Binns, W. R. and Israel, M. H. and Klarmann, J. and Garrard, T. L. and Stone, E. C. and Waddington, C. J.
(1987)
Measurements of Ultraheavy Cosmic Rays with HEAO-3.
In:
Essays in Space Science.
NASA Conference Publication.
No.CP-2464.
NASA
, Washington, DC, pp. 173-179.
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Abstract
The HEAO-3 Heavy Nuclei Experiment has measured abundances of elements from ^(18)Ar to ^(92)U in the cosmic rays. The results of the ultraheavy elements, those with atomic numbers greater than 30, indicate that the sources of cosmic rays contain a mixture of r-process and s-process material similar to that found in the solar system. This result is at variance with previous indications that the sources are greatly enhanced with freshly synthesized r-process material. Apparent discrepancies between our results and the accepted solar-system abundances have led to a re-examination of data on photospheric abundances of Ge and Pb, resulting in suggested reductions in their values.
Item Type: | Book Section |
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Contact Email Address: | dmiles@caltech.edu |
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Additional Information: | This work was supported in part by NASA contracts NAS 8-27976, 77, 78; by NASA grants NAG 8-498, 500, 502; and by NASA grants NGR 05-002-0160, 24-005-050, 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 | NAS 8-27976 | NASA | NAS 8-27977 | NASA | NAS 8-27978 | 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 | 1986-02 |
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Series Name: | NASA Conference Publication |
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Issue or Number: | CP-2464 |
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Record Number: | CaltechAUTHORS:20140429-140516645 |
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Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20140429-140516645 |
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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: | 45317 |
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Collection: | CaltechAUTHORS |
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Deposited By: |
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Deposited On: | 29 Apr 2014 23:41 |
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Last Modified: | 09 Mar 2020 13:18 |
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