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Simulation of Tunka-Grande and TAIGA-Muon scintillation facilities
Russian version
M. Ternovoy1, I. Astapov2, P. Bezyazeekov1, E. Bonvech3, A. Borodin4, N. Budnev1, A. Bulan3, N. Volkov5, P. Volchugov3, D. Voronin6, A. Gafarov1, E. Gress1, О. Gress1, T. Gress1, O. Grishin1, A. Garmash7,8, V. Grebenyuk4,9, A. Grinyuk4, A. Dyachok1, D. Zhurov1,10, A. Zagorodnikov1, A. D. Ivanova1,11, A. L. Ivanova1,7, M.A. Iliushin1, N. Kalmykov3, V. Kindin2, S. Kiryuhin1, R. Kokoulin2, N. Kolosov1, K. Kompaniets2, E. Korosteleva3, V. Kozhin3, E. Kravchenko7,8, A. Kryukov3, L. Kuzmichev3, A. Lagutin5, M. Lavrova4, Y. Lemeshev1, B. Lubsandorzhiev6, N. Lubsandorzhiev3, S. Malakhov1, R. Mirgazov1, R. Monkhoev1, E. Okuneva3, E. Osipova3, A. Pakhorukov1, A. Pan4, A. Panov3, L. Pankov1, A. Petrukhin2, D. Podgrudkov3, E. Popova3, E. Postnikov3, V. Prosin3, V. Ptuskin12, A. Pushnin1, A. Razumov3, R. Raikin5, G. Rubtsov6, E. Ryabov1, V. Samoliga1, I. Satyshev4, A. Silaev3, A. Silaev (junior) 3, A. Sidorenkov6, A. Skurikhin3, A. Sokolov7,8, L. Sveshnikova3, V. Tabolenko1, A. Tanaev1, L. Tkachev4,9, N. Ushakov6, D. Chernov3, I. Yashin2, Chiavassa A.13, Vaidyanathan A.7
1Research Institute of Applied Physics, Irkutsk State University, Irkutsk, Russia
2National Research Nuclear University “MEPhI”, Moscow, Russia
3Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics, Moscow, Russia
4Joint Institute for Nuclear Research, Dubna, Russia
5Altai State University, Barnaul, Russia
6 Institute for Nuclear Research of Russian Academy of Sciences, Moscow, Russian
7Novosibirsk State University, Novosibirsk, Russia
8Budker Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences, Novosibirsk, Russia
9Dubna State University, Dubna, Russia
10Irkutsk National Research Technical University, Irkutsk, Russia
11Moscow Institute of Physics and Technology (National Research University), Dolgoprudny, Moscow Region, Russia
12Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of the Russian Academy of Sciences, Moscow, Russia
13National Institute for Nuclear Physics, Torino, Italy
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A planning for computer generated simulation of scintillation equipment based on the CORSIKA and Geant4 software packages is presented. Method developed to optimize the simulation process is presented. A possible approach for determining the mass composition of charged cosmic rays is discussed. Preliminary results of computer generated of the Tunka-Grande installation in the energy range 10-100 PeV are also presented. Keywords: experimental complex TAIGA, cosmic rays, wide atmospheric showers, mass composition, CORSIKA, Geant4.
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