subject Category
Space Radiation
Accession Number
85N34005
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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