Computer Science
Scientific paper
Jun 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988gecoa..52.1649e&link_type=abstract
Geochimica et Cosmochimica Acta (ISSN 0016-7037), vol. 52, June 1988, p. 1649-1662. SNSF-supported research.
Computer Science
134
Chondrites, Cosmic Rays, Isotopic Enrichment, Meteoritic Composition, Radioactive Age Determination, Rare Gases, Argon Isotopes, Cosmochemistry, Helium Isotopes, Krypton Isotopes, Neon Isotopes, Xenon Isotopes
Scientific paper
The cosmic-ray production rates for He-3, Ne-21, Ar-38, Kr-83, and Xe-126 in 13 chondrites were determined on the basis of the isotopic abundance data and the Kr-81/Kr exposure ages. The cosmic-rate production rates were obtained as a function of the shielding-dependent cosmogenic ratio (Ne-22/Ne-21)c and of the chemical compositlion of CI, CM, CO, CV, H, L, LL, EH, and EL chondrites. The ages derived from different noble gases were found to be in good agreement, demonstrating the consistency of the adopted production rate equations.
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