Influence of hadronic interaction models and the cosmic ray spectrum on the high energy atmospheric muon and neutrino fluxJan 1, 2012·Anatoli Fedynitch,Julia Becker Tjus,Paolo Desiati· 0 min read Cite DOI URLTypeJournal articlePublicationPhysical Review D - Particles, Fields, Gravitation and CosmologyLast updated on Jan 1, 2012 ← Cosmic rays and stochastic magnetic reconnection in the heliotail Jan 1, 2012Magnetic reconnection as the cause of cosmic ray excess from the heliospheric tail Jan 1, 2012 →