We present a measurement of the most probable cosmic muon energy at near sea level using a two-paddle cosmic ray detector. Muon rates at two different elevations (27 and 326 m) were measured. Data were collected for 2-3 h for each data set at 1 min intervals in the afternoon of successive days. Muon counts were extracted from a Gaussian fit to the distributions of both sets. Despite the fact that only a limited amount of data were collected and measurements were performed at relatively close altitudes, we observed good agreement between the 2.28 +/- 0.21 GeV energy measured in this work and the value of 2 GeV that is reported in the literature
The ALEPH detector at LEP has been used to measure the momentum spectrum and charge ratio of vertica...
One of the uncertainties in the interpretation of ultrahigh energy cosmic ray data comes from the ha...
We have measured directly the residual energy of cosmic ray muons crossing the MACRO detector at the...
Typescript (photocopy).An investigation of scintillations in ground-level cosmic ray muons has been ...
The absolute directional differential intensities of high-energy cosmic ray muons near sea level hav...
Angular distribution of cosmic-ray muons at sea level has been investigated using the Geant4 simulat...
The absolute intensities of cosmic ray muons in the vertical direction and at several large zenith a...
We have determined the momentum spectrum and charge ratio of muons in the region from 250 MeV/c to 1...
International audienceIn this work, a portable cosmic-ray telescope was designed, assembled and oper...
The angular and energy distributions of the primary cosmic rays that are responsible for the muons r...
International audienceIn this work, a water tank muon spectrometer was designed, assembled and opera...
Abstract: A review of measurements of the high muon energy spectra for altitudes close to the sea le...
The vertical muon intensity measured with MACRO at the Gran Sasso Laboratory, in the depth range 320...
High energy particles from deep space are constantly raining down on the earth’s upper atmosphere. ...
The charge ratio of sea level muons has been estimated from the new scaling variable model and the C...
The ALEPH detector at LEP has been used to measure the momentum spectrum and charge ratio of vertica...
One of the uncertainties in the interpretation of ultrahigh energy cosmic ray data comes from the ha...
We have measured directly the residual energy of cosmic ray muons crossing the MACRO detector at the...
Typescript (photocopy).An investigation of scintillations in ground-level cosmic ray muons has been ...
The absolute directional differential intensities of high-energy cosmic ray muons near sea level hav...
Angular distribution of cosmic-ray muons at sea level has been investigated using the Geant4 simulat...
The absolute intensities of cosmic ray muons in the vertical direction and at several large zenith a...
We have determined the momentum spectrum and charge ratio of muons in the region from 250 MeV/c to 1...
International audienceIn this work, a portable cosmic-ray telescope was designed, assembled and oper...
The angular and energy distributions of the primary cosmic rays that are responsible for the muons r...
International audienceIn this work, a water tank muon spectrometer was designed, assembled and opera...
Abstract: A review of measurements of the high muon energy spectra for altitudes close to the sea le...
The vertical muon intensity measured with MACRO at the Gran Sasso Laboratory, in the depth range 320...
High energy particles from deep space are constantly raining down on the earth’s upper atmosphere. ...
The charge ratio of sea level muons has been estimated from the new scaling variable model and the C...
The ALEPH detector at LEP has been used to measure the momentum spectrum and charge ratio of vertica...
One of the uncertainties in the interpretation of ultrahigh energy cosmic ray data comes from the ha...
We have measured directly the residual energy of cosmic ray muons crossing the MACRO detector at the...