Published 1987
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Cosmic-Ray Energy Spectra Between Ten and Several Hundred GeV/amu for Elements from _(18)Ar to _(25)Ni--Results from HEAO-3
Abstract
Using the relativistic rise of energy loss as a measure of energy, we have determined the energy dependence of the abundances relative to _(26)Fe of the elements _(18)Ar, _(19)K, _(20)Ca, _(21)Sc, _(22)Ti, _(23)V, and _(28)Ni, from 10 to several hundred Ge V /amu. From the energy dependence of the observed Ar/Fe and Ca/Fe ratios we infer primary source ratios for these elements.
Additional Information
© INR. Provided by the NASA Astrophysics Data System. This work was supported by NASA grants NAG 8-498, 500, 502, and NGR 05-002-160, 24-005-050, and 26-008-001.Attached Files
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Additional details
- Eprint ID
- 45685
- Resolver ID
- CaltechAUTHORS:20140512-120447856
- NAG 8-498
- NASA
- NAG 8-500
- NASA
- NAG 8-502
- NASA
- NGR 05-002-160
- NASA
- NGR 24-005-050
- NASA
- NGR 26-008-001
- NASA
- Created
-
2014-05-12Created from EPrint's datestamp field
- Updated
-
2020-03-09Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory
- Other Numbering System Name
- Space Radiation Laboratory
- Other Numbering System Identifier
- 1987-03