NASA NTRS · 19890041950
High energy nucleon data bases
Abstract
The buildup of 200 MeV secondary protons in an Al shield according to the Bertini (1976) cross sections and Ranft (1980) cross sections is studied. The number of transmitted secondary photons is presented as a function of shield thickness for two different cross section sets. It is found that the Bertini code does not emphasize high LET components.
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Wilson, John W., Townsend, L. W., Chun, S. Y., Buck, W. W.. 1988-11-01. High energy nucleon data bases. https://ntrs.nasa.gov/citations/19890041950
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