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Prosin, V.V.; Berezhnev, S.F.; Budnev, N.M.; Brückner, M.; Chiavassa, A.; Chvalaev, O.A.; Dyachok, A.V.; Epimakhov, S.N.; Gafarov, A.V.; Gress, O.A.; Gress, T.I.; Horns, D.; Kalmykov, N.N.; Karpov, N.I.; Kiryuhin, S.N.; Konstantinov, E.N.; Korobchenko, A.V.; Korosteleva, E.E.; Kozhin, V.A.; Kunnas, M.; Kuzmichev, L.A.; Lubsandorzhiev, B.K.; Lubsandorzhiev, N.B.; Mirgazov, R.R.; Monkhoev, R.D.; Nachtigall, R.; Osipova, E.A.; Pakhorukov, A.L.; Panasyuk, M.I.; Pankov, L.V.; Poleschuk, V.A.; Popova, E.G.; Porelli, A.; Ptuskin, V.S.; Rubtsov, G.I.; Rüger, M.; Samoliga, V.S.; Semeney, Y.A.; Silaev, A.A.; Silaev, A.A.; Skurikhin, A.V.; Spiering, C.; Sveshnikova, L.G.; Tluczykont, M.; Wischnewski, R.; Zagorodnikov, A.V.; Zurbanov, A.V.
EPJ Web of conferences, 01/2016, Letnik: 121Journal Article
Data obtained with two detectors located at the Tunka Cosmic Ray facility are presented. The Cherenkov light array for registration of extensive air showers (EAS) Tunka-133 collected data during 5 winter seasons since 2009 to 2014. The differential energy spectrum of all particles and the dependence of the average maximum depth on the energy in the range of 6 · 1015−1018 eV measured for 1540 hours of observation are presented. The preliminary all particle energy spectrum by the data of Tunka-HiSCORE prototype array, installed in 2013, is presented. Some additional experiments in the Tunka Valley are briefly described.
