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Studying the Mass Composition of Cosmic Rays with Energies of 1015–1017 eV in the PRISMA Project

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dc.contributor.authorShchegolev, O. B.
dc.contributor.authorAlekseenko, V. V.
dc.contributor.authorStepanov, V. I.
dc.contributor.authorYanin, Y. V.
dc.contributor.authorStenkin, Y. V.
dc.contributor.authorСтенькин, Юрий Васильевич
dc.date.accessioned2024-11-21T09:49:49Z
dc.date.available2024-11-21T09:49:49Z
dc.date.issued2019
dc.description.abstract© 2019, Allerton Press, Inc.Abstract: The mass composition of primary cosmic rays remains an unresolved problem of physics in the region of energies above the knee. Results from different experiments are contradictory in assessments of the mean mass number and its variation as the primary energy grows. The PRISMA project is designed to study the energy spectrum and mass composition of cosmic rays at energies of 1015–1017 eV. The project is based on a detector capable of simultaneously detecting the electromagnetic and hadron components of a shower. The results are presented from measurements with the PRISMA-YBJ prototype located at 4300 m a.s.l., made over 3.5 years of operation. A new way of estimating the average mass composition from the electron/neutron ratio is tested.
dc.format.extentС. 632-634
dc.identifier.citationStudying the Mass Composition of Cosmic Rays with Energies of 1015–1017 eV in the PRISMA Project / Shchegolev, O.B. [et al.] // Bulletin of the Russian Academy of Sciences: Physics. - 2019. - 83. - № 5. - P. 632-634. - 10.3103/S1062873819050320
dc.identifier.doi10.3103/S1062873819050320
dc.identifier.urihttps://www.doi.org/10.3103/S1062873819050320
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85067556678&origin=resultslist
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/18302
dc.relation.ispartofBulletin of the Russian Academy of Sciences: Physics
dc.titleStudying the Mass Composition of Cosmic Rays with Energies of 1015–1017 eV in the PRISMA Project
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue5
oaire.citation.volume83
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relation.isAuthorOfPublication.latestForDiscovery6f27583c-a224-476f-8264-3775be121041
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