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

In: Bulletin of the Russian Academy of Sciences: Physics, Vol. 83, No. 8, 01.08.2019, p. 1016-1019.

Research output: Contribution to journal › Article › peer-review

Harvard

the TAIGA Collaboration 2019, 'Energy Spectrum of Primary Cosmic Rays, According to TUNKA-133 and TAIGA-HiSCORE EAS Cherenkov Light Data', Bulletin of the Russian Academy of Sciences: Physics, vol. 83, no. 8, pp. 1016-1019. https://doi.org/10.3103/S1062873819080343

APA

the TAIGA Collaboration (2019). Energy Spectrum of Primary Cosmic Rays, According to TUNKA-133 and TAIGA-HiSCORE EAS Cherenkov Light Data. Bulletin of the Russian Academy of Sciences: Physics, 83(8), 1016-1019. https://doi.org/10.3103/S1062873819080343

Vancouver

the TAIGA Collaboration. Energy Spectrum of Primary Cosmic Rays, According to TUNKA-133 and TAIGA-HiSCORE EAS Cherenkov Light Data. Bulletin of the Russian Academy of Sciences: Physics. 2019 Aug 1;83(8):1016-1019. doi: 10.3103/S1062873819080343

Author

the TAIGA Collaboration. / Energy Spectrum of Primary Cosmic Rays, According to TUNKA-133 and TAIGA-HiSCORE EAS Cherenkov Light Data. In: Bulletin of the Russian Academy of Sciences: Physics. 2019 ; Vol. 83, No. 8. pp. 1016-1019.

BibTeX

@article{9f186a4e896541288372b9742b77b1c2,
title = "Energy Spectrum of Primary Cosmic Rays, According to TUNKA-133 and TAIGA-HiSCORE EAS Cherenkov Light Data",
abstract = "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{\textquoteright}s axis. Data on lower energies are collected by determining the energy of the light flux near a shower{\textquoteright}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.",
author = "{the TAIGA Collaboration} and Prosin, {V. V.} and Astapov, {I. I.} and Bezyazeekov, {P. A.} and V. Boreyko and Borodin, {A. N.} and M. Brueckner and Budnev, {N. M.} and R. Wischnewski and Garmash, {A. Yu} and Gafarov, {A. R.} and Gorbunov, {N. V.} and Grebenyuk, {V. M.} and Gress, {O. A.} and Gress, {T. I.} and Grinyuk, {A. A.} and Grishin, {O. G.} and Dyachok, {A. N.} and Zhurov, {D. P.} and Zagorodnikov, {A. V.} and Zurbanov, {V. L.} and Ivanova, {A. L.} and Kazarina, {Yu A.} and Kalmykov, {N. N.} and Kindin, {V. V.} and Kirilenko, {P. S.} and Kiryuhin, {S. N.} and Kozhin, {V. A.} and Kokoulin, {R. P.} and Kompaniets, {K. G.} and Korosteleva, {E. E.} and Kravchenko, {E. A.} and Kuzmichev, {L. A.} and M. Kunnas and A. Chiavassa and Lagutin, {A. A.} and Yu Lemeshev and Lenok, {V. V.} and Lubsandorzhiev, {B. K.} and Lubsandorzhiev, {N. B.} and Mirgazov, {R. R.} and R. Mirzoyan and Monkhoev, {R. D.} and Osipova, {E. A.} and Panasyuk, {M. I.} and Pankov, {L. V.} and Pakhorukov, {A. L.} and Petrukhin, {A. A.} and Poleschuk, {V. A.} and Rubtsov, {G. I.} and Sokolov, {A. V.}",
note = "Publisher Copyright: {\textcopyright} 2019, Allerton Press, Inc.",
year = "2019",
month = aug,
day = "1",
doi = "10.3103/S1062873819080343",
language = "English",
volume = "83",
pages = "1016--1019",
journal = "Bulletin of the Russian Academy of Sciences: Physics",
issn = "1062-8738",
publisher = "PLEIADES PUBLISHING INC",
number = "8",

}

RIS

TY - JOUR

T1 - Energy Spectrum of Primary Cosmic Rays, According to TUNKA-133 and TAIGA-HiSCORE EAS Cherenkov Light Data

AU - the TAIGA Collaboration

AU - Prosin, V. V.

AU - Astapov, I. I.

AU - Bezyazeekov, P. A.

AU - Boreyko, V.

AU - Borodin, A. N.

AU - Brueckner, M.

AU - Budnev, N. M.

AU - Wischnewski, R.

AU - Garmash, A. Yu

AU - Gafarov, A. R.

AU - Gorbunov, N. V.

AU - Grebenyuk, V. M.

AU - Gress, O. A.

AU - Gress, T. I.

AU - Grinyuk, A. A.

AU - Grishin, O. G.

AU - Dyachok, A. N.

AU - Zhurov, D. P.

AU - Zagorodnikov, A. V.

AU - Zurbanov, V. L.

AU - Ivanova, A. L.

AU - Kazarina, Yu A.

AU - Kalmykov, N. N.

AU - Kindin, V. V.

AU - Kirilenko, P. S.

AU - Kiryuhin, S. N.

AU - Kozhin, V. A.

AU - Kokoulin, R. P.

AU - Kompaniets, K. G.

AU - Korosteleva, E. E.

AU - Kravchenko, E. A.

AU - Kuzmichev, L. A.

AU - Kunnas, M.

AU - Chiavassa, A.

AU - Lagutin, A. A.

AU - Lemeshev, Yu

AU - Lenok, V. V.

AU - Lubsandorzhiev, B. K.

AU - Lubsandorzhiev, N. B.

AU - Mirgazov, R. R.

AU - Mirzoyan, R.

AU - Monkhoev, R. D.

AU - Osipova, E. A.

AU - Panasyuk, M. I.

AU - Pankov, L. V.

AU - Pakhorukov, A. L.

AU - Petrukhin, A. A.

AU - Poleschuk, V. A.

AU - Rubtsov, G. I.

AU - Sokolov, A. V.

N1 - Publisher Copyright: © 2019, Allerton Press, Inc.

PY - 2019/8/1

Y1 - 2019/8/1

N2 - 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.

AB - 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.

UR - http://www.scopus.com/inward/record.url?scp=85073209890&partnerID=8YFLogxK

U2 - 10.3103/S1062873819080343

DO - 10.3103/S1062873819080343

M3 - Article

AN - SCOPUS:85073209890

VL - 83

SP - 1016

EP - 1019

JO - Bulletin of the Russian Academy of Sciences: Physics

JF - Bulletin of the Russian Academy of Sciences: Physics

SN - 1062-8738

IS - 8

ER -

ID: 21854399