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

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发表日期：

2025年6月1日

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V. V. Prosin,
I. I. Astapov,
P. A. Bezyazeekov,
A. V. Blinov,
A. N. Borodin,
E. A. Bonvech,
N. M. Budnev,
A. V. Bulan,
N. V. Volkov,
P. A. Volchugov,
D. M. Voronin,
A. R. Gafarov,
E. O. Gress,
O. A. Gress,
T. I. Gress,
A. A. Grinyuk,
O. G. Grishin,
A. Yu. Garmash,
V. M. Grebenyuk,
A. N. Dyachok,
D. P. Zhurov,
A. V. Zagorodnikov,
V. N. Zirakashvili,
A. D. Ivanova,
A. L. Ivanova,
M. A. Iliushin,
N. N. Kalmykov,
V. V. Kindin,
S. N. Kiryuhin,
R. P. Kokoulin,
N. I. Kolosov,
K. G. Kompaniets,
E. E. Korosteleva,
V. A. Kozhin,
E. A. Kravchenko,
A. P. Kryukov,
L. A. Kuzmichev,
A. Chiavassa,
M. V. Lavrova,
A. A. Lagutin,
Yu. E. Lemeshev,
B. K. Lubsandorzhiev,
N. B. Lubsandorzhiev,
A. D. Lukanov,
S. D. Malakhov,
R. R. Mirgazov,
R. D. Monkhoev,
E. A. Okuneva,
E. A. Osipova,
A. L. Pakhorukov,
A. Pan,
A. D. Panov,
L. V. Pankov,
A. A. Petrukhin,
D. A. Podgrudkov,
I. A. Poddubny,
E. G. Popova,
E. B. Postnikov,
A. A. Pushnin,
A. Yu. Razumov,
R. Raikin,
G. I. Rubtsov,
E. V. Ryabov,
V. S. Samoliga,
I. I. Satyshev,
L. G. Sveshnikova,
A. A. Silaev,
A. A. Silaev Jr.,
A. Yu. Sidorenkov,
A. V. Skurikhin,
A. V. Sokolov,
V. A. Tabolenko,
A. B. Tanaev,
M. Yu. Ternovoy,
L. G. Tkachev,
N. A. Ushakov,
D. V. Chernov,
A. V. Shaikovsky,
I. I. Yashin

摘要

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.