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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

Harvard

the 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, vol. 87, no. 7, pp. 1043-1045. https://doi.org/10.3103/S1062873823702362

APA

the 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, 87(7), 1043-1045. https://doi.org/10.3103/S1062873823702362

Vancouver

the 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 Jul;87(7):1043-1045. doi: 10.3103/S1062873823702362

Author

the TAIGA Collaboration ; Вайдянатан, Арун . / Energy Spectrum of Primary Cosmic Rays According to the Data of the TAIGA Astrophysical Complex. In: Bulletin of the Russian Academy of Sciences: Physics. 2023 ; Vol. 87, No. 7. pp. 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 A. Chiavassa and Garmash, {A. Yu} and Ivanova, {A. L.} and Kravchenko, {E. A.} and Monkhoev, {R. 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",
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 - Chiavassa, A.

AU - Garmash, A. Yu

AU - Ivanova, A. L.

AU - Kravchenko, E. A.

AU - Monkhoev, R. 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