Can we get the cosmic ray actinide abundance from the study of tracks in meteorites?

Details Can we get the cosmic ray actinide abundance from the study of tracks in meteorites? Can we get the cosmic ray actinide abundance from the study of tracks in meteorites?

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....9..127p&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Late Papers. Volume 9 (A85-22801 0

Computer Science

Abundance, Actinide Series, Cosmic Rays, Meteoritic Composition, Particle Tracks, Uranium 238, Etching, Olivine

Scientific paper

The feasibility of a cosmic ray actinide abundance measurement by means of tracks in meteorites is discussed in the light of recent studies of high-energy U ion tracks in meteoritic minerals. It is concluded that the main difficulties of such measurements may not be those usually thought of, but rather lie in the etching process itself. Olivine is probably not a favorable detector, and man-made detectors are also not entirely safe.

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