Abstract
Ultrahigh-energy extensive air showers detected at the Yakutsk array are analyzed. Showers different in the muon content are revealed. Four classes of showers are separated.
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V. P. Egorova, A. V. Glushkov, A. A. Ivanov, et al., Nucl. Phys. B (Proc. Suppl.) 136, 3 (2004).
N. N. Efimov, T. A. Egorov, A. V. Glushkov, et al., in Proceedings of ICRR International Symposium on Astrophysical Aspects of the Most Energetic Cosmic Rays (Kofu, 1990), p. 20.
J. N. Taylor, R. N. Manchester, and A. G. Lyne, Astrophys. J., Suppl. 88, 529 (1993).
C. I. Syrovatskiĭ, Preprint No. 151, FIAN (Physical Inst., USSR Academy of Sciences, Moscow, 1969).
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Original Russian Text © A.A. Mikhaĭlov, N.N. Efremov, E.S. Nikiforova, 2006, published in Pis’ma v Zhurnal Éksperimental’noĭ i Teoreticheskoĭ Fiziki, 2006, Vol. 83, No. 7, pp. 323–325.
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Mikhaĭlov, A.A., Efremov, N.N. & Nikiforova, E.S. Classification of ultrahigh-energy extensive air showers in terms of the muon content. Jetp Lett. 83, 265–267 (2006). https://doi.org/10.1134/S0021364006070010
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DOI: https://doi.org/10.1134/S0021364006070010