Klarmann, J. and Binns, W. R. and Israel, M. H. and Fickle, R. K. and Waddington, C. J. and Garrard, T. L. and Stone, E. C.
(1981)
Abundances of Cosmic Ray Nuclei for 26 ≤ Z ≤ 40 From HEAO-3 Heavy Nuclei Experiment.
In:
Proceedings of the 17th International Cosmic Ray Conference.
Vol.2.
CEN Saclay
, Gif-sur-Yvette, France, pp. 13-17.
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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.
Item Type: | Book Section |
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Contact Email Address: | dmiles@caltech.edu |
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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 #: 1981-12 |
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Group: | Space Radiation Laboratory |
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Funders: | Funding Agency | Grant Number |
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NASA | NAS8-27976 | NASA | NAS8-27977 | NASA | NAS8-27978 | NASA | NGR 05-002-160 | NASA | 24-005-050 | NASA | 26-008-001 |
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Space Radiation Laboratory | 1981-12 |
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Record Number: | CaltechAUTHORS:20140417-151754488 |
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Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20140417-151754488 |
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Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. |
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ID Code: | 45032 |
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Collection: | CaltechAUTHORS |
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Deposited On: | 22 Apr 2014 21:40 |
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Last Modified: | 09 Mar 2020 13:18 |
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