Journal
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT
Volume 756, Issue -, Pages 94-101Publisher
ELSEVIER SCIENCE BV
DOI: 10.1016/j.nima.2013.09.018
Keywords
Tunka-133; Spectrum; Composition; Cherenkov light
Categories
Funding
- Russian Federation Ministry of Education and Science [G/C 14.518.11.7046, 14.B25.31.0010, 14.14.B37.21.0785, 14.B37.21.1294]
- Russian Foundation for Basic Research [11-02-00409, 13-02-00214, 13-02-12095, 13-02-10001]
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The EAS Cherenkov light array Tunka-133, with similar to 3 km(2) 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. (C) 2013 Published by Elsevier B.V.
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