Energy Spectrum of Primary Cosmic Rays, According to TUNKA-133 and TAIGA-HiSCORE EAS Cherenkov Light Data

被引：9

作者：

Prosin V.V. ^{[1
]}

Astapov I.I. ^{[2
]}

Bezyazeekov P.A. ^{[3
]}

Boreyko V. ^{[4
]}

Borodin A.N. ^{[4
]}

Brueckner M. ^{[5
]}

Budnev N.M. ^{[3
]}

Wischnewski R. ^{[5
]}

Garmash A.Y. ^{[6
,7
]}

Gafarov A.R. ^{[3
]}

Gorbunov N.V. ^{[4
]}

Grebenyuk V.M. ^{[4
,8
]}

Gress O.A. ^{[3
]}

Gress T.I. ^{[3
]}

Grinyuk A.A. ^{[4
]}

Grishin O.G. ^{[3
]}

Dyachok A.N. ^{[3
]}

Zhurov D.P. ^{[3
]}

Zagorodnikov A.V. ^{[3
]}

Zurbanov V.L. ^{[3
]}

Ivanova A.L. ^{[3
]}

Kazarina Y.A. ^{[3
]}

Kalmykov N.N. ^{[1
]}

Kindin V.V. ^{[2
]}

Kirilenko P.S. ^{[6
]}

Kiryuhin S.N. ^{[3
]}

Kozhin V.A. ^{[1
]}

Kokoulin R.P. ^{[2
]}

Kompaniets K.G. ^{[2
]}

Korosteleva E.E. ^{[1
]}

Kravchenko E.A. ^{[6
,7
]}

Kuzmichev L.A. ^{[1
]}

Kunnas M. ^{[9
]}

Chiavassa A. ^{[10
]}

Lagutin A.A. ^{[11
]}

Lemeshev Y. ^{[3
]}

Lenok V.V. ^{[3
]}

Lubsandorzhiev B.K. ^{[12
]}

Lubsandorzhiev N.B. ^{[1
]}

Mirgazov R.R. ^{[3
]}

Mirzoyan R. ^{[3
,13
]}

Monkhoev R.D. ^{[3
]}

Osipova E.A. ^{[1
]}

Panasyuk M.I. ^{[1
]}

Pankov L.V. ^{[3
]}

Pakhorukov A.L. ^{[3
]}

Petrukhin A.A. ^{[2
]}

Poleschuk V.A. ^{[3
]}

Popescu M. ^{[14
]}

Popova E.G. ^{[1
]}

机构：

[1] Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow

[2] National Research Nuclear University MEPhI (Moscow Engineering Physics Institute), Moscow

[3] Institute of Applied Physics, Irkutsk State University, Irkutsk

[4] Joint Institute for Nuclear Research, Dubna

[5] Deutsches Elektronen-Synchrotron (DESY), Zeuthen

[6] Novosibirsk National Research University, Novosibirsk

[7] Institute of Applied Physics, Russian Academy of Sciences, Nizhny Novgorod

[8] Dubna University, Dubna

[9] Institute for Experimental Physics, University of Hamburg, Hamburg

[10] Department of Physics, Turin University, National Institute for Nuclear Physics, Turin

[11] Altai State University, Barnaul

[12] Institute for Nuclear Research, Russian Academy of Sciences, Moscow

[13] Max Planck Institute, Munich

[14] Institute of Space Sciences, Bucharest

[15] Pushkov Institute of Terrestrial Magnetism, the Ionosphere, and Radiowave Propagation, Russian Academy of Sciences, Moscow

来源：

Bulletin of the Russian Academy of Sciences: Physics | 2019年 / 83卷 / 08期

基金：

俄罗斯基础研究基金会;

关键词：

Cosmic rays;

D O I：

10.3103/S1062873819080343

中图分类号：

学科分类号：

摘要：

Abstract: The Tunka-133 Cherenkov complex for recording extensive air showers (EAS) collected data over seven winters from 2009 to 2017. The differential energy spectra of all particles was acquired in the 6 × 1015–3 × 1018 eV range of energies over 2175 h. The TAIGA-HiSCORE complex is continually being expanded and upgraded. Data acquired by 30 first-line stations over 35 days during the period 2017–2018 is analyzed in this work. As at the Tunka-133 setup, the primary particle energies above 1015 eV are measured using the density of the Cherenkov light flux at a distance of 200 m from a shower’s axis. Data on lower energies are collected by determining the energy of the light flux near a shower’s axis. This results in a spectrum of 2 × 1014–1017 eV. The combined spectrum for the two systems covers a range of 2 × 1014–2 × 1018 eV. © 2019, Allerton Press, Inc.

引用

页码：1016 / 1019

页数：3

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