Published 1983
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Correlation of Source Abundances of Ultraheavy Cosmic Rays with First Ionization Potential - Results from HEAO-3
Abstract
The cosmic-ray-source abundances inferred from HEAO-3 observation by the Heavy Nuclei Experiment for 30 < Z < 60 generally follow the correlation with first-ionization potential which has previously been observed for Z < 30. However the low Ge abundance suggests that the elemental "volatility" may be an organizing factor.
Additional Information
This work was supported in part by NASA under contracts NAS 8-27976, 77, 78 and grants NGR 05-002-160, 24-005-050, 26-008-001, and NAG8-448.Attached Files
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Additional details
- Eprint ID
- 45174
- Resolver ID
- CaltechAUTHORS:20140423-144319881
- NASA
- NAS 8-27976
- NASA
- NAS 8-27977
- NASA
- NAS 8-27978
- NASA
- NGR 05-002-160
- NASA
- NGR 24-005-050
- NASA
- NGR 26-008-001
- NASA
- NAG8-448
- Created
-
2014-04-23Created 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
- 1983-23