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

Israel, M. H. and Binns, W. R. and Grossman, D. P. and Klarmann, J. and Margolis, S. H. and Stone, E. C. and Garrard, T. L. and Krombel, K. E. and Brewster, N. R. and Fickle, R. K. and Waddington, C. J. (1983) Correlation of Source Abundances of Ultraheavy Cosmic Rays with First Ionization Potential - Results from HEAO-3. In: 18th International Cosmic Ray Conference, Bangalore, India, August 22 to September 3, 1983. Vol.9. Tata Institute of Fundamental Research , Bombay, India, pp. 305-308. http://resolver.caltech.edu/CaltechAUTHORS:20140423-144319881

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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.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://adsabs.harvard.edu/abs/1983ICRC....9..305IADSArticle
Contact Email Address:dmiles@caltech.edu
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.
Group:Space Radiation Laboratory
Funders:
Funding AgencyGrant Number
NASANAS 8-27976
NASANAS 8-27977
NASANAS 8-27978
NASANGR 05-002-160
NASANGR 24-005-050
NASANGR 26-008-001
NASANAG8-448
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory1983-23
Record Number:CaltechAUTHORS:20140423-144319881
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20140423-144319881
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:45174
Collection:CaltechAUTHORS
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Deposited On:23 Apr 2014 23:15
Last Modified:23 Apr 2014 23:15

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