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Published 1987 | Version Published
Book Section - Chapter Open

Cosmic-Ray Energy Spectra Between Ten and Several Hundred GeV/amu for Elements from _(18)Ar to _(25)Ni--Results from HEAO-3

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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.

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Eprint ID
45685
Resolver ID
CaltechAUTHORS:20140512-120447856

Related works

Describes
http://adsabs.harvard.edu/abs/1987ICRC....1..330I (URL)

Funding

NASA
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

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2014-05-12
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Updated
2020-03-09
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Space Radiation Laboratory
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Space Radiation Laboratory
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1987-03