Published 1983
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Cosmic Ray Elemental Abundances for 26 ≤ Z ≤ 42 Measured on HEAO-3
Abstract
Measurements from the Heavy Nuclei Experiment (Binns et al. 1981a) aboard the HEAO-3 satellite have been used to extract definite-abundance values for the even charge nuclei and upper limit values for the less abundant odd charge nuclei. Individual peaks in the charge spectrum for even charge nuclei over this charge region are observed and the cosmic ray abundances obtained from this charge spectrum are compared with abundances characteristic of the solar system and with a solar system r process.
Additional Information
© 1983 INSDOC. Provided by the NASA Astrophysics Data System. This work was supported in part by NASA under contracts NAS8-27976,77,78 and grants NGR 05-002-160, 24-005-050, 26-008-001, and NAG 8448.Attached Files
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Additional details
- Eprint ID
- 45165
- Resolver ID
- CaltechAUTHORS:20140423-140020677
- NAS8-27976
- NASA
- NAS8-27977
- NASA
- NAS8-27978
- NASA
- NGR 05-002-160
- NASA
- NGR 24-005-050
- NASA
- NGR 26-008-001
- NASA
- NAG 8448
- NASA
- Created
-
2014-04-24Created 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
- 1983-17