Standard

Spectrum and Composition of Primary Cosmic Rays, According to Data from the TAIGA-HiSCORE Array. / the TAIGA Collaboration.

In: Bulletin of the Russian Academy of Sciences: Physics, Vol. 89, No. 6, 15.07.2025, p. 907-912.

Research output: Contribution to journal › Article › peer-review

Harvard

the TAIGA Collaboration 2025, 'Spectrum and Composition of Primary Cosmic Rays, According to Data from the TAIGA-HiSCORE Array', Bulletin of the Russian Academy of Sciences: Physics, vol. 89, no. 6, pp. 907-912. https://doi.org/10.1134/S1062873825711663

APA

the TAIGA Collaboration (2025). Spectrum and Composition of Primary Cosmic Rays, According to Data from the TAIGA-HiSCORE Array. Bulletin of the Russian Academy of Sciences: Physics, 89(6), 907-912. https://doi.org/10.1134/S1062873825711663

Vancouver

the TAIGA Collaboration. Spectrum and Composition of Primary Cosmic Rays, According to Data from the TAIGA-HiSCORE Array. Bulletin of the Russian Academy of Sciences: Physics. 2025 Jul 15;89(6):907-912. doi: 10.1134/S1062873825711663

Author

the TAIGA Collaboration. / Spectrum and Composition of Primary Cosmic Rays, According to Data from the TAIGA-HiSCORE Array. In: Bulletin of the Russian Academy of Sciences: Physics. 2025 ; Vol. 89, No. 6. pp. 907-912.

BibTeX

@article{a912c2833cf6417da7da3c72951d141e,
title = "Spectrum and Composition of Primary Cosmic Rays, According to Data from the TAIGA-HiSCORE Array",
abstract = "Abstract: Results are presented from operating the TAIGA-HiSCORE array after raising the number of stations to 114 and directing all stations to the zenith. The conversion from the measured Cherenkov light flux of an extensive air shower (EAS) to the primary energy of cosmic particles is refined. Parameter 〈lnA〉, recalculated from the maximum depth characterizing the average composition of primary cosmic radiation, is compared to results obtained at our Tunka-133 installation and others from the LHAASO and AUGER experiments.",
keywords = "energy spectrum, extensive air showers, mass composition",
author = "{TAIGA Collaboration} and Prosin, {V. V.} and Astapov, {I. I.} and Bezyazeekov, {P. A.} and Blinov, {A. V.} and Borodin, {A. N.} and Bonvech, {E. A.} and Budnev, {N. M.} and Bulan, {A. V.} and Volkov, {N. V.} and Volchugov, {P. A.} and Voronin, {D. M.} and Gafarov, {A. R.} and Gress, {E. O.} and Gress, {O. A.} and Gress, {T. I.} and Grinyuk, {A. A.} and Grishin, {O. G.} and Garmash, {A. Yu} and Grebenyuk, {V. M.} and Dyachok, {A. N.} and Zhurov, {D. P.} and Zagorodnikov, {A. V.} and Zirakashvili, {V. N.} and Ivanova, {A. D.} and Ivanova, {A. L.} and Iliushin, {M. A.} 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 A. Chiavassa and Lavrova, {M. V.} and Monkhoev, {R. D.} and Osipova, {E. A.} and Panov, {A. D.} and Popova, {E. G.} and Rubtsov, {G. I.} and Ryabov, {E. V.} and Samoliga, {V. S.} and Skurikhin, {A. V.} and Sokolov, {A. V.} and Ushakov, {N. A.} and Chernov, {D. V.}",
note = "This work was performed at the MSU-ISU Astrophysical Complex. It was supported by the Russian Science Foundation (project no. 23-72-00016: Sections “Restoring EAS Parameters,” “Depth of an EAS Maximum,” and “Average Mass Composition” and project no. 3-72-00019: Section “Experimental Energy Spectrum”), and State Tasks FZZE-2023-0004 and FZZE-2024-0005 from the Ministry of Science and Higher Education of the Russian Federation.",
year = "2025",
month = jul,
day = "15",
doi = "10.1134/S1062873825711663",
language = "русский",
volume = "89",
pages = "907--912",
journal = "Bulletin of the Russian Academy of Sciences: Physics",
issn = "1062-8738",
publisher = "Pleiades Publishing",
number = "6",

