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Abundances of Cosmic Ray Nuclei for 26 ≤ Z ≤ 40 From HEAO-3 Heavy Nuclei Experiment

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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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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URLURL TypeDescription
Binns, W. R.0000-0001-6110-3407
Israel, M. H.0000-0002-8104-208X
Stone, E. C.0000-0002-2010-5462
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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
Group:Space Radiation Laboratory
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NASANGR 05-002-160
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Space Radiation Laboratory1981-12
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Deposited On:22 Apr 2014 21:40
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