Products from cosmic-ray interactions in extraterrestrial matter: What they tell us about radiation backgrounds in space

Details Products from cosmic-ray interactions in extraterrestrial matter: What they tell us about radiation backgrounds in space Products from cosmic-ray interactions in extraterrestrial matter: What they tell us about radiation backgrounds in space

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987stin...8826288r&link_type=abstract

Presented at the Conference on High Energy Radiation Backgrounds in Space, Sanibel Island, Fla., 3 Nov. 1987

Physics

High Energy Interactions, Radiation Hazards, Cosmic Rays, Extraterrestrial Matter, Meteorites, Alpha Particles, Energetic Particles, Heavy Ions, Nuclear Reactions, Protons, Time Dependence

Scientific paper

The nuclides and the heavy-nuclei tracks made by the interactions of solar and galactic cosmic-ray particles with meteorites, lunar samples, and the Earth have been extensively studied, simulated, and modelled. Most research involves the use of these cosmogenic products to study the history of the targets or of the cosmic rays. However, much work has also been done in understanding these interactions and in predicting their rates as a function of the target's size and shape and of the location inside the target. These studies apply to any object exposed to cosmic rays. The fluxes as a function of depth for cosmic-ray primary and secondary particles vary greatly with particle energy and type. The variations of the fluxes of these cosmic rays in the past have been studied. Energetic solar particles are unpredictable and are the greatest potential radiation hazard in space.

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