Ultraheavy cosmic ray tracks in meteorites: A reappraisal, based on calibrations with relativistic ions

Details Ultraheavy cosmic ray tracks in meteorites: A reappraisal, based on calibrations with relativistic ions Ultraheavy cosmic ray tracks in meteorites: A reappraisal, based on calibrations with relativistic ions

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..135p&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 2 p 135-138 (SEE N85-34006 22-93)

Computer Science

Abundance, Cosmic Rays, Heavy Nuclei, Meteorites, Particle Tracks, Etching, Ions, Olivine, Radiation Damage, Uranium

Scientific paper

Experiments have been carried out on tracks of high energy U ions on olivine, a common meteoritic mineral. The results offer an explanation for the lack of success of previous attempts to derive the ultraheavy cosmic ray composition from the study of tracks in meteorites. They also suggest how such experiments should be performed. The methods are described and illustrated.

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