Abundance of the Super-Heavy (Z>55) Galactic Cosmic Ray Nuclei by the Meteorite Track Data: Comparison with the Satellite Apparatus Measuring and the Sun and Solar System Values

Details Abundance of the Super-Heavy (Z>55) Galactic Cosmic Ray Nuclei by the Meteorite Track Data: Comparison with the Satellite Apparatus Measuring and the Sun and Solar System Values Abundance of the Super-Heavy (Z>55) Galactic Cosmic Ray Nuclei by the Meteorite Track Data: Comparison with the Satellite Apparatus Measuring and the Sun and Solar System Values

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1597b&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1597

Computer Science

Scientific paper

Track parameters in olivine crystals from pallasite Marjalahti were
recorded. Some results of comparison of obtained nucleus abundance
distribution data with the results of satellite apparatus measuring and
Sun and solar system values are presented.

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