Super Heavy (Z>50) Galactic Cosmic Ray Nuclei Abundance on the Base of the Track Parameters Measuring in the Pallasite Olivine Crystals
Abstract
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.
- Publication:
-
40th Annual Lunar and Planetary Science Conference
- Pub Date:
- March 2009
- Bibcode:
- 2009LPI....40.1407A