Mathematics
Scientific paper
May 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980e%26psl..47..361e&link_type=abstract
Earth and Planetary Science Letters, vol. 47, no. 3, May 1980, p. 361-369. Research supported by the Bundesministerium für Fors
Mathematics
10
Cosmic Rays, Manganese Isotopes, Meteoritic Composition, Spallation, Depth, Evolution (Development), Flux (Rate), Helium, Mathematical Models, Neon, Radiation Effects, Tables (Data), Meteorites, H6 Chondrites, St. Severin Meteorite, Spallation, Depth, Manganese 53, Samples, Meteorite, Models, Particles, Flux, Isotopes, Spallogenic Gases, Helium, Neon, Isotopic Ratios, Cosmic Rays, Data, Exposure Ages, Experiments, Iron, Nickel, Cobalt, Comparisons
Scientific paper
The contents of spallogenic Mn-53 and target elements for its production were determined in 80- to 400-mg samples from 13 different locations of the LL6 chondrite St. Severin, along the 34.8-cm drill core AIII. The Mn-53 content increases from the surface to the center of the stone by approximately 30%. The variation with depth is described by several models, presuming that appropriate primary and secondary particle fluxes are chosen. The Mn-53 saturation activities are linearly correlated with the spallogenic He-3/Ne-21 and Ne-22/Ne-21 ratios, which suggests the possibility of eliminating uncertainties in the determination of Mn-53 cosmic ray exposure ages arising from depth effects and terrestrial residence times.
Englert Peter
Herr W.
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