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

L. G. Tkachev; A. V. Tkachenko; M. Tluczykont; O. L. Fedorov; D. Horns; C. Spiering; I. I. Yashin; V. V. Prosin; I. I. Astapov; P. A. Bezyazeekov; V. Boreyko; A. N. Borodin; M. Brueckner; N. M. Budnev; R. Wischnewski; A. Yu. Garmash; A. R. Gafarov; N. V. Gorbunov; V. M. Grebenyuk; O. A. Gress; T. I. Gress; A. A. Grinyuk; O. G. Grishin; A. N. Dyachok; D. P. Zhurov; A. V. Zagorodnikov; V. L. Zurbanov; A. L. Ivanova; Yu. A. Kazarina; N. N. Kalmykov; V. V. Kindin; P. S. Kirilenko; S. N. Kiryuhin; V. A. Kozhin; R. P. Kokoulin; K. G. Kompaniets; E. E. Korosteleva; E. A. Kravchenko; L. A. Kuzmichev; M. Kunnas; A. Chiavassa; A. A. Lagutin; Yu. Lemeshev; V. V. Lenok; B. K. Lubsandorzhiev; N. B. Lubsandorzhiev; R. R. Mirgazov; R. Mirzoyan; R. D. Monkhoev; E. A. Osipova; M. I. Panasyuk; L. V. Pankov; A. L. Pakhorukov; A. A. Petrukhin; V. A. Poleschuk; M. Popescu; E. G. Popova; A. Porelli; E. B. Postnikov; V. S. Ptuskin; A. A. Pushnin; R. I. Raikin; G. I. Rubtsov; E. V. Rjabov; B. M. Sabirov; Y. I. Sagan; V. S. Samoliga; L. G. Sveshnikova; Yu. A. Semeney; A. Yu. Sidorenkov; A. A. Silaev; A. A. Silaev; A. V. Skurikhin; M. Slunecka; A. V. Sokolov; V. A. Tabolenko; B. A. Tarashansky

doi:10.3103/S1062873819080343

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

Авторлар: Tkachev L.G.¹^,2, Tkachenko A.V.¹, Tluczykont M.³, Fedorov O.L.⁴, Horns D.³, Spiering C.⁵, Yashin I.I.⁶, Prosin V.V.⁷, Astapov I.I.⁶, Bezyazeekov P.A.⁴, Boreyko V.¹, Borodin A.N.¹, Brueckner M.⁵, Budnev N.M.⁴, Wischnewski R.⁵, Garmash A.Y.⁸^,9, Gafarov A.R.⁴, Gorbunov N.V.¹, Grebenyuk V.M.¹^,2, Gress O.A.⁴, Gress T.I.⁴, Grinyuk A.A.¹, Grishin O.G.⁴, Dyachok A.N.⁴, Zhurov D.P.⁴, Zagorodnikov A.V.⁴, Zurbanov V.L.⁴, Ivanova A.L.⁴, Kazarina Y.A.⁴, Kalmykov N.N.⁷, Kindin V.V.⁶, Kirilenko P.S.⁸, Kiryuhin S.N.⁴, Kozhin V.A.⁷, Kokoulin R.P.⁶, Kompaniets K.G.⁶, Korosteleva E.E.⁷, Kravchenko E.A.⁸^,9, Kuzmichev L.A.⁷, Kunnas M.³, Chiavassa A.¹⁰, Lagutin A.A.¹¹, Lemeshev Y.⁴, Lenok V.V.⁴, Lubsandorzhiev B.K.¹², Lubsandorzhiev N.B.⁷, Mirgazov R.R.⁴, Mirzoyan R.⁴^,13, Monkhoev R.D.⁴, Osipova E.A.⁷, Panasyuk M.I.⁷, Pankov L.V.⁴, Pakhorukov A.L.⁴, Petrukhin A.A.⁶, Poleschuk V.A.⁴, Popescu M.¹⁴, Popova E.G.⁷, Porelli A.⁵, Postnikov E.B.⁷, Ptuskin V.S.¹⁵, Pushnin A.A.⁴, Raikin R.I.¹¹, Rubtsov G.I.¹², Rjabov E.V.⁴, Sabirov B.M.¹, Sagan Y.I.¹^,2, Samoliga V.S.⁴, Sveshnikova L.G.⁷, Semeney Y.A.⁴, Sidorenkov A.Y.¹², Silaev A.A.⁷, Silaev A.A.⁷, Skurikhin A.V.⁷, Slunecka M.¹, Sokolov A.V.⁸^,9, Tabolenko V.A.⁴, Tarashansky B.A.⁴
Мекемелер:
1. Joint Institute for Nuclear Research
2. Dubna University
3. Institute for Experimental Physics, University of Hamburg
4. Institute of Applied Physics, Irkutsk State University
5. Deutsches Elektronen-Synchrotron (DESY)
6. National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
7. Skobeltsyn Institute of Nuclear Physics, Moscow State University
8. Novosibirsk National Research University
9. Institute of Applied Physics, Russian Academy of Sciences
10. Department of Physics, Turin University, National Institute for Nuclear Physics
11. Altai State University
12. Institute for Nuclear Research, Russian Academy of Sciences
13. Max Planck Institute
14. Institute of Space Sciences
15. Pushkov Institute of Terrestrial Magnetism, the Ionosphere, and Radiowave Propagation, Russian Academy of Sciences
Шығарылым: Том 83, № 8 (2019)
Беттер: 1016-1019
Бөлім: Article
URL: https://journals.rcsi.science/1062-8738/article/view/187504
DOI: https://doi.org/10.3103/S1062873819080343
ID: 187504

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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.

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

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