학술논문
Energy Spectrum of Primary Cosmic Rays According to the Data of the TAIGA Astrophysical Complex
Document Type
Original Paper
Author
Prosin, V. V.; Astapov, I. I.; Bezyazeekov, P. A.; Bonvech, E. A.; Borodin, A. N.; Budnev, N. M.; Bulan, A. V.; Chernov, D. V.; Chiavassa, A.; Dyachok, A. N.; Gafarov, A. R.; Garmash, A. Yu.; Grebenyuk, V. M.; Gress, E. O.; Gress, O. A.; Gress, T. I.; Grinyuk, A. A.; Grishin, O. G.; Iliushin, M. A.; Ivanova, A. D.; Ivanova, A. L.; Kalmykov, N. N.; Kindin, V. V.; Kiryuhin, S. N.; Kokoulin, R. P.; Kolosov, N. I.; Kompaniets, K. G.; Korosteleva, E. E.; Kozhin, V. A.; Kravchenko, E. A.; Kryukov, A. P.; Kuzmichev, L. A.; Lagutin, A. A.; Lavrova, M. V.; Lemeshev, Yu. E.; Lubsandorzhiev, B. K.; Lubsandorzhiev, N. B.; Malakhov, S. D.; Mirgazov, R. R.; Monkhoev, R. A.; Okuneva, E. A.; Osipova, E. A.; Pakhorukov, A. L.; Pan, A.; Panov, A. D.; Pankov, L. V.; Petrukhin, A. A.; Podgrudkov, D. A.; Popova, E. G.; Postnikov, E. B.; Ptuskin, V. S.; Pushnin, A. A.; Raikin, R. I.; Razumov, A. V.; Rjabov, E. V.; Rubtsov, G. I.; Samoliga, V. S.; Satyshev, I.; Sidorenkov, A. Yu.; Silaev, A. A.; Silaev, Jr., A. A.; Skurikhin, A. V.; Sokolov, A. V.; Sveshnikova, L. G.; Tabolenko, V. A.; Tanaev, A. B.; Tarashansky, B. A.; Ternovoy, M. Yu.; Tkachev, L. G.; Ushakov, N. A.; Vaidyanathan, A.; Volkov, N. V.; Volchugov, P. A.; Voronin, D. M.; Yashin, I. I.; Zagorodnikov, A. V.; Zhurov, D. P.
Source
Bulletin of the Russian Academy of Sciences: Physics. 87(7):1043-1045
Subject
Language
English
ISSN
1062-8738
1934-9432
1934-9432
Abstract
The more correct recalculation from the measured Cherenkov light fluxes at distances of 200 (Q200) and 100 (Q100) m from the Extensive Air Shower (EAS) core to the energy of the primary particle has been developed using the results of M-C simulation by the CORSIKA code, assuming a light primary composition of cosmic rays. Using the new conversion expressions, a differential energy spectrum was obtained according to the data of the Tunka-133 array for 7 years of operation and the TAIGA-HiSCORE array for 2 years of operation.