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.
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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 |
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| 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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| Group: | Space Radiation Laboratory |
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| Funders: | | Funding Agency | Grant Number |
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| 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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| Other Numbering System: | | Other Numbering System Name | Other Numbering System ID |
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| Space Radiation Laboratory | 1987-03 |
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| Record Number: | CaltechAUTHORS:20140512-120447856 |
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| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20140512-120447856 |
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| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. |
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| ID Code: | 45685 |
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| Collection: | CaltechAUTHORS |
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| Deposited By: |
Joy Painter
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| Deposited On: | 12 May 2014 19:24 |
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| Last Modified: | 09 Mar 2020 13:18 |
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