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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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dc.contributor.authorProsin, V. V.
dc.contributor.authorBezyazeekov, P. A.
dc.contributor.authorBoreyko, V.
dc.contributor.authorBorodin, A. N.
dc.contributor.authorAstapov, I. I.
dc.contributor.authorKindin, V. V.
dc.contributor.authorKokoulin, R. P.
dc.contributor.authorKompaniets, K. G.
dc.contributor.authorPetrukhin, A. A.
dc.contributor.authorYashin, I. I.
dc.contributor.authorАстапов, Иван Иванович
dc.contributor.authorКиндин, Виктор Владимирович
dc.contributor.authorКокоулин, Ростислав Павлович
dc.contributor.authorКомпаниец, Константин Георгиевич
dc.contributor.authorПетрухин, Анатолий Афанасьевич
dc.contributor.authorЯшин, Игорь Иванович
dc.date.accessioned2024-11-22T06:41:23Z
dc.date.available2024-11-22T06:41:23Z
dc.date.issued2019
dc.description.abstract© 2019, Allerton Press, Inc.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.
dc.format.extentС. 1016-1019
dc.identifier.citationEnergy Spectrum of Primary Cosmic Rays, According to TUNKA-133 and TAIGA-HiSCORE EAS Cherenkov Light Data / Prosin, V.V. [et al.] // Bulletin of the Russian Academy of Sciences: Physics. - 2019. - 83. - № 8. - P. 1016-1019. - 10.3103/S1062873819080343
dc.identifier.doi10.3103/S1062873819080343
dc.identifier.urihttps://www.doi.org/10.3103/S1062873819080343
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85073209890&origin=resultslist
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/19685
dc.relation.ispartofBulletin of the Russian Academy of Sciences: Physics
dc.titleEnergy Spectrum of Primary Cosmic Rays, According to TUNKA-133 and TAIGA-HiSCORE EAS Cherenkov Light Data
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue8
oaire.citation.volume83
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