Spallogenic origin of nuclei in meteorites

Details Spallogenic origin of nuclei in meteorites Spallogenic origin of nuclei in meteorites

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..398z&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 398-401 (SEE N85-34991 23-93)

Other

Cosmic Rays, Energy Dissipation, Meteoritic Composition, Particle Flux Density, Particle Production, Spallation, Computerized Simulation, Flux (Rate), Fragmentation, Ionization, Mathematical Models, Meteorites, Transport Theory

Scientific paper

Results obtained from a model built to evaluate the different interactions between cosmic rays and meteorites are presented. The model, computes, fluxes as a function of depth inside the meteorite, taking into account energy losses by ionization and spallation reactions which induce both particle destruction and production. This procedure, in which particle fluxes and cross sections are treated independently from each other, differs significantly from the thick target approach based on the measurement of spallation products generated in accelerator experiments.

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