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Pis'ma v Zhurnal Èksperimental'noi i Teoreticheskoi Fiziki, 2019, Volume 109, Issue 9, Pages 579–583
DOI: https://doi.org/10.1134/S0370274X19090017 (Mi jetpl5885) 		 
This article is cited in 12 scientific papers (total in 12 papers)

ASTROPHYSICS AND COSMOLOGY

Mass composition of cosmic rays with energies above 10$^{17}$ eV according to the data from the muon detectors of the Yakutsk EAS array

A. V. Glushkov, A. V. Saburov

Shafer Institute of Cosmophysical Research and Aeronomy, Yakut Research Center, Siberian Branch, Russian Academy of Sciences, Yakutsk, Russia
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DOI: https://doi.org/10.1134/S0370274X19090017
Abstract: The lateral distribution of muons in extensive air showers with energies above 10$^{17}$ eV detected by underground scintillation detectors with a threshold of 1.0 GeV at the Yakutsk array in 1986–2016 has been analyzed. The experimental data on the muon flux density at a distance of 300 m from the shower axis have been compared to the calculations within various models of hadron interactions at ultrahigh energies. The experimental data are in the best agreement with the QGSJet01 and QGSJet II-04 models. The mass composition of cosmic rays in the energy range of $(1-30) \times 10^{17}$ eV changes from middle nuclei to a purely proton composition.
Received: 22.02.2019
Revised: 22.03.2019
Accepted: 27.03.2019
English version:
Journal of Experimental and Theoretical Physics Letters, 2019, Volume 109, Issue 9, Pages 559–563
DOI: https://doi.org/10.1134/S0021364019090091
Bibliographic databases:
Document Type: Article
Language: Russian
Citation: A. V. Glushkov, A. V. Saburov, “Mass composition of cosmic rays with energies above 10$^{17}$ eV according to the data from the muon detectors of the Yakutsk EAS array”, Pis'ma v Zh. Èksper. Teoret. Fiz., 109:9 (2019), 579–583; JETP Letters, 109:9 (2019), 559–563
Citation in format AMSBIB
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    • This publication is cited in the following 12 articles:
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