Physics
Scientist
Moskovskij Gosudarstvennyj Univ., Moscow, Russia
Altitude Variation of EAS and Particle Lateral Distribution Function in the Upper Atmosphere
Characteristics of backscattered particles generated by high-energy primary cosmic-ray nuclei in absorbing matter
Energy spectra of different cosmic-ray components at energies higher than 2 TeV measured by the SOKOL facility
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.
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