Research output: Contribution to journal › Article › peer-review
Research output: Contribution to journal › Article › peer-review
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TY - JOUR
T1 - Depth of the Maximum of Extensive Air Showers (EASes) and the Mean Mass Composition of Primary Cosmic Rays in the 1015–1018 eV Range of Energies, According to Data from the TUNKA-133 and TAIGA-HiSCORE Arrays for Detecting EAS Cherenkov Light in the Tunkinsk Valley
AU - the TAIGA Collaboration
AU - Prosin, V. V.
AU - Astapov, I. I.
AU - Bezyazeekov, P. A.
AU - Borodin, A. N.
AU - Brückner, M.
AU - Budnev, N. M.
AU - Bulan, A.
AU - Vaidyanathan, A.
AU - Wischnewski, R.
AU - Volchugov, P.
AU - Voronin, D.
AU - Gafarov, A. R.
AU - Garmash, A. Yu
AU - Grebenyuk, V. M.
AU - Gress, O. A.
AU - Gress, T. I.
AU - Grinyuk, A. A.
AU - Grishin, O. G.
AU - Dyachok, A. N.
AU - Zhurov, D. P.
AU - Zagorodnikov, A. V.
AU - Ivanova, A. L.
AU - Kalmykov, N. N.
AU - Kindin, V. V.
AU - Kiryuhin, S. N.
AU - Kozhin, V. A.
AU - Kokoulin, R. P.
AU - Kompaniets, K. G.
AU - Korosteleva, E. E.
AU - Kravchenko, E. A.
AU - Kryukov, A. P.
AU - Kuzmichev, L. A.
AU - Chiavassa, A.
AU - Lavrova, M.
AU - Lagutin, A. A.
AU - Lemeshev, Yu
AU - Lubsandorzhiev, B. K.
AU - Lubsandorzhiev, N. B.
AU - Mirgazov, R. R.
AU - Mirzoyan, R.
AU - Monkhoev, R. D.
AU - Osipova, E. A.
AU - Pan, A.
AU - Panasyuk, M. I.
AU - Pankov, L. V.
AU - Pakhorukov, A. L.
AU - Petrukhin, A. A.
AU - Poleschuk, V. A.
AU - Popesku, M.
AU - Sokolov, A. V.
N1 - Funding Information: This work was supported by the RF Ministry of Education and Science as part of State Task no. FZZE-2020-0024, agreement no. 075-15-2019-1631; and by the Russian Science Foundation, project no. 19-72-20067, section 2. Publisher Copyright: © 2021, Allerton Press, Inc. Copyright: Copyright 2021 Elsevier B.V., All rights reserved.
PY - 2021/4
Y1 - 2021/4
N2 - A corrected energy dependence of the depth of the maximum in the wide range of energies 1015 to 1018 eV is obtained using data collected at the Tunka-133 facility over 7 years of operation (2009–2017) and the TAIGA-HiSCORE facility in the 2019–2020 season. At the highest energies, our results match those of the Pierre Auger observatory. The results are converted to parameter ❬ln A❭, which characterizes the mean EAS composition.
AB - A corrected energy dependence of the depth of the maximum in the wide range of energies 1015 to 1018 eV is obtained using data collected at the Tunka-133 facility over 7 years of operation (2009–2017) and the TAIGA-HiSCORE facility in the 2019–2020 season. At the highest energies, our results match those of the Pierre Auger observatory. The results are converted to parameter ❬ln A❭, which characterizes the mean EAS composition.
UR - http://www.scopus.com/inward/record.url?scp=85106263802&partnerID=8YFLogxK
UR - https://www.elibrary.ru/item.asp?id=46082271
U2 - 10.3103/S1062873821040298
DO - 10.3103/S1062873821040298
M3 - Article
AN - SCOPUS:85106263802
VL - 85
SP - 395
EP - 397
JO - Bulletin of the Russian Academy of Sciences: Physics
JF - Bulletin of the Russian Academy of Sciences: Physics
SN - 1062-8738
IS - 4
ER -
ID: 28861310