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Results from Tunka-133 (5 years observation) and from the Tunka-HiSCORE prototype

2016; EDP Sciences; Volume: 121; Linguagem: Inglês

10.1051/epjconf/201612103004

2101-6275

В. В. Просин, S.F. Berezhnev, Н. Буднев, Martin Brückner, A. Chiavassa, O.A. Chvalaev, A.V. Dyachok, S. Epimakhov, A. Gafarov, О. Гресс, Т. И. Гресс, D. Horns, Н. Н. Калмыков, N. Karpov, S. Kiryuhin, E. Konstantinov, А. В. Коробченко, Е. Е. Коростелева, В. А. Кожин, М. Куннас, L. Kuzmichev, Б. К. Лубсандоржиев, Н. Лубсандоржиев, Р. Р. Миргазов, Р. Д. Монхоев, R. Nachtigall, E. Osipova, А. Пахоруков, M. I. Panasyuk, L. Pankov, V. Poleschuk, E.G. Popova, А. Порелли, В. С. Птускин, Г. Рубцов, Michael Rüger, В. Самолига, Yu. Semeney, А. А. Силаев, А. А. Силаев, А. В. Скурихин, C. Spiering, Л. Г. Свешникова, M. Tluczykont, R. Wischnewski, А. Загородников, A.V. Zurbanov,

Particle Detector Development and Performance

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.