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Diffuse galactic gamma ray linesThe production rate of 4.44-MeV line for a variety of assumed cosmic ray spectra is evaluated. These results are compared with reported galactic gamma-ray line intensities and are consistent with a low energy cosmic ray density which increases toward the galactic center in proportion to the molecular gas density.
Document ID
19770014051
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Lingenfelter, R. E.
(Calif. Univ. Los Angeles, United States)
Ramaty, R.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 8, 2013
Publication Date
January 1, 1977
Publication Information
Publication: The Struct. and Content of the Galaxy and Galactic Gamma Rays
Subject Category
Space Radiation
Accession Number
77N20995
Funding Number(s)
CONTRACT_GRANT: NSF AST-67-08178
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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