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Energy Spectrum of Primary Cosmic Rays According to the Data of the TAIGA Astrophysical Complex. / TAIGA Collaboration ; Вайдянатан, Арун .

в: Bulletin of the Russian Academy of Sciences: Physics, Том 87, № 7, 07.2023, стр. 1043-1045.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

Harvard

TAIGA Collaboration & Вайдянатан, А 2023, 'Energy Spectrum of Primary Cosmic Rays According to the Data of the TAIGA Astrophysical Complex', Bulletin of the Russian Academy of Sciences: Physics, Том. 87, № 7, стр. 1043-1045. https://doi.org/10.3103/S1062873823702362

APA

Vancouver

TAIGA Collaboration, Вайдянатан А. Energy Spectrum of Primary Cosmic Rays According to the Data of the TAIGA Astrophysical Complex. Bulletin of the Russian Academy of Sciences: Physics. 2023 июль;87(7):1043-1045. doi: 10.3103/S1062873823702362

Author

TAIGA Collaboration ; Вайдянатан, Арун . / Energy Spectrum of Primary Cosmic Rays According to the Data of the TAIGA Astrophysical Complex. в: Bulletin of the Russian Academy of Sciences: Physics. 2023 ; Том 87, № 7. стр. 1043-1045.

BibTeX

@article{026949d4b8c84041aedfd5097bb38abf,
title = "Energy Spectrum of Primary Cosmic Rays According to the Data of the TAIGA Astrophysical Complex",
abstract = "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.",
keywords = "Cerenkov light flux, extensive air shower, primary particle energy spectrum",
author = "{the TAIGA Collaboration} and Prosin, {V. V.} and Astapov, {I. I.} and Bezyazeekov, {P. A.} and Bonvech, {E. A.} and Borodin, {A. N.} and Budnev, {N. M.} and Bulan, {A. V.} and Chernov, {D. V.} and A. Chiavassa and Dyachok, {A. N.} and Gafarov, {A. R.} and Garmash, {A. Yu} and Grebenyuk, {V. M.} and Gress, {E. O.} and Gress, {O. A.} and Gress, {T. I.} and Grinyuk, {A. A.} and Grishin, {O. G.} and Iliushin, {M. A.} and Ivanova, {A. D.} and Ivanova, {A. L.} and Kalmykov, {N. N.} and Kindin, {V. V.} and Kiryuhin, {S. N.} and Kokoulin, {R. P.} and Kolosov, {N. I.} and Kompaniets, {K. G.} and Korosteleva, {E. E.} and Kozhin, {V. A.} and Kravchenko, {E. A.} and Kryukov, {A. P.} and Kuzmichev, {L. A.} and Lagutin, {A. A.} and Lavrova, {M. V.} and Lemeshev, {Yu E.} and Lubsandorzhiev, {B. K.} and Lubsandorzhiev, {N. B.} and Malakhov, {S. D.} and Mirgazov, {R. R.} and Monkhoev, {R. A.} and Okuneva, {E. A.} and Osipova, {E. A.} and Pakhorukov, {A. L.} and A. Pan and Panov, {A. D.} and Pankov, {L. V.} and Petrukhin, {A. A.} and Podgrudkov, {D. A.} and Rubtsov, {G. I.} and Sokolov, {A. V.} and Арун Вайдянатан",
note = "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.",
year = "2023",
month = jul,
doi = "10.3103/S1062873823702362",
language = "English",
volume = "87",
pages = "1043--1045",
journal = "Bulletin of the Russian Academy of Sciences: Physics",
issn = "1062-8738",
publisher = "PLEIADES PUBLISHING INC",
number = "7",

}

RIS

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