Abstract
Gamma-ray production cross sections have been measured for the γ-ray lines which are most strongly excited in the proton bombardment of C, O, Mg, Si, and Fe targets of natural isotopic composition. High resolution germanium detectors were used to collect γ-ray spectra at proton bombarding energies of 20, 30, 33, 40 and 50 MeV.
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© 1988 D. Reidel Publishing Company, Dordrecht, Holland
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Lesko, K.T., Norman, E.B., Larimer, R.M., Crane, S.G. (1988). Measurements of Cross Sections Relevant to γ-Ray Line Astronomy. In: Shapiro, M.M., Wefel, J.P. (eds) Genesis and Propagation of Cosmic Rays. NATO ASI Series, vol 220. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4025-3_24
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DOI: https://doi.org/10.1007/978-94-009-4025-3_24
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-8286-0
Online ISBN: 978-94-009-4025-3
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