Add to ORKGSpectrum of cascades generated by cosmic ray muons underground is presented. The mean zenith angle of the muon arrival is theta=35 deg the depth approx. 1000 hg/sq cm. In cascades energy range 700 GeV the measured spectrum is in agreement with the sea-level integral muon spectrum index gamma=3.0. Some decrease of this exponent has been found in the range 4000 Gev
A muon telescope based on 8 water cherenkov detectors was mounted at Basic Environmental Observatory...
Measurements of cosmogenic particles at various locations and altitudes are becoming increasingly im...
Multiplicity spectrum of muon bundles underground, with Eμ ≥ few × 100 GeV, is an effective tool for...
A new method to estimate the mean atomic number of primary cosmic rays in energy range 10 to the 3rd...
The energy spectrum of cascade showers induced by electromagnetic interactions of high energy muons ...
The overall data from the investigation of the cosmic ray muon flux in the range of zenith angles (0...
The multiplicity spectrum of muon showers has been observed at depths of 1400-3400 hg/cm2 undergroun...
The final analysis of the data obtained by the Sydney University Giant Airshower Recorder (SUGAR) is...
The data on muon groups observed at Baksan underground scintillation telescope is analyzed. In this ...
Muon energy spectra and muon lateral distribution in EAS were investigated with the underground magn...
The neutrino experiment at the Baksan Underground Scintillation Telescope is operating for 35 years....
Energy spectra and angular distribution data on generation and interaction of high energy muons with...
High-statistics data on near-horizontal muons collected with Russian-Italian coordinate detector DEC...
An experimental investigation of high energy muons above 200 GeV in extensive air showers has been m...
Typescript (photocopy).An investigation of scintillations in ground-level cosmic ray muons has been ...
A muon telescope based on 8 water cherenkov detectors was mounted at Basic Environmental Observatory...
Measurements of cosmogenic particles at various locations and altitudes are becoming increasingly im...
Multiplicity spectrum of muon bundles underground, with Eμ ≥ few × 100 GeV, is an effective tool for...
A new method to estimate the mean atomic number of primary cosmic rays in energy range 10 to the 3rd...
The energy spectrum of cascade showers induced by electromagnetic interactions of high energy muons ...
The overall data from the investigation of the cosmic ray muon flux in the range of zenith angles (0...
The multiplicity spectrum of muon showers has been observed at depths of 1400-3400 hg/cm2 undergroun...
The final analysis of the data obtained by the Sydney University Giant Airshower Recorder (SUGAR) is...
The data on muon groups observed at Baksan underground scintillation telescope is analyzed. In this ...
Muon energy spectra and muon lateral distribution in EAS were investigated with the underground magn...
The neutrino experiment at the Baksan Underground Scintillation Telescope is operating for 35 years....
Energy spectra and angular distribution data on generation and interaction of high energy muons with...
High-statistics data on near-horizontal muons collected with Russian-Italian coordinate detector DEC...
An experimental investigation of high energy muons above 200 GeV in extensive air showers has been m...
Typescript (photocopy).An investigation of scintillations in ground-level cosmic ray muons has been ...
A muon telescope based on 8 water cherenkov detectors was mounted at Basic Environmental Observatory...
Measurements of cosmogenic particles at various locations and altitudes are becoming increasingly im...
Multiplicity spectrum of muon bundles underground, with Eμ ≥ few × 100 GeV, is an effective tool for...