Computer Science
Scientific paper
Sep 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989e%26psl..94..171z&link_type=abstract
Earth and Planetary Science Letters (ISSN 0012-821X), vol. 94, no. 3-4, Sept. 1989, p. 171-188.
Computer Science
11
Galactic Cosmic Rays, Iron Meteorites, Particle Energy, Radiation Distribution, Spallation, Monte Carlo Method, Nuclear Reactions, Secondary Emission, Meteorites, Cosmic Rays, Spallation, Iron Meteorites, Origin, Models, Depth, Particles, Flux, Production Rate, Nuclides, Energy, Parameters, Neutrons, Protons, Irradiation, Grant, Comparisons, Calculations, Diagrams, Abundance, Transport, Age
Scientific paper
A model for evaluating the variations with depth of high-energy particle fluxes propagating inside spherical solid bodies is proposed for use in calculating the production rates of spallogenic nuclides in meteorites. It is shown that the production by secondary particles is the major process determining the abundances of the produced nuclides. The angular distribution of these particles is of little incidence. The model is restricted to energies above 300 MeV. Results are presented from application of the model to the products of high-energy reactions induced in iron meteorites.
Audouze Jean
Malinie Guy
Zanda Brigitte
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