Super Heavy (Z>50) Galactic Cosmic Ray Nuclei Abundance on the Base of the Track Parameters Measuring in the Pallasite Olivine Crystals

Details Super Heavy (Z>50) Galactic Cosmic Ray Nuclei Abundance on the Base of the Track Parameters Measuring in the Pallasite Olivine Crystals Super Heavy (Z>50) Galactic Cosmic Ray Nuclei Abundance on the Base of the Track Parameters Measuring in the Pallasite Olivine Crystals

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1407a&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

Scientific paper

New results of the super-heavy cosmic ray nuclei abundance due to the
track in the pallasite olivine in the frame of OLIMPIA project are
presented. It was detected near 850 tracks with Z>50 and four
corresponding Th-U group.

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