A model for GCR-particle fluxes in stony meteorites and production rates of cosmogenic nuclides.

Details A model for GCR-particle fluxes in stony meteorites and production rates of cosmogenic nuclides. A model for GCR-particle fluxes in stony meteorites and production rates of cosmogenic nuclides.

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985jgr....90..722r&link_type=abstract

Journal of Geophysical Research, Vol. 90, Suppl., p. C722 - C728

Physics

35

Cosmic Rays:Stony Meteorites, Stony Meteorites:Cosmic Rays

Scientific paper

A model is presented for the differential fluxes of galactic cosmic ray (GCR) particles with energies above 1 MeV inside any spherical stony meteorite as a function of the meteorite's preatmospheric radius and the sample's depth. This model is based on the Reedy-Arnold equations for the energy-dependent fluxes of GCR particles in the moon and is an extension of flux parameters that were derived for several meteorites of various sizes. This flux model is used to calculate the production rates of many cosmogenic nuclides as a function of radius and depth.

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