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Tunka-133: Results of 3 year operation

V V Prosin,S F Berezhnev,N M Budnev,A Chiavassa,O A Chvalaev,O Gress,A N Dyachok,S N Epimakhov,N I Karpov,N N Kalmykov,E Konstantinov,A V Korobchenko,E E Korosteleva,V A Kozhin,L A Kuzmichev,B K Lubsandorzhiev,N B Lubsandorzhiev,R R Mirgazov,M I Panasyuk,L V Pankov,E Popova,V S Ptuskin,Yu A Semeney,A A Silaev,A V Skurikhin,C Spiering,L G Sveshnikova,I V Yashin,A V Zagorodnikov

Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment（2014）

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摘要
The EAS Cherenkov light array Tunka-133, with ~3km2 geometric area, is taking data since 2009. The array permits a detailed study of cosmic ray energy spectrum and mass composition in the PeV energy range. After a short description of the methods of EAS parameter reconstruction, we present the all-particle energy spectrum and results of studying CR composition, based on 3 seasons of array operation. In the last part of the paper, we discuss possible interpretations of the obtained results.
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关键词
Tunka-133,Spectrum,Composition,Cherenkov light
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