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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

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dc.contributor.authorProsin, V. V.
dc.contributor.authorBezyazeekov, P. A.
dc.contributor.authorBorodin, A. N.
dc.contributor.authorBruckner, M.
dc.contributor.authorAstapov, I. I.
dc.contributor.authorKindin, V. V.
dc.contributor.authorKindin,V.V.
dc.contributor.authorKokoulin, R. P.
dc.contributor.authorKokoulin,R.P.
dc.contributor.authorKompaniets, K. G.
dc.contributor.authorPetrukhin, A. A.
dc.contributor.authorSuvorkin, Y.
dc.contributor.authorTanaev, A.
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.accessioned2024-12-02T10:07:53Z
dc.date.available2024-12-02T10:07:53Z
dc.date.issued2021
dc.description.abstract© 2021, Allerton Press, Inc.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.
dc.format.extentС. 395-397
dc.identifier.citationDepth 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 / Prosin, V.V. [et al.] // Bulletin of the Russian Academy of Sciences: Physics. - 2021. - 85. - № 4. - P. 395-397. - 10.3103/S1062873821040298
dc.identifier.doi10.3103/S1062873821040298
dc.identifier.urihttps://www.doi.org/10.3103/S1062873821040298
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85106263802&origin=resultslist
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/25516
dc.relation.ispartofBulletin of the Russian Academy of Sciences: Physics
dc.titleDepth 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
dc.typeArticle
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oaire.citation.issue4
oaire.citation.volume85
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