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The Tunka – Multi-component EAS detector for high energy cosmic ray studies

S F Berezhnev,D Besson,Nikolay M Budnev,M Buker,M Brueckner,A Chiavassa,O A Chvalaev,O Gress,A N Dyachok,S N Epimakhov,D Hampf,A Haungs,Roger G Hiller,D Horns,Ana Ivanova,N I Karpov,N N Kalmykov,Y Kazarina,E Konstantinov,D Kostunin,A V Korobchenko,E E Korosteleva,V A Kozhin,M Kunnas,L A Kuzmichev,B K Lubsandorzhiev,N B Lubsandorzhiev,R R Mirgazov, R Monhoev,R Nachtigall,M I Panasyuk,L V Pankov,A Pankov, A Pokhorukov,E G Popova,A Porelli,V V Prosin,V S Ptuskin,G Rowell,F G Schroder,Yu A Semeney,B A Shaibonov,A A Silaev,A V Skurikhin,C Spiering,D Spitschan,L G Sveshnikova,R Wischnewski,I V Yashin,A V Zagorodnikov

Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment（2013）

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Abstract
The EAS Cherenkov array Tunka-133, with about 3km2 sensitive area, has been installed in the Tunka Valley, Siberia. The accessible energy range is 1015–1018eV. In this contribution, a description of the array and main results obtained so far are presented. A current update of the array includes the deployment of scintillation stations, radio antennas, as well as optical stations. The deployments of these optical stations are the first step towards Tunka-HiSCORE, a wide-angle, large field-of-view gamma-ray telescope.
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Cosmic rays,Tunka-133,Tunka-HiSCORE
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