The cosmic rays (CR) at sea level comprise particles from the extensive air showers (EAS). Their major components are muons, which are the decay products of pions or kaons from high altitudes. Despite a lifetime of only about 2 µs, muons can penetrate the atmosphere down to the sea level before they decay because of the relativistic time dilation effect. When muons travel through the atmosphere, they lose their energy by the proces
Cosmic ray intensity variations of primary origin and those caused by meteorological changes appear ...
The atmospheric effects on the muon intensity have been observed using muon telescopes at Poatina, C...
The angular and energy distributions of the primary cosmic rays that are responsible for the muons r...
The day-night variation of cosmic rays intensity at sea level has been observed by a simple G-M coun...
A Study of Cosmic Rays Cosmic rays are a form of radiation associated with a group of elementary par...
Angular distribution of cosmic-ray muons at sea level has been investigated using the Geant4 simulat...
Cosmic rays are highly energetic particles which are produced by a variety of interstellar sources. ...
The absolute directional differential intensities of high-energy cosmic ray muons near sea level hav...
High energy particles from deep space are constantly raining down on the earth’s upper atmosphere. ...
The temperature of the upper atmosphere affects the height of primary cosmic ray interactions and th...
Cosmic rays are charged particles whose flux observed at Earth shows temporal variations related to ...
The recently proposed new process for energetic-muon production in the atmosphere should be tested a...
International audienceIn this work, a portable cosmic-ray telescope was designed, assembled and oper...
The rate of low energy ( 150 MeV) cosmic ray muons was measured at ground level as a function of sev...
Distributions of secondary muons at sea level from cosmic gamma rays below 10 Te
Cosmic ray intensity variations of primary origin and those caused by meteorological changes appear ...
The atmospheric effects on the muon intensity have been observed using muon telescopes at Poatina, C...
The angular and energy distributions of the primary cosmic rays that are responsible for the muons r...
The day-night variation of cosmic rays intensity at sea level has been observed by a simple G-M coun...
A Study of Cosmic Rays Cosmic rays are a form of radiation associated with a group of elementary par...
Angular distribution of cosmic-ray muons at sea level has been investigated using the Geant4 simulat...
Cosmic rays are highly energetic particles which are produced by a variety of interstellar sources. ...
The absolute directional differential intensities of high-energy cosmic ray muons near sea level hav...
High energy particles from deep space are constantly raining down on the earth’s upper atmosphere. ...
The temperature of the upper atmosphere affects the height of primary cosmic ray interactions and th...
Cosmic rays are charged particles whose flux observed at Earth shows temporal variations related to ...
The recently proposed new process for energetic-muon production in the atmosphere should be tested a...
International audienceIn this work, a portable cosmic-ray telescope was designed, assembled and oper...
The rate of low energy ( 150 MeV) cosmic ray muons was measured at ground level as a function of sev...
Distributions of secondary muons at sea level from cosmic gamma rays below 10 Te
Cosmic ray intensity variations of primary origin and those caused by meteorological changes appear ...
The atmospheric effects on the muon intensity have been observed using muon telescopes at Poatina, C...
The angular and energy distributions of the primary cosmic rays that are responsible for the muons r...