Experimental measurements of cosmic ray muon intensity deep underwater aimed at determining a muon absorption curve are of considerable interest, as they allow to reproduce independently the muon energy spectrum at sea level. The comparison of the muon absorption curve in sea water with that in rock makes it possible to determine muon energy losses caused by nuclear interactions. The data available on muon absorption in water and that in rock are not equivalent. Underground measurements are numerous and have been carried out down to the depth of approx. 15km w.e., whereas underwater muon intensity have been measured twice and only down to approx. 3km deep
The Daya Bay reactor neutrino experiment aims to determine sin2 2θ13 with a sensitivity of 0.01 or ...
Ambient light intensities at the DUMAND site, west of the island of Hawaii were measured around the ...
The present study is based on the sample of about 3 mln single muons observed by LVD at underground ...
The vertical sea-level muon spectrum at energies above 1 GeV and the underground/underwater muon int...
Registration and identification of muons and muon groups penetrating into the ocean depth, can be pe...
High energy spectra and zenith angle distributions of the atmospheric muons are calculated for the d...
We present a review of atmospheric and underground muon flux measurements. The relevance of these da...
The intensity of narrow muon groups observed in Kolar Gold Field (KGF) at the depth of 3375 m.w.e. w...
A production rate of 0.065 + or - 0.003 Ar-37 atom/kg min of K-39 at 2-mwe depth below sea level was...
A new parameterisation of atmospheric muons deep underwater (or ice) is presented. It takes into acc...
We have measured the muon flux and production rate of muon-induced neutrons at a depth of 611 m wate...
The cosmic ray data on vertical intensity versus depth below 10 to the 5th power g sq cm is fitted t...
International audienceIn this work, a water tank muon spectrometer was designed, assembled and opera...
In this work we used a particle detector and a digital oscilloscope to measure the mean life time of...
Spectrum of cascades generated by cosmic ray muons underground is presented. The mean zenith angle o...
The Daya Bay reactor neutrino experiment aims to determine sin2 2θ13 with a sensitivity of 0.01 or ...
Ambient light intensities at the DUMAND site, west of the island of Hawaii were measured around the ...
The present study is based on the sample of about 3 mln single muons observed by LVD at underground ...
The vertical sea-level muon spectrum at energies above 1 GeV and the underground/underwater muon int...
Registration and identification of muons and muon groups penetrating into the ocean depth, can be pe...
High energy spectra and zenith angle distributions of the atmospheric muons are calculated for the d...
We present a review of atmospheric and underground muon flux measurements. The relevance of these da...
The intensity of narrow muon groups observed in Kolar Gold Field (KGF) at the depth of 3375 m.w.e. w...
A production rate of 0.065 + or - 0.003 Ar-37 atom/kg min of K-39 at 2-mwe depth below sea level was...
A new parameterisation of atmospheric muons deep underwater (or ice) is presented. It takes into acc...
We have measured the muon flux and production rate of muon-induced neutrons at a depth of 611 m wate...
The cosmic ray data on vertical intensity versus depth below 10 to the 5th power g sq cm is fitted t...
International audienceIn this work, a water tank muon spectrometer was designed, assembled and opera...
In this work we used a particle detector and a digital oscilloscope to measure the mean life time of...
Spectrum of cascades generated by cosmic ray muons underground is presented. The mean zenith angle o...
The Daya Bay reactor neutrino experiment aims to determine sin2 2θ13 with a sensitivity of 0.01 or ...
Ambient light intensities at the DUMAND site, west of the island of Hawaii were measured around the ...
The present study is based on the sample of about 3 mln single muons observed by LVD at underground ...