Physics
Scientist
Moskovskii Gosudarstvennyi Universitet, Moscow, USSR
Characteristics of backscattered particles generated by high-energy primary cosmic-ray nuclei in absorbing matter
Energy spectrum of primary cosmic-ray particles at 1 - 100 TeV from data from the Sokol package.
Primary cosmic ray nuclei with 6 ≤ Z ≤ 30 in the energy range 1012 - 1014eV from Kosmos-1543 and Kosmos-1713 experimental data.
Registration of nuclear interactions of particles of high-energy primary cosmic rays with the method of a controlled emulsion pile.
Some characteristics of nucleus-nucleus interactions at energies on the order of 1 TeV
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