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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

Israel, M. H. and Jones , M. D. and Kamionkowski, M. P. and Klarmann, J. and Stone, E. C. and Waddington, C. J. and Binns, W. R. and Garrard, T. L. (1987) Cosmic-Ray Energy Spectra Between Ten and Several Hundred GeV/amu for Elements from _(18)Ar to _(25)Ni--Results from HEAO-3. In: Proceedings of the 21st International Cosmic Ray Conference. Vol.1. , Nakau, Russia, pp. 330-333. http://resolver.caltech.edu/CaltechAUTHORS:20140512-120447856

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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.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://adsabs.harvard.edu/abs/1987ICRC....1..330IADSArticle
ORCID:
AuthorORCID
Kamionkowski, M. P. 0000-0001-7018-2055
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.
Group:Space Radiation Laboratory
Funders:
Funding AgencyGrant Number
NASANAG 8-498
NASANAG 8-500
NASANAG 8-502
NASANGR 05-002-160
NASANGR 24-005-050
NASANGR 26-008-001
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory1987-03
Record Number:CaltechAUTHORS:20140512-120447856
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20140512-120447856
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:45685
Collection:CaltechAUTHORS
Deposited By: Joy Painter
Deposited On:12 May 2014 19:24
Last Modified:10 Dec 2016 23:28

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