Underground muon intensities up to 10000 m.w.e. and angular distribution up to 6500 m.w.e. in standard rock have been investigated using Geant4 simulation package. Muons with energies above 100 GeV were distributed from the ground level taking into account the muon charge ratio of ∼1.3 at sea level. The simulated differential muon intensities are in good agreement with the intensities given in the literature. Furthermore, the simulation results for the integrated intensities are consistent with the experimental data, particularly at depths above 4000 m.w.e., where the simulation gives slightly smaller intensities than the experimental ones. In addition, the simulated exponent n at different underground depths agrees well with the experiment...
Underground muon events detected by the MACRO experiment at Gran Sasso have been studied for differe...
The multiplicity spectrum of muon showers has been observed at depths of 1400-3400 hg/cm2 undergroun...
The angular and energy distributions of the primary cosmic rays that are responsible for the muons r...
Underground muon intensities up to 10000 m.w.e. and angular distribution up to 6500 m.w.e. in standa...
Recent measurements of the intensity of muons below 3000 m.w.e. (metres water equivalent) undergroun...
We have investigated the zenith angle distribution of muon intensities at three different depths of ...
The vertical underground muon intensity has been measured in the slant depth range 3200-7000 hg cm(-...
The intensity of narrow muon groups observed in Kolar Gold Field (KGF) at the depth of 3375 m.w.e. w...
With a pretty good-resolution mountain profile, we simulated the underground muon background at the ...
The cosmic ray data on vertical intensity versus depth below 10 to the 5th power g sq cm is fitted t...
The vertical sea-level muon spectrum at energies above 1 GeV and the underground/underwater muon int...
The present study is based on the sample of about 3 mln single muons observed by LVD at underground ...
We report data taken by the LVD Experiment during a live-time period of 11 556 h. We have measured t...
The vertical underground muon intensity has been measured in the slant depth range 3200-7000 hg cm(-...
A telescope of area 4 m2, consisting of horizontal layers of plastic scintillators, neon flash tubes...
Underground muon events detected by the MACRO experiment at Gran Sasso have been studied for differe...
The multiplicity spectrum of muon showers has been observed at depths of 1400-3400 hg/cm2 undergroun...
The angular and energy distributions of the primary cosmic rays that are responsible for the muons r...
Underground muon intensities up to 10000 m.w.e. and angular distribution up to 6500 m.w.e. in standa...
Recent measurements of the intensity of muons below 3000 m.w.e. (metres water equivalent) undergroun...
We have investigated the zenith angle distribution of muon intensities at three different depths of ...
The vertical underground muon intensity has been measured in the slant depth range 3200-7000 hg cm(-...
The intensity of narrow muon groups observed in Kolar Gold Field (KGF) at the depth of 3375 m.w.e. w...
With a pretty good-resolution mountain profile, we simulated the underground muon background at the ...
The cosmic ray data on vertical intensity versus depth below 10 to the 5th power g sq cm is fitted t...
The vertical sea-level muon spectrum at energies above 1 GeV and the underground/underwater muon int...
The present study is based on the sample of about 3 mln single muons observed by LVD at underground ...
We report data taken by the LVD Experiment during a live-time period of 11 556 h. We have measured t...
The vertical underground muon intensity has been measured in the slant depth range 3200-7000 hg cm(-...
A telescope of area 4 m2, consisting of horizontal layers of plastic scintillators, neon flash tubes...
Underground muon events detected by the MACRO experiment at Gran Sasso have been studied for differe...
The multiplicity spectrum of muon showers has been observed at depths of 1400-3400 hg/cm2 undergroun...
The angular and energy distributions of the primary cosmic rays that are responsible for the muons r...