Research output: Contribution to journal › Article › peer-review
Energy Spectrum of Primary Cosmic Rays According to the Data of the TAIGA Astrophysical Complex. / the TAIGA Collaboration ; Вайдянатан, Арун .
In: Bulletin of the Russian Academy of Sciences: Physics, Vol. 87, No. 7, 07.2023, p. 1043-1045.Research output: Contribution to journal › Article › peer-review
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TY - JOUR
T1 - Energy Spectrum of Primary Cosmic Rays According to the Data of the TAIGA Astrophysical Complex
AU - the TAIGA Collaboration
AU - Prosin, V. V.
AU - Astapov, I. I.
AU - Bezyazeekov, P. A.
AU - Bonvech, E. A.
AU - Borodin, A. N.
AU - Budnev, N. M.
AU - Bulan, A. V.
AU - Chernov, D. V.
AU - Chiavassa, A.
AU - Dyachok, A. N.
AU - Gafarov, A. R.
AU - Garmash, A. Yu
AU - Grebenyuk, V. M.
AU - Gress, E. O.
AU - Gress, O. A.
AU - Gress, T. I.
AU - Grinyuk, A. A.
AU - Grishin, O. G.
AU - Iliushin, M. A.
AU - Ivanova, A. D.
AU - Ivanova, A. L.
AU - Kalmykov, N. N.
AU - Kindin, V. V.
AU - Kiryuhin, S. N.
AU - Kokoulin, R. P.
AU - Kolosov, N. I.
AU - Kompaniets, K. G.
AU - Korosteleva, E. E.
AU - Kozhin, V. A.
AU - Kravchenko, E. A.
AU - Kryukov, A. P.
AU - Kuzmichev, L. A.
AU - Lagutin, A. A.
AU - Lavrova, M. V.
AU - Lemeshev, Yu E.
AU - Lubsandorzhiev, B. K.
AU - Lubsandorzhiev, N. B.
AU - Malakhov, S. D.
AU - Mirgazov, R. R.
AU - Monkhoev, R. A.
AU - Okuneva, E. A.
AU - Osipova, E. A.
AU - Pakhorukov, A. L.
AU - Pan, A.
AU - Panov, A. D.
AU - Pankov, L. V.
AU - Petrukhin, A. A.
AU - Podgrudkov, D. A.
AU - Rubtsov, G. I.
AU - Sokolov, A. V.
AU - Вайдянатан, Арун
N1 - The work was performed at the UNU “Astrophysical Complex of MSU-ISU” (agreement EB 075-15-2021-675). This work is supported by the Russian Foundation for Basic Research (grant nos. 19-52-44002, 19-32-60003), Russian Science Foundation (grant no. 19-72-20067 (section 2)), the Russian Federation Ministry of Science and High Education (projects FZE-2020-0017, FUZZY-2020-0024, and FSUS-2020-0039). Публикация для корректировки.
PY - 2023/7
Y1 - 2023/7
N2 - 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.
AB - 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.
KW - Cerenkov light flux
KW - extensive air shower
KW - primary particle energy spectrum
UR - https://www.scopus.com/record/display.uri?eid=2-s2.0-85159684079&origin=inward&txGid=aba388ba5c127595bdca99bf0a113b24
UR - https://www.mendeley.com/catalogue/d8ea5fb5-f91a-3be1-926f-9bfb41dcad97/
U2 - 10.3103/S1062873823702362
DO - 10.3103/S1062873823702362
M3 - Article
VL - 87
SP - 1043
EP - 1045
JO - Bulletin of the Russian Academy of Sciences: Physics
JF - Bulletin of the Russian Academy of Sciences: Physics
SN - 1062-8738
IS - 7
ER -
ID: 59589592