Depth of the Maximum of Extensive Air Showers (EASes) and the Mean Mass Composition of Primary Cosmic Rays in the 1015–1018 eV Range of Energies, According to Data from the TUNKA-133 and TAIGA-HiSCORE Arrays for Detecting EAS Cherenkov Light in the Tunkinsk Valley

被引：0

作者：

Prosin V.V. ^{[1
]}

Astapov I.I. ^{[2
]}

Bezyazeekov P.A. ^{[3
]}

Borodin A.N. ^{[4
]}

Brückner M. ^{[5
]}

Budnev N.M. ^{[3
]}

Bulan A. ^{[1
]}

Vaidyanathan A. ^{[5
]}

Wischnewski R. ^{[5
]}

Volchugov P. ^{[1
]}

Voronin D. ^{[6
]}

Gafarov A.R. ^{[3
]}

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

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
]}

Ivanova A.L. ^{[3
]}

Kalmykov N.N. ^{[1
]}

Kindin V.V. ^{[2
]}

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
]}

Kryukov A.P. ^{[1
]}

Kuzmichev L.A. ^{[1
]}

Chiavassa A. ^{[10
]}

Lavrova M. ^{[3
]}

Lagutin A.A. ^{[11
]}

Lemeshev Y. ^{[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
]}

Pan A. ^{[3
]}

Panasyuk M.I. ^{[1
]}

Pankov L.V. ^{[3
]}

Pakhorukov A.L. ^{[3
]}

Petrukhin A.A. ^{[2
]}

Poleschuk V.A. ^{[3
]}

Popesku 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

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

[4] Joint Institute for Nuclear Research, Dubna, 141980, Moscow oblast

[5] German Electron Synchrotron (DESY), Zeuthen

[6] Novosibirsk State University, Novosibirsk

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

[8] Dubna State University, Dubna, 141982, Moscow oblast

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

[10] Department of Physics and INFN, Torino University, Turin

[11] Altai State University, Barnaul, 656049, Altai krai

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

[13] Max Planck Institute, Munich

[14] Institute of Space Sciences, Bucharest

[15] Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, Russian Academy of Sciences, TroitskMoscow

来源：

Bulletin of the Russian Academy of Sciences: Physics | 2021年 / 85卷 / 04期

基金：

俄罗斯科学基金会;

关键词：

D O I：

10.3103/S1062873821040298

中图分类号：

学科分类号：

摘要：

Abstract: A corrected energy dependence of the depth of the maximum in the wide range of energies 1015 to 1018 eV is obtained using data collected at the Tunka-133 facility over 7 years of operation (2009–2017) and the TAIGA-HiSCORE facility in the 2019–2020 season. At the highest energies, our results match those of the Pierre Auger observatory. The results are converted to parameter ❬ln A❭, which characterizes the mean EAS composition. © 2021, Allerton Press, Inc.

引用

页码：395 / 397

页数：2

共 7 条

[1] Energy Spectrum of Primary Cosmic Rays, According to TUNKA-133 and TAIGA-HiSCORE EAS Cherenkov Light Data
Prosin V.V.
Astapov I.I.
Bezyazeekov P.A.
Boreyko V.
Borodin A.N.
Brueckner M.
Budnev N.M.
Wischnewski R.
Garmash A.Y.
Gafarov A.R.
Gorbunov N.V.
Grebenyuk V.M.
Gress O.A.
Gress T.I.
Grinyuk A.A.
Grishin O.G.
Dyachok A.N.
Zhurov D.P.
Zagorodnikov A.V.
Zurbanov V.L.
Ivanova A.L.
Kazarina Y.A.
Kalmykov N.N.
Kindin V.V.
Kirilenko P.S.
Kiryuhin S.N.
Kozhin V.A.
Kokoulin R.P.
Kompaniets K.G.
Korosteleva E.E.
Kravchenko E.A.
Kuzmichev L.A.
Kunnas M.
Chiavassa A.
Lagutin A.A.
Lemeshev Y.
Lenok V.V.
Lubsandorzhiev B.K.
Lubsandorzhiev N.B.
Mirgazov R.R.
Mirzoyan R.
Monkhoev R.D.
Osipova E.A.
Panasyuk M.I.
Pankov L.V.
Pakhorukov A.L.
Petrukhin A.A.
Poleschuk V.A.
Popescu M.
Popova E.G.
Bulletin of the Russian Academy of Sciences: Physics, 2019, 83 (08) : 1016 - 1019
[2] On the sensitivity of the spatial-angular distribution of the Cherenkov light in extensive air showers to the mass composition of primary cosmic rays with energies of 1015–1016 eV
V. I. Galkin
T. A. Dzhatdoev
Moscow University Physics Bulletin, 2010, 65 : 195 - 202
[3] On the sensitivity of the spatial-angular distribution of the Cherenkov light in extensive air showers to the mass composition of primary cosmic rays with energies of 1015-1016 eV
Galkin, V. I.
Dzhatdoev, T. A.
MOSCOW UNIVERSITY PHYSICS BULLETIN, 2010, 65 (03) : 195 - 202
[4] Depth of the maximum of extensive air showers and mass composition of primary cosmic radiation at an energy of 4 × 1017 eV according to data on radioemission from extensive air showers
O. V. Vedeneev
Physics of Atomic Nuclei, 2009, 72 : 250 - 256
[5] Depth of the maximum of extensive air showers and mass composition of primary cosmic radiation at an energy of 4 x 1017 eV according to data on radioemission from extensive air showers
Vedeneev, O. V.
PHYSICS OF ATOMIC NUCLEI, 2009, 72 (02) : 250 - 256
[6] Mass composition of 1017- to 1018-eV primary cosmic rays according to data on the lateral distribution of radio emission from extensive air showers
N. N. Kalmykov
A. A. Konstantinov
O. V. Vedeneev
Physics of Atomic Nuclei, 2012, 75 : 1513 - 1522
[7] Mass composition of 1017- to 1018-eV primary cosmic rays according to data on the lateral distribution of radio emission from extensive air showers
Kalmykov, N. N.
Konstantinov, A. A.
Vedeneev, O. V.
PHYSICS OF ATOMIC NUCLEI, 2012, 75 (12) : 1513 - 1522

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