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Energy and zenith angle dependence of atmospheric muons
The recently proposed new process for energetic-muon production in the atmosphere should be tested at Mt. Chacaltaya. Rigorous calculations of zenith-angle distribution of atmospheric muons have been made for the altitude of 5200 m above sea level with energy range from 100 GeV to 100 TeV and for ze...
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| Lenguaje: | eng |
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1973
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| Acceso en línea: | https://dx.doi.org/10.1002/prop.19730210302 http://cds.cern.ch/record/880731 |