Semi-analytic approximations for production of atmospheric muons and neutrinos
- 1 January 2002
- journal article
- Published by Elsevier in Astroparticle Physics
- Vol. 16 (3) , 285-294
- https://doi.org/10.1016/s0927-6505(01)00143-8
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This publication has 18 references indexed in Scilit:
- Pion production in proton collisions with light nuclei: implications for atmospheric neutrinosPhysics Letters B, 2000
- The Cosmic‐Ray Proton and Helium Spectra between 0.4 and 200 GVThe Astrophysical Journal, 1999
- Measurement of the Flux and Zenith-Angle Distribution of Upward Throughgoing Muons by Super-KamiokandePhysical Review Letters, 1999
- Path length distributions of atmospheric neutrinosPhysical Review D, 1998
- Atmospheric neutrino flux above 1 GeVPhysical Review D, 1996
- Lepton spectra in the earth's atmosphereAstroparticle Physics, 1993
- Nucleus-nucleus collisions and interpretation of cosmic-ray cascadesPhysical Review D, 1992
- Measurement of cosmic-ray proton and helium spectra during the 1987 solar minimumThe Astrophysical Journal, 1991
- Calculation of Muon yields, response functions, and sea level integral energy spectrum using recent accelerator data and Feynman scalingJournal of Geophysical Research, 1974
- Limiting Fragmentation and the Charge Ratio of Cosmic-Ray MuonsPhysical Review D, 1972