Standard

Energy spectrum and mass composition of cosmic rays according to the data of the TAIGA-HiSCORE installation. / TAIGA Collaboration ; Иванова, Анна Леонидовна; Кабанник, Иван Артемович и др.

в: Proceedings of Science, Том 501, 206, 30.12.2025.

Результаты исследований: Научные публикации в периодических изданиях › статья по материалам конференции › Рецензирование

Harvard

TAIGA Collaboration, Иванова, АЛ, Кабанник, ИА, Кравченко, ЕА, Монхоев, РД & Соколов, АВ 2025, 'Energy spectrum and mass composition of cosmic rays according to the data of the TAIGA-HiSCORE installation', Proceedings of Science, Том. 501, 206. https://doi.org/10.22323/1.501.0206

APA

TAIGA Collaboration, Иванова, А. Л., Кабанник, И. А., Кравченко, Е. А., Монхоев, Р. Д., & Соколов, А. В. (2025). Energy spectrum and mass composition of cosmic rays according to the data of the TAIGA-HiSCORE installation. Proceedings of Science, 501, [206]. https://doi.org/10.22323/1.501.0206

Vancouver

TAIGA Collaboration, Иванова АЛ, Кабанник ИА, Кравченко ЕА, Монхоев РД, Соколов АВ. Energy spectrum and mass composition of cosmic rays according to the data of the TAIGA-HiSCORE installation. Proceedings of Science. 2025 дек. 30;501:206. doi: 10.22323/1.501.0206

Author

TAIGA Collaboration ; Иванова, Анна Леонидовна ; Кабанник, Иван Артемович и др. / Energy spectrum and mass composition of cosmic rays according to the data of the TAIGA-HiSCORE installation. в: Proceedings of Science. 2025 ; Том 501.

BibTeX

@article{724b02fdeaab487ea18cc2ddd2d6b1c3,
title = "Energy spectrum and mass composition of cosmic rays according to the data of the TAIGA-HiSCORE installation",
abstract = "Since 2022, the TAIGA-HiSCORE installation, part of the TAIGA astrophysical complex, has been operational with 120 Cherenkov stations covering an area of 1 km2. The energy of Extensive Air Showers (EAS) is determined by the flux density of Cherenkov light at a distance of 200 m from the EAS axis for energies above 1 PeV and at 100 m for lower energies. The depth of the EAS maximum (Xmax) is derived from the steepness of the spatial distribution function of light, defined as the ratio of light fluxes at 80 m and 200 m from the axis. This paper presents the energy spectrum and mass composition of cosmic rays based on 700 hours of data collection, providing insights into the cosmic ray properties in the energy range of 105 to 1020 eV.",
author = "{the TAIGA Collaboration} and Гармаш, {Алексей Юрьевич} and Иванова, {Анна Леонидовна} and Кабанник, {Иван Артемович} and Кравченко, {Евгений Анатольевич} and Монхоев, {Роман Дмитриевич} and Соколов, {Андрей Валерьевич}",
note = "This work was carried out at the unique scientific installation “Astrophysical Complex MSU-ISU”. It was supported by the Russian Federation Ministry of Science and Higher Education (projects FZZE-2024-0005, FZZE-2023-0004, FSUS-2025-0008), the Russian Science Foundation (projects 23-72-00016 (section 5) and 23-72-00054 (section 4)), and the Irkutsk State University (project 091-25-309).; 39th International Cosmic Ray Conference , ICRC2025 ; Conference date: 15-07-2025 Through 24-07-2025",
year = "2025",
month = dec,
day = "30",
doi = "10.22323/1.501.0206",
language = "English",
volume = "501",
journal = "Proceedings of Science",
issn = "1824-8039",
publisher = "Sissa Medialab Srl",

}

RIS

TY - JOUR

T1 - Energy spectrum and mass composition of cosmic rays according to the data of the TAIGA-HiSCORE installation

AU - the TAIGA Collaboration

AU - Гармаш, Алексей Юрьевич

AU - Иванова, Анна Леонидовна

AU - Кабанник, Иван Артемович

AU - Кравченко, Евгений Анатольевич

AU - Монхоев, Роман Дмитриевич

AU - Соколов, Андрей Валерьевич

N1 - Conference code: 39

PY - 2025/12/30

Y1 - 2025/12/30

N2 - Since 2022, the TAIGA-HiSCORE installation, part of the TAIGA astrophysical complex, has been operational with 120 Cherenkov stations covering an area of 1 km2. The energy of Extensive Air Showers (EAS) is determined by the flux density of Cherenkov light at a distance of 200 m from the EAS axis for energies above 1 PeV and at 100 m for lower energies. The depth of the EAS maximum (Xmax) is derived from the steepness of the spatial distribution function of light, defined as the ratio of light fluxes at 80 m and 200 m from the axis. This paper presents the energy spectrum and mass composition of cosmic rays based on 700 hours of data collection, providing insights into the cosmic ray properties in the energy range of 105 to 1020 eV.

AB - Since 2022, the TAIGA-HiSCORE installation, part of the TAIGA astrophysical complex, has been operational with 120 Cherenkov stations covering an area of 1 km2. The energy of Extensive Air Showers (EAS) is determined by the flux density of Cherenkov light at a distance of 200 m from the EAS axis for energies above 1 PeV and at 100 m for lower energies. The depth of the EAS maximum (Xmax) is derived from the steepness of the spatial distribution function of light, defined as the ratio of light fluxes at 80 m and 200 m from the axis. This paper presents the energy spectrum and mass composition of cosmic rays based on 700 hours of data collection, providing insights into the cosmic ray properties in the energy range of 105 to 1020 eV.

UR - https://www.scopus.com/pages/publications/105029028114

U2 - 10.22323/1.501.0206

DO - 10.22323/1.501.0206

M3 - Conference article

VL - 501

JO - Proceedings of Science

JF - Proceedings of Science

SN - 1824-8039

M1 - 206

T2 - 39th International Cosmic Ray Conference

Y2 - 15 July 2025 through 24 July 2025

ER -

ID: 75618412