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Published 1983 | Version Published
Book Section - Chapter Open

Correlation of Source Abundances of Ultraheavy Cosmic Rays with First Ionization Potential - Results from HEAO-3

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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.

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Eprint ID
45174
Resolver ID
CaltechAUTHORS:20140423-144319881

Related works

Describes
http://adsabs.harvard.edu/abs/1983ICRC....9..305I (URL)

Funding

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

Dates

Created
2014-04-23
Created from EPrint's datestamp field
Updated
2020-03-09
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Space Radiation Laboratory
Other Numbering System Name
Space Radiation Laboratory
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1983-23