1. Results from Tunka-133 (5 years observation) and from the Tunka-HiSCORE prototype
- Author
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Yu. A. Semeney, A. Pakhorukov, A. V. Skurikhin, V. A. Poleschuk, R. Nachtigall, O. A. Gress, A. V. Gafarov, M. Kunnas, A.V. Zurbanov, A. Porelli, S. Kiryuhin, Dieter Horns, V. A. Kozhin, C. Spiering, Bayarto Lubsandorzhiev, M. Tluczykont, M. I. Panasyuk, M. Rüger, A.V. Dyachok, L. G. Sveshnikova, A. Chiavassa, V. Prosin, S. F. Berezhnev, A.V. Korobchenko, S. Epimakhov, V. S. Ptuskin, E. E. Korosteleva, L. V. Pankov, R. D. Monkhoev, T. I. Gress, Aleksey Zagorodnikov, N. B. Lubsandorzhiev, N. I. Karpov, Grigory Rubtsov, N. N. Kalmykov, N. M. Budnev, L. A. Kuzmichev, A. A. Silaev, R. Wischnewski, E. N. Konstantinov, E.G. Popova, R. R. Mirgazov, V. Samoliga, O.A. Chvalaev, M. Brückner, and E. A. Osipova
- Subjects
Physics ,010308 nuclear & particles physics ,Maximum depth ,QC1-999 ,0103 physical sciences ,Energy spectrum ,Cosmic ray ,Astrophysics ,010306 general physics ,01 natural sciences ,Cherenkov radiation ,Remote sensing - Abstract
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 · 10 15 −10 18 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.
- Published
- 2016
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