Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Junior
Skobeltsyn Institute of Nuclear Physics, Moscow State University
SINP MSU, Moscow
junior
Moskovskii Gosudarstvennyi Universitet, Moscow, USSR
Moscow State University, D.V. Skobeltsyn Institute of Nuclear Physics, 119899 Moscow, Russia
D.V. Skobeltsyn Institute of Nuclear Physics, Moscow State University, 119899 Moscow, Russia
Institute of Nuclear Physics, Moscow State University, Moscow 119 899, Russia
Institut Teoreticheskoi i Eksperimental'noi Fiziki, Moscow, USSR
Samarkandskii Gosudarstvennyi Universitet, Samarkand, Uzbek SSR; Moskovskii Gosudarstvennyi Universitet, Moscow, USSR
Altaiskii Gosudarstvennyi Universitet, Barnaul, USSR
Inst. of Nucl. Phys., Moscow State University, Russia
Moskovskij Gosudarstvennyj Univ., Moscow, Russia
MGU, Moscow; RAN, Inst. Kosmofizicheskikh Issledovanij i Aeronomii, Yakutsk, Russia; ANK, Inst. Fiziki Vysokikh Ehnergij; Kazakhskij Univ., Alma-Ata, Kazakhstan; NPO Monokristallreaktiv, Ukraine; Turku Univ., Finland; Lodz Univ., Poland
Institute of Nuclear Physics Moscow State University, Moscow 119899, Russia
Moskovskii Gosudarstvennyi Universitet, Moscow, USSR; Uzbekskii Gosudarstvennyi Universitet, Samarkand, Uzbek SSR
Moskovskii Gosudarstvennyi Universitet, Moscow; Akademiia Nauk SSSR, Institut Kosmofizicheskikh Issledovanii i Aeronomii, Yakutsk, USSR
Institute of Nuclear Physics of Moscow State University, Moscow 119899, Russia
Institute of Nuclear Physics, Moscow State University, Moscow, Russia, 119899
Moskovskii Gosudarstvennyi Universitet, Moscow, USSR; Lodz, Uniwersytet, Lodz, Poland
Scobeltsyn Institut of Nuclear Physics of MSU, Moscow, Russia
Analysis of the muon component in extensive air showers
Analysis of the spatial distribution of Cerenkov emission from extensive air showers obtained at the Samarkand University installation
Breakdown of scaling and means of modifying the elementary-event model to ultrahigh energies
Calculation of EAS characteristics in the theory of a supercritical pomeron with allowance for an additive quark model
Characteristics of Low-Energy Hadrons and Muons of 1015 - 3 x 1019 eV EAS at Different Atmosphere Levels
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