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The cosmic ray source compositionThe cosmic ray source composition is shown to be related to the observed cosmic ray abundances by a set of linear equations which are valid for either ad hoc pathlength distributions or quantitative solutions to Galactic propagation models. These relations can be used to propagate abundances from the source or to the source, and the method described here allows a simple propagation of abundance uncertainties. A simultaneous analysis of B/C and (21-25)Fe indicates a need for truncation of the pathlength distribution.
Document ID
19850040848
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Margolis, S. H. (Washington University St. Louis, MO, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1983
Subject Category
Space Radiation
Meeting Information
Meeting: International Cosmic Ray Conference
Location: Bangalore
Country: India
Start Date: August 22, 1983
End Date: September 3, 1983
Accession Number
85A22999
Funding Number(s)
CONTRACT_GRANT: NAG8-448
Distribution Limits
Public
Copyright
Other

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