The proton-air inelastic cross section (σp-airinel) is measured at √s≈2 TeV at the EAS-TOP extensive air shower experiment by studying the absorption length of cosmic ray proton primaries cascades reaching the maximum development at the observation level. Primary energies, in the region E0=(1.5÷2.5)·10(15 ) eV, are selected through the EAS muon number (Nμ), and proton originated cascades at maximum development are selected by means of the shower size (Ne). The observed absorption length (λobs) is a convolution of the proton-air interaction length (λp-air) and of the shower and detector fluctuations. The conversion factor k=λobs/λint is obtained by means of simulations performed with the CORSIKA code and the QGSJET II and SIBYLL interaction...
We present estimation of proton-air inelastic interaction cross-section obtained for different energ...
Cosmic ray data may allow the determination of the proton-air cross section at ultra-high energy. Fo...
Determination of the primary particle mass using air fluorescence or a Cherenkov detector array is o...
The proton-air inelastic cross section (σp-airinel) is measured at √s≈2 TeV at the EAS-TOP extensiv...
The proton-air inelastic cross section (σp-airinel) is measured at s≈2TeV at the EAS-TOP extensive a...
The attenuation length of proton primaries and the proton-air inelastic cross section are studied at...
Abstract: The study of cosmic ray extensive air showers (EAS) offers a unique way to extract proton-...
Detecting Ultra High Energy Cosmic Rays (UHECRs) enables us to measure the proton-air inelastic cros...
In this work we are reporting on the measurement of the proton-air inelastic cross section σp-airine...
Ultrahigh energy cosmic rays provide the highest known energy source in the Universe to measure prot...
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...
Conclusions are made about the increase with energy of the inelastic proton air cross section σp−air...
Journal ArticleWe have measured the proton-air inelastic cross section at s 1/2 = 30 TeV by observin...
The model dependence of the development of extensive air showers generated by high-energy cosmic-ray...
We present estimation of proton-air inelastic interaction cross-section obtained for different energ...
Cosmic ray data may allow the determination of the proton-air cross section at ultra-high energy. Fo...
Determination of the primary particle mass using air fluorescence or a Cherenkov detector array is o...
The proton-air inelastic cross section (σp-airinel) is measured at √s≈2 TeV at the EAS-TOP extensiv...
The proton-air inelastic cross section (σp-airinel) is measured at s≈2TeV at the EAS-TOP extensive a...
The attenuation length of proton primaries and the proton-air inelastic cross section are studied at...
Abstract: The study of cosmic ray extensive air showers (EAS) offers a unique way to extract proton-...
Detecting Ultra High Energy Cosmic Rays (UHECRs) enables us to measure the proton-air inelastic cros...
In this work we are reporting on the measurement of the proton-air inelastic cross section σp-airine...
Ultrahigh energy cosmic rays provide the highest known energy source in the Universe to measure prot...
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...
Conclusions are made about the increase with energy of the inelastic proton air cross section σp−air...
Journal ArticleWe have measured the proton-air inelastic cross section at s 1/2 = 30 TeV by observin...
The model dependence of the development of extensive air showers generated by high-energy cosmic-ray...
We present estimation of proton-air inelastic interaction cross-section obtained for different energ...
Cosmic ray data may allow the determination of the proton-air cross section at ultra-high energy. Fo...
Determination of the primary particle mass using air fluorescence or a Cherenkov detector array is o...