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Fomin, Yu.A.; Kalmykov, N.N.; Karpikov, I.S.; Kulikov, G.V.; Kuznetsov, M.Yu; Rubtsov, G.I.; Sulakov, V.P.; Troitsky, S.V.
Astroparticle physics, June 2017, 2017-06-00, Volume: 92Journal Article
Some discrepancies have been reported between observed and simulated muon content of extensive air showers: the number of observed muons exceeded the expectations in HiRes-MIA, Yakutsk and Pierre Auger Observatory data. Here, we analyze the data of the Moscow State University Extensive Air Shower (EAS–MSU) array on Eμ ≳ 10 GeV muons in showers caused by ∼(1017−1018) eV primary particles and demonstrate that they agree with simulations (QGSJET-II-04 hadronic interaction model) once the primary composition inferred from the surface-detector data is assumed.
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