Abstract
We present the results of our study of the temporal structure of the muon disk at the Yakutsk array in extensive air showers with primary energies E 0 ≥ 5 × 1016 eV at distances of 250–1500 m from the shower axis obtained using a large muon detector with an area of 184 m2 and a detection threshold of E μ ≈ 0.5 sec θ GeV. We have found two components with different muon disk thicknesses that require significant revisions of our view of the development of extensive air showers.
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Translated from Zhurnal Éksperimental’no\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l}\) i Teoretichesko\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l}\) Fiziki, Vol. 126, No. 1, 2004, pp. 5–13.
Original Russian Text Copyright © 2004 by Glushkov, Dedenko, Pravdin, Sleptsov.
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Glushkov, A.V., Dedenko, L.G., Pravdin, M.I. et al. Spatio-temporal structure of the muon disk at E 0 ≥ 5 × 1016 eV from Yakutsk EAS array data. J. Exp. Theor. Phys. 99, 1–8 (2004). https://doi.org/10.1134/1.1787072
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DOI: https://doi.org/10.1134/1.1787072