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Technique for reconstructing the parameters of EAS and primary cosmic rays based on experimental data of the Tunka-Grande scintillation array. / TAIGA Collaboration.

в: St. Petersburg State Polytechnical University Journal: Physics and Mathematics, Том 16, № S1.2, 2023, стр. 389-394.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

TAIGA Collaboration 2023, 'Technique for reconstructing the parameters of EAS and primary cosmic rays based on experimental data of the Tunka-Grande scintillation array', St. Petersburg State Polytechnical University Journal: Physics and Mathematics, Том. 16, № S1.2, стр. 389-394. https://doi.org/10.18721/JPM.161.259

APA

TAIGA Collaboration (2023). Technique for reconstructing the parameters of EAS and primary cosmic rays based on experimental data of the Tunka-Grande scintillation array. St. Petersburg State Polytechnical University Journal: Physics and Mathematics, 16(S1.2), 389-394. https://doi.org/10.18721/JPM.161.259

Vancouver

TAIGA Collaboration. Technique for reconstructing the parameters of EAS and primary cosmic rays based on experimental data of the Tunka-Grande scintillation array. St. Petersburg State Polytechnical University Journal: Physics and Mathematics. 2023;16(S1.2):389-394. doi: 10.18721/JPM.161.259

Author

TAIGA Collaboration. / Technique for reconstructing the parameters of EAS and primary cosmic rays based on experimental data of the Tunka-Grande scintillation array. в: St. Petersburg State Polytechnical University Journal: Physics and Mathematics. 2023 ; Том 16, № S1.2. стр. 389-394.

BibTeX

@article{464278cdfa084c33be93194baf456fee,
title = "Technique for reconstructing the parameters of EAS and primary cosmic rays based on experimental data of the Tunka-Grande scintillation array",
abstract = "The Tunka-Grande scintillation array is a part of a single TAIGA experimental complex located in the Tunka Valley, 50 km from the Lake Baikal. It consists of 19 observation stations deployed on an area of about 0.5 km2. The main aim of the Tunka-Grande facility is a detailed study of the energy spectrum and mass composition of cosmic rays in the energy range from 10 PeV to 1 EeV by detecting the charged and muon component of EAS. The article presents a method for reconstructing the parameters of the EAS and primary cosmic rays, the cosmic rays energy spectrum based on 4 measurement seasons, and compares the results obtained with the data of the Tunka-133 and TAIGA-HiSCORE Cherenkov arrays.",
author = "{the TAIGA Collaboration} and Иванова, {Анна Леонидовна}",
note = "The work was performed at the UNU “Astrophysical Complex of MSU-ISU” (agreement EB-075-15-2021-675). The work is supported by Russian Foundation for Basic Research (grant 19-32-60003), the Russian Science Foundation (grants 23-72-00016 (Section 3), 23-72-00054 (Sections 4, 5)), the Ministry of Science and Higher Education of the Russian Federation (projects FZZE-2020-0024, FZZE-2023-0004, FSUS-2020-0039, FSUS-2022-0015).",
year = "2023",
doi = "10.18721/JPM.161.259",
language = "English",
volume = "16",
pages = "389--394",
journal = "Научно-технические ведомости СПбГПУ. Физико-математические науки Cанкт-Петербургский политехнический университет Петра Великого ru",
issn = "2304-9782",
publisher = "Санкт-Петербургский политехнический университет Петра Великого",
number = "S1.2",

}

RIS

TY - JOUR

T1 - Technique for reconstructing the parameters of EAS and primary cosmic rays based on experimental data of the Tunka-Grande scintillation array

AU - the TAIGA Collaboration

AU - Иванова, Анна Леонидовна

N1 - The work was performed at the UNU “Astrophysical Complex of MSU-ISU” (agreement EB-075-15-2021-675). The work is supported by Russian Foundation for Basic Research (grant 19-32-60003), the Russian Science Foundation (grants 23-72-00016 (Section 3), 23-72-00054 (Sections 4, 5)), the Ministry of Science and Higher Education of the Russian Federation (projects FZZE-2020-0024, FZZE-2023-0004, FSUS-2020-0039, FSUS-2022-0015).

PY - 2023

Y1 - 2023

N2 - The Tunka-Grande scintillation array is a part of a single TAIGA experimental complex located in the Tunka Valley, 50 km from the Lake Baikal. It consists of 19 observation stations deployed on an area of about 0.5 km2. The main aim of the Tunka-Grande facility is a detailed study of the energy spectrum and mass composition of cosmic rays in the energy range from 10 PeV to 1 EeV by detecting the charged and muon component of EAS. The article presents a method for reconstructing the parameters of the EAS and primary cosmic rays, the cosmic rays energy spectrum based on 4 measurement seasons, and compares the results obtained with the data of the Tunka-133 and TAIGA-HiSCORE Cherenkov arrays.

AB - The Tunka-Grande scintillation array is a part of a single TAIGA experimental complex located in the Tunka Valley, 50 km from the Lake Baikal. It consists of 19 observation stations deployed on an area of about 0.5 km2. The main aim of the Tunka-Grande facility is a detailed study of the energy spectrum and mass composition of cosmic rays in the energy range from 10 PeV to 1 EeV by detecting the charged and muon component of EAS. The article presents a method for reconstructing the parameters of the EAS and primary cosmic rays, the cosmic rays energy spectrum based on 4 measurement seasons, and compares the results obtained with the data of the Tunka-133 and TAIGA-HiSCORE Cherenkov arrays.

UR - https://www.scopus.com/record/display.uri?eid=2-s2.0-85218784733&origin=inward&txGid=0b49daded63afd82effed8da824409c7

UR - https://www.elibrary.ru/item.asp?id=54663985

U2 - 10.18721/JPM.161.259

DO - 10.18721/JPM.161.259

M3 - Article

VL - 16

SP - 389

EP - 394

JO - Научно-технические ведомости СПбГПУ. Физико-математические науки Cанкт-Петербургский политехнический университет Петра Великого ru

JF - Научно-технические ведомости СПбГПУ. Физико-математические науки Cанкт-Петербургский политехнический университет Петра Великого ru

SN - 2304-9782

IS - S1.2

ER -

ID: 65076941