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Published 1985 | Version Published
Book Section - Chapter Open

Measurements of Fe and Ar Fragmentation Cross Sections

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Abstract

Measurements are reported of the yields of individual isotopes of Cr to Co (Z = 24 to 27) resulting from the fragmentation of ^(56)Fe, and the isotopes of Mg to K (Z = 12 to 19) resulting from the fragmentation of ^(40)Ar.

Additional Information

© NASA/STI. Provided by the NASA Astrophysics Data System. We are grateful to Dr. M. E. Wiedenbeck, who developed the Monte Carlo approach for evaluating the semi-empirical cross-section formulae, for helpful discussions on a number of aspects of this work. Dr. J. D. Spalding was responsible for developing most of the techniques for resolving Fe isotopes in HlST and offered advice on several occasions. We also thank Dr. H. C. Crawford for help with the Bevalac calibrations. This work was supported in part by NASA under grant NGR 05-002-160 and contract NAS5-28449.

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Published - 1985ICRC____3___91L.pdf

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45454
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CaltechAUTHORS:20140501-203501005

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http://adsabs.harvard.edu/abs/1985ICRC....3...91L (URL)

Funding

NASA
NGR 05-002-160
NASA
NAS5-28449

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2014-05-02
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2020-02-20
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Space Radiation Laboratory
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Space Radiation Labortory
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1985-06