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Analysis of cosmic rays with Z > 50 registered in meteorite minerals

Bajram Jakupi ; Faculty of Science, University of Priština, 38000 Priština, Yugoslavia
Mustafa Bytyci ; Faculty of Science, University of Priština, 38000 Priština, Yugoslavia
Vladimir P. Perelygin ; Joint Institute for Nuclear Research, Dubna, USSR
Stanislav G. Stetsenko ; Joint Institute for Nuclear Research, Dubna, USSR
Radovan Antanasijević ; Institute of Physics, 11001 Beograd, P. 0. Box 57, Yugoslavia
Živojin Todorović ; Institute of Physics, 11001 Beograd, P. 0. Box 57, Yugoslavia
Ana B. Akopova ; Institute of Physics, Yerevan, USSR
Larisa Y. Melkumyan ; Institute of Physics, Yerevan, USSR

Sažetak

Cosmic rays with Z > 50 captured in olivine meteorite crystal (Marjalahti) is analyzed. The length distribution of such cosmic ray traces (R > 100 µm) at 6 and 9 cm from the meteorite surface is determined. Utilizing the dependency curve between trace length and charge, the relative contribution of nuclei with Z > 50 is ascertained and compared with similar experimental results from the literature. We estimate the energy spectrum decay index of cosmic rays for nuclei from 50 < Z < 70, 70 < Z < 90 and Z > 90.

Ključne riječi

Hrčak ID:

329223

URI

https://hrcak.srce.hr/329223

Datum izdavanja:

3.12.1984.

Podaci na drugim jezicima: hrvatski

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