Accelerator experiments on the contribution of secondary particles to the production of cosmogenic nuclides in meteorites

Details Accelerator experiments on the contribution of secondary particles to the production of cosmogenic nuclides in meteorites Accelerator experiments on the contribution of secondary particles to the production of cosmogenic nuclides in meteorites

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..390d&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 390-393 (SEE N85-34991 23-93)

Computer Science

Acceleration, Cosmic Ray Showers, Cosmic Rays, Galactic Radiation, Meteoritic Composition, Particle Flux Density, Chemical Composition, Computerized Simulation, Electron Bombardment, Meteoroid Showers, Particle Beams, Secondary Cosmic Rays

Scientific paper

Through the interaction of galactic cosmic particle radiation (GCR) a wide variety of cosmogenic nuclides is produced in meteorites. They provide historical information about the cosmic radiation and the bombarded meteorites. An important way to understand the production mechanisms of cosmogenic nuclides in meteorites is to gather information about the depth and size dependence of the build-up of Galactic Rays Cosmic-secondary particles within meteorites of different sizes and chemical compositions. Simulation experiments with meteorite models offer an alternative to direct observation providing a data basis to describe the development and action of the secondary cascade induced by the GCR in meteorites.

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