Abstract:A new method for investigation of the ultra-heavy component of Galactic cosmic-ray nuclei (Z = 50-92) has been developed since 1980. It depends on the ability of extraterrestrial silicate crystals (olivine) to register and store during many million years the tracks due to cosmic-ray nuclei with Z~22. Our approach .bases on the partial annealing of both "fossil" tracks and the tracks due to accelerated Kr, Xe, Au, Pb and U ions, and on the chemical etching of total volume track length of the cosmic-ray nuclei i… Show more
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