Add to ORKGContribution to the 27th ICRC (Hamburg, August 7-15, 2001), 4 pages, 3 .eps figures, uses icrc.clsThe analytical expression for integral energy spectra and zenith angle distributions of atmospheric muons at large depths is derived. Fluctuations of muon energy losses are described using the parametrized correction factor. The fitting formula for the sea level muon spectrum at different zenith angles for spherical atmosphere is proposed. The concrete calculations for pure water are presented
Revtex4 33 pages, 16 figures and 4 tablesMuon backgrounds at Super-Kamiokande, KamLAND and CHOOZ are...
Distributions of secondary muons at sea level from cosmic gamma rays below 10 Te
The angular and energy distributions of the primary cosmic rays that are responsible for the muons r...
Contribution to the 27th ICRC (Hamburg, AUgust 7-15, 2001), 4 pages, 3 .eps figures, uses icrc.clsTh...
We have investigated the differential and integrated muon fluxes, muon charge ratios and the zenith ...
The recently proposed new process for energetic-muon production in the atmosphere should be tested a...
We present a review of atmospheric muon flux and energy spectrum measurements over almost six decade...
Recent measurements of the intensity of muons below 3000 m.w.e. (metres water equivalent) undergroun...
Angular distribution of cosmic-ray muons at sea level has been investigated using the Geant4 simulat...
International audienceIn this work, a water tank muon spectrometer was designed, assembled and opera...
To date, several dozens of new muon detectors have been built. When studying cosmic-ray intensity va...
The vertical sea-level muon spectrum at energies above 1 GeV and the underground/underwater muon int...
none4Atmospheric muons play an important role in underwater/ice neutrino detectors. In this paper, a...
none1noA new parameterisation of atmospheric muons deep underwater (or ice) is presented. It takes i...
Atmospheric muons play an important role in underwater/ice neutrino detectors. A parameterisation of...
Revtex4 33 pages, 16 figures and 4 tablesMuon backgrounds at Super-Kamiokande, KamLAND and CHOOZ are...
Distributions of secondary muons at sea level from cosmic gamma rays below 10 Te
The angular and energy distributions of the primary cosmic rays that are responsible for the muons r...
Contribution to the 27th ICRC (Hamburg, AUgust 7-15, 2001), 4 pages, 3 .eps figures, uses icrc.clsTh...
We have investigated the differential and integrated muon fluxes, muon charge ratios and the zenith ...
The recently proposed new process for energetic-muon production in the atmosphere should be tested a...
We present a review of atmospheric muon flux and energy spectrum measurements over almost six decade...
Recent measurements of the intensity of muons below 3000 m.w.e. (metres water equivalent) undergroun...
Angular distribution of cosmic-ray muons at sea level has been investigated using the Geant4 simulat...
International audienceIn this work, a water tank muon spectrometer was designed, assembled and opera...
To date, several dozens of new muon detectors have been built. When studying cosmic-ray intensity va...
The vertical sea-level muon spectrum at energies above 1 GeV and the underground/underwater muon int...
none4Atmospheric muons play an important role in underwater/ice neutrino detectors. In this paper, a...
none1noA new parameterisation of atmospheric muons deep underwater (or ice) is presented. It takes i...
Atmospheric muons play an important role in underwater/ice neutrino detectors. A parameterisation of...
Revtex4 33 pages, 16 figures and 4 tablesMuon backgrounds at Super-Kamiokande, KamLAND and CHOOZ are...
Distributions of secondary muons at sea level from cosmic gamma rays below 10 Te
The angular and energy distributions of the primary cosmic rays that are responsible for the muons r...