Revtex4 33 pages, 16 figures and 4 tablesMuon backgrounds at Super-Kamiokande, KamLAND and CHOOZ are calculated using MUSIC. A modified version of the Gaisser sea level muon distribution and a well-tested Monte Carlo integration method are introduced. Average muon energy, flux and rate are tabulated. Plots of average energy and angular distributions are given. Implications on muon tracker design for future experiments are discussed
A dedicated cosmic muon Monte-Carlo event generator CMSCGEN has been developed for the CMS experimen...
The atmospheric muon and neutrino flux have been simulated using the same approach which successfull...
The air shower experiment KASCADE is a groundbased detector system that measures simultaneously the ...
Revtex4 33 pages, 16 figures and 4 tablesMuon backgrounds at Super-Kamiokande, KamLAND and CHOOZ are...
With a pretty good-resolution mountain profile, we simulated the underground muon background at the ...
Geant4 simulation package was used to simulate muon fluxes at different locations, the floor of UNIR...
The atmospheric muon and neutrino flux have been simulated using the same approach which successfull...
We have investigated the zenith angle distribution of muon intensities at three different depths of ...
International audienceIn this work, a water tank muon spectrometer was designed, assembled and opera...
Contribution to the 27th ICRC (Hamburg, August 7-15, 2001), 4 pages, 3 .eps figures, uses icrc.clsTh...
The atmospheric muon and neutrino flux have been calculated by a full 3-dimensional simulation. For ...
We have investigated the differential and integrated muon fluxes, muon charge ratios and the zenith ...
Underground muon intensities up to 10000 m.w.e. and angular distribution up to 6500 m.w.e. in standa...
Abstract The present work has one aim and one aim only: to increase the geological credibility of si...
The angular and energy distributions of the primary cosmic rays that are responsible for the muons r...
A dedicated cosmic muon Monte-Carlo event generator CMSCGEN has been developed for the CMS experimen...
The atmospheric muon and neutrino flux have been simulated using the same approach which successfull...
The air shower experiment KASCADE is a groundbased detector system that measures simultaneously the ...
Revtex4 33 pages, 16 figures and 4 tablesMuon backgrounds at Super-Kamiokande, KamLAND and CHOOZ are...
With a pretty good-resolution mountain profile, we simulated the underground muon background at the ...
Geant4 simulation package was used to simulate muon fluxes at different locations, the floor of UNIR...
The atmospheric muon and neutrino flux have been simulated using the same approach which successfull...
We have investigated the zenith angle distribution of muon intensities at three different depths of ...
International audienceIn this work, a water tank muon spectrometer was designed, assembled and opera...
Contribution to the 27th ICRC (Hamburg, August 7-15, 2001), 4 pages, 3 .eps figures, uses icrc.clsTh...
The atmospheric muon and neutrino flux have been calculated by a full 3-dimensional simulation. For ...
We have investigated the differential and integrated muon fluxes, muon charge ratios and the zenith ...
Underground muon intensities up to 10000 m.w.e. and angular distribution up to 6500 m.w.e. in standa...
Abstract The present work has one aim and one aim only: to increase the geological credibility of si...
The angular and energy distributions of the primary cosmic rays that are responsible for the muons r...
A dedicated cosmic muon Monte-Carlo event generator CMSCGEN has been developed for the CMS experimen...
The atmospheric muon and neutrino flux have been simulated using the same approach which successfull...
The air shower experiment KASCADE is a groundbased detector system that measures simultaneously the ...