}

RIS

TY - JOUR

T1 - Spectrum and Composition of Primary Cosmic Rays, According to Data from the TAIGA-HiSCORE Array

AU - TAIGA Collaboration

AU - Prosin, V. V.

AU - Astapov, I. I.

AU - Bezyazeekov, P. A.

AU - Blinov, A. V.

AU - Borodin, A. N.

AU - Bonvech, E. A.

AU - Budnev, N. M.

AU - Bulan, A. V.

AU - Volkov, N. V.

AU - Volchugov, P. A.

AU - Voronin, D. M.

AU - Gafarov, A. R.

AU - Gress, E. O.

AU - Gress, O. A.

AU - Gress, T. I.

AU - Grinyuk, A. A.

AU - Grishin, O. G.

AU - Garmash, A. Yu

AU - Grebenyuk, V. M.

AU - Dyachok, A. N.

AU - Zhurov, D. P.

AU - Zagorodnikov, A. V.

AU - Zirakashvili, V. N.

AU - Ivanova, A. D.

AU - Ivanova, A. L.

AU - Iliushin, M. A.

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 - Chiavassa, A.

AU - Lavrova, M. V.

AU - Monkhoev, R. D.

AU - Osipova, E. A.

AU - Panov, A. D.

AU - Popova, E. G.

AU - Rubtsov, G. I.

AU - Ryabov, E. V.

AU - Samoliga, V. S.

AU - Skurikhin, A. V.

AU - Sokolov, A. V.

AU - Ushakov, N. A.

AU - Chernov, D. V.

N1 - This work was performed at the MSU-ISU Astrophysical Complex. It was supported by the Russian Science Foundation (project no. 23-72-00016: Sections “Restoring EAS Parameters,” “Depth of an EAS Maximum,” and “Average Mass Composition” and project no. 3-72-00019: Section “Experimental Energy Spectrum”), and State Tasks FZZE-2023-0004 and FZZE-2024-0005 from the Ministry of Science and Higher Education of the Russian Federation.

PY - 2025/7/15

Y1 - 2025/7/15

N2 - Abstract: Results are presented from operating the TAIGA-HiSCORE array after raising the number of stations to 114 and directing all stations to the zenith. The conversion from the measured Cherenkov light flux of an extensive air shower (EAS) to the primary energy of cosmic particles is refined. Parameter 〈lnA〉, recalculated from the maximum depth characterizing the average composition of primary cosmic radiation, is compared to results obtained at our Tunka-133 installation and others from the LHAASO and AUGER experiments.

AB - Abstract: Results are presented from operating the TAIGA-HiSCORE array after raising the number of stations to 114 and directing all stations to the zenith. The conversion from the measured Cherenkov light flux of an extensive air shower (EAS) to the primary energy of cosmic particles is refined. Parameter 〈lnA〉, recalculated from the maximum depth characterizing the average composition of primary cosmic radiation, is compared to results obtained at our Tunka-133 installation and others from the LHAASO and AUGER experiments.

KW - energy spectrum

KW - extensive air showers

KW - mass composition

UR - https://www.mendeley.com/catalogue/31dbd76a-8ef5-3db2-924f-574a0a5ce48b/

UR - https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=105010730044&origin=inward

U2 - 10.1134/S1062873825711663

DO - 10.1134/S1062873825711663

M3 - статья

VL - 89

SP - 907

EP - 912

JO - Bulletin of the Russian Academy of Sciences: Physics

JF - Bulletin of the Russian Academy of Sciences: Physics

SN - 1062-8738

IS - 6

ER -

ID: 68545869