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Estimation of the Light Component Spectrum of Cosmic Rays in the Energy Range of 200–10 000 TeV by the Hybrid Method. / the TAIGA Collaboration.

In: Bulletin of the Russian Academy of Sciences: Physics, Vol. 89, No. 6, 15.07.2025, p. 899-903.

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

Harvard

the TAIGA Collaboration 2025, 'Estimation of the Light Component Spectrum of Cosmic Rays in the Energy Range of 200–10 000 TeV by the Hybrid Method', Bulletin of the Russian Academy of Sciences: Physics, vol. 89, no. 6, pp. 899-903. https://doi.org/10.1134/S1062873825711638

APA

the TAIGA Collaboration (2025). Estimation of the Light Component Spectrum of Cosmic Rays in the Energy Range of 200–10 000 TeV by the Hybrid Method. Bulletin of the Russian Academy of Sciences: Physics, 89(6), 899-903. https://doi.org/10.1134/S1062873825711638

Vancouver

the TAIGA Collaboration. Estimation of the Light Component Spectrum of Cosmic Rays in the Energy Range of 200–10 000 TeV by the Hybrid Method. Bulletin of the Russian Academy of Sciences: Physics. 2025 Jul 15;89(6):899-903. doi: 10.1134/S1062873825711638

Author

the TAIGA Collaboration. / Estimation of the Light Component Spectrum of Cosmic Rays in the Energy Range of 200–10 000 TeV by the Hybrid Method. In: Bulletin of the Russian Academy of Sciences: Physics. 2025 ; Vol. 89, No. 6. pp. 899-903.

BibTeX

@article{b1accaa83bf640d291ee83e11305dc77,
title = "Estimation of the Light Component Spectrum of Cosmic Rays in the Energy Range of 200–10 000 TeV by the Hybrid Method",
abstract = "Abstract: New results on measuring the spectrum of the light component (protons + helium) of cosmic rays in the classical knee region in the primary cosmic ray spectrum at energies of ∼200–20 000 are presented. The results were obtained from hybrid data of the TAIGA experiment in which Cherenkov light of the shower is recorded simultaneously by two (IACT + HiSCORE) facilities. The showers are separated from the light component for the first time using image parameters recorded by the IACT atmospheric image telescope. The developed approach to separation of the light component is based on and confirmed by Monte Carlo calculations. In the obtained spectrum of the light component in the energy range of 200–20 000 TeV, a pronounced knee is observed at an energy of about 3 PeV.",
keywords = "Cherenkov telescope, chemical composition, extensive atmospheric showers, primary cosmic rays",
author = "{TAIGA Collaboration} and Sveshnikova, {L. G.} and Okuneva, {E. A.} 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 Chernov, {D. V.} and A. Chiavassa and Dyachok, {A. N.} and Gafarov, {A. R.} and Garmash, {A. Yu} and Gress, {E. O.} and Gress, {O. A.} and Gress, {T. I.} and Grebenyuk, {V. M.} and Grinyuk, {A. A.} and Grishin, {O. G.} and Ivanova, {A. L.} and Ivanova, {A. D.} and Iliushin, {M. A.} and Kalmykov, {N. N.} and Kindin, {V. V.} and Kiryuhin, {S. N.} and Kokoulin, {R. P.} 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 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 Volkov, {N. V.} and Voronin, {D. M.}",
note = "This work was supported by the Ministry of Science and Higher Education of the Russian Federation (agreement EB-075-15-2021-675, subjects of the state assignment FZZE-2023-0004 and FZZE-2024-0005) and the Russian Science Foundation (project no. 23-72-00019: sections “Procedure of Extracting the Light Component,” “Spectrum of the Light Component,” and “Conclusions”; project no. 23-72-00016: sections “Procedure of Extracting the Light Component” and “Spectrum of the Light Component”).",
year = "2025",
month = jul,
day = "15",
doi = "10.1134/S1062873825711638",
language = "русский",
volume = "89",
pages = "899--903",
journal = "Bulletin of the Russian Academy of Sciences: Physics",
issn = "1062-8738",
publisher = "Pleiades Publishing",
number = "6",

}

RIS

TY - JOUR

T1 - Estimation of the Light Component Spectrum of Cosmic Rays in the Energy Range of 200–10 000 TeV by the Hybrid Method

AU - TAIGA Collaboration

AU - Sveshnikova, L. G.

AU - Okuneva, E. A.

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 - Chernov, D. V.

AU - Chiavassa, A.

AU - Dyachok, A. N.

AU - Gafarov, A. R.

AU - Garmash, A. Yu

AU - Gress, E. O.

AU - Gress, O. A.

AU - Gress, T. I.

AU - Grebenyuk, V. M.

AU - Grinyuk, A. A.

AU - Grishin, O. G.

AU - Ivanova, A. L.

AU - Ivanova, A. D.

AU - Iliushin, M. A.

AU - Kalmykov, N. N.

AU - Kindin, V. V.

AU - Kiryuhin, S. N.

AU - Kokoulin, R. P.

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 - 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 - Volkov, N. V.

AU - Voronin, D. M.

N1 - This work was supported by the Ministry of Science and Higher Education of the Russian Federation (agreement EB-075-15-2021-675, subjects of the state assignment FZZE-2023-0004 and FZZE-2024-0005) and the Russian Science Foundation (project no. 23-72-00019: sections “Procedure of Extracting the Light Component,” “Spectrum of the Light Component,” and “Conclusions”; project no. 23-72-00016: sections “Procedure of Extracting the Light Component” and “Spectrum of the Light Component”).

PY - 2025/7/15

Y1 - 2025/7/15

N2 - Abstract: New results on measuring the spectrum of the light component (protons + helium) of cosmic rays in the classical knee region in the primary cosmic ray spectrum at energies of ∼200–20 000 are presented. The results were obtained from hybrid data of the TAIGA experiment in which Cherenkov light of the shower is recorded simultaneously by two (IACT + HiSCORE) facilities. The showers are separated from the light component for the first time using image parameters recorded by the IACT atmospheric image telescope. The developed approach to separation of the light component is based on and confirmed by Monte Carlo calculations. In the obtained spectrum of the light component in the energy range of 200–20 000 TeV, a pronounced knee is observed at an energy of about 3 PeV.

AB - Abstract: New results on measuring the spectrum of the light component (protons + helium) of cosmic rays in the classical knee region in the primary cosmic ray spectrum at energies of ∼200–20 000 are presented. The results were obtained from hybrid data of the TAIGA experiment in which Cherenkov light of the shower is recorded simultaneously by two (IACT + HiSCORE) facilities. The showers are separated from the light component for the first time using image parameters recorded by the IACT atmospheric image telescope. The developed approach to separation of the light component is based on and confirmed by Monte Carlo calculations. In the obtained spectrum of the light component in the energy range of 200–20 000 TeV, a pronounced knee is observed at an energy of about 3 PeV.

KW - Cherenkov telescope

KW - chemical composition

KW - extensive atmospheric showers

KW - primary cosmic rays

UR - https://www.mendeley.com/catalogue/77364c8d-6a2f-3aa0-a5cb-671e9f74fd2e/

UR - https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=105010705309&origin=inward

U2 - 10.1134/S1062873825711638

DO - 10.1134/S1062873825711638

M3 - статья

VL - 89

SP - 899

EP - 903

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: 68545657