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- W2736684719 abstract "The evolution of the muon content of very high energy air showers (EAS) in the atmosphere is investigated with data of the KASCADE-Grande observatory. For this purpose, the muon attenuation length in the atmosphere is obtained to $Lambda_mu = 1256 , pm 85 , ^{+229}_{-232}(mbox{syst}), mbox{g/cm}^2$ from the experimental data for shower energies between $10^{16.3}$ and $10^{17.0} , mbox{eV}$. Comparison of this quantity with predictions of the high-energy hadronic interaction models QGSJET-II-02, SIBYLL 2.1, QGSJET-II-04 and EPOS-LHC reveals that the attenuation of the muon content of measured EAS in the atmosphere is lower than predicted. Deviations are, however, less significant with the post-LHC models. The presence of such deviations seems to be related to a difference between the simulated and the measured zenith angle evolutions of the lateral muon density distributions of EAS, which also causes a discrepancy between the measured absorption lengths of the density of shower muons and the predicted ones at large distances from the EAS core. The studied deficiencies show that all four considered hadronic interaction models fail to describe consistently the zenith angle evolution of the muon content of EAS in the aforesaid energy regime." @default.
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- W2736684719 date "2017-10-01" @default.
- W2736684719 modified "2023-10-05" @default.
- W2736684719 title "Probing the evolution of the EAS muon content in the atmosphere with KASCADE-Grande" @default.
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- W2736684719 cites W2023302165 @default.
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- W2736684719 cites W2080353696 @default.
- W2736684719 cites W2081694213 @default.
- W2736684719 cites W2083055131 @default.
- W2736684719 cites W2085832497 @default.
- W2736684719 cites W2092740067 @default.
- W2736684719 cites W2099375436 @default.
- W2736684719 cites W2100094352 @default.
- W2736684719 cites W2117086324 @default.
- W2736684719 cites W2119592578 @default.
- W2736684719 cites W2125194998 @default.
- W2736684719 cites W2125245607 @default.
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- W2736684719 cites W2131388739 @default.
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- W2736684719 doi "https://doi.org/10.1016/j.astropartphys.2017.07.001" @default.
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