Published 1981
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Abundances of Cosmic Ray Nuclei for 26 ≤ Z ≤ 40 From HEAO-3 Heavy Nuclei Experiment
Abstract
Individual elements in the cosmic radiation of even atomic number (Z)in the interval 26≤ Z ≤ 40 have been resolved and their relative abundances measured. The results are inconsistent with a cosmic-ray source whose composition in this charge interval is dominated by r-process nucleosynthesis.
Additional Information
© IUPAP. Provided by the NASA Astrophysics Data System. We thank T. Aufrance, B. Gauld, D. Grossman, K. Krombel, and D. Mitchell for assistance in programming for data analysis; R. N. F. Walker for development of thje propagation code and S. H. Margolis and K. L. Hainebach for the program to evaluate crosssections for the propagation code. The research was supported in part by NASA under contracts NASB-27976,77,78 and grants NGR 05-002-160, 24-005-050, and 26-008-001. Space Radiation Laboratory SRL ID #: 1981-12Attached Files
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Additional details
- Eprint ID
- 45032
- Resolver ID
- CaltechAUTHORS:20140417-151754488
- NASA
- NAS8-27976
- NASA
- NAS8-27977
- NASA
- NAS8-27978
- NASA
- NGR 05-002-160
- NASA
- 24-005-050
- NASA
- 26-008-001
- Created
-
2014-04-22Created 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
- 1981-12