The distribution of the maxima of high energy cosmic ray induced extensive air showers in the atmosphere was measured as a function of atmospheric depth. From the exponential tail of this distribution, it was determined that the proton-air inelastic cross section at 30 TeV center-of-mass energy to be 540 + or - 40mb
p. 1-9We report a measurement of the proton-air cross section for particle production at the center-...
The extensive air showers (EAS) cascade curves from the Cerenkov light lateral distribution measurem...
The increasing cosmic ray statistics collected by present experiments and the future prospects with ...
We present measurements of the depth of maximum for extensive air showers (EAS) produced by cosmic r...
More than 3000 extensive air showers with energies above 1018 eV were observed in stereo mode by th...
Journal ArticleWe have measured the proton-air inelastic cross section at s 1/2 = 30 TeV by observin...
The longitudinal shower development of extensive air showers (EAS) observed in the fly's eye is used...
Ultrahigh energy cosmic rays provide the highest known energy source in the Universe to measure prot...
Ultra high energy cosmic rays provide the highest known energy source in the universe to measure pro...
Ultrahigh energy cosmic rays provide the highest known energy source in the Universe to measure prot...
In this paper, we will discuss the prospects of deducing the proton-air cross section from fluoresce...
The model dependence of the development of extensive air showers generated by high-energy cosmic-ray...
We describe the measurement of the depth of maximum, X(max), of the longitudinal development of air ...
We simultaneously fit a QCD-inspired parameterization of all accelerator data on forward proton-prot...
The Fly’s Eye (FE) and the Michigan Muon Array (MA) simultaneously detect Extensive Air Showers (EAS...
p. 1-9We report a measurement of the proton-air cross section for particle production at the center-...
The extensive air showers (EAS) cascade curves from the Cerenkov light lateral distribution measurem...
The increasing cosmic ray statistics collected by present experiments and the future prospects with ...
We present measurements of the depth of maximum for extensive air showers (EAS) produced by cosmic r...
More than 3000 extensive air showers with energies above 1018 eV were observed in stereo mode by th...
Journal ArticleWe have measured the proton-air inelastic cross section at s 1/2 = 30 TeV by observin...
The longitudinal shower development of extensive air showers (EAS) observed in the fly's eye is used...
Ultrahigh energy cosmic rays provide the highest known energy source in the Universe to measure prot...
Ultra high energy cosmic rays provide the highest known energy source in the universe to measure pro...
Ultrahigh energy cosmic rays provide the highest known energy source in the Universe to measure prot...
In this paper, we will discuss the prospects of deducing the proton-air cross section from fluoresce...
The model dependence of the development of extensive air showers generated by high-energy cosmic-ray...
We describe the measurement of the depth of maximum, X(max), of the longitudinal development of air ...
We simultaneously fit a QCD-inspired parameterization of all accelerator data on forward proton-prot...
The Fly’s Eye (FE) and the Michigan Muon Array (MA) simultaneously detect Extensive Air Showers (EAS...
p. 1-9We report a measurement of the proton-air cross section for particle production at the center-...
The extensive air showers (EAS) cascade curves from the Cerenkov light lateral distribution measurem...
The increasing cosmic ray statistics collected by present experiments and the future prospects with ...