The attenuation length of proton primaries and the proton-air inelastic cross section are studied at energies E-0 approximate to 10(15) eV by using the EAS-TOP array data. Proton initiated Extensive Air Showers, in the energy range (2 divided by 4) 10(15) eV and near maximum development, are selected from their N-mu(E-mu > 1 GeV) and N-e sizes. The experimental attenuation length Lambda(obs) is compared with those obtained from simulations, including the full detector response, based on different interaction models (HDPM, VENUS, DPMJET, QGSJET and SIBYLL) in the frame of CORSIKA code. The proton-air inelastic cross section is also inferred by using the factor k = Lambda(obs)(sim)/lambda(p-air)(sim) obtained from each interaction model
Determination of the primary particle mass using air fluorescence or a Cherenkov detector array is o...
The analysis of extensive air shower (EAS) data depends strongly on simulations of the air shower de...
The proton-air cross section in the energy range 1???100 TeV has been measured by the ARGO-YBJ cosmi...
The attenuation length of proton primaries and the proton-air inelastic cross section are studied at...
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...
We present estimation of proton-air inelastic interaction cross-section obtained for different energ...
The model dependence of the development of extensive air showers generated by high-energy cosmic-ray...
Abstract: The study of cosmic ray extensive air showers (EAS) offers a unique way to extract proton-...
Using the data taken by the ARGO-YBJ experiment (606 $g/cm^{2}$, Tibet, P.R.China) in the period of ...
First results of the measurement of the interaction cross section between primary protons and air n...
Journal ArticleWe have measured the proton-air inelastic cross section at s 1/2 = 30 TeV by observin...
Applying the recently constructed analytic representation for the pp scattering amplitudes, we prese...
Conclusions are made about the increase with energy of the inelastic proton air cross section σp−air...
In this work we are reporting on the measurement of the proton-air inelastic cross section σp-airine...
Determination of the primary particle mass using air fluorescence or a Cherenkov detector array is o...
The analysis of extensive air shower (EAS) data depends strongly on simulations of the air shower de...
The proton-air cross section in the energy range 1???100 TeV has been measured by the ARGO-YBJ cosmi...
The attenuation length of proton primaries and the proton-air inelastic cross section are studied at...
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...
We present estimation of proton-air inelastic interaction cross-section obtained for different energ...
The model dependence of the development of extensive air showers generated by high-energy cosmic-ray...
Abstract: The study of cosmic ray extensive air showers (EAS) offers a unique way to extract proton-...
Using the data taken by the ARGO-YBJ experiment (606 $g/cm^{2}$, Tibet, P.R.China) in the period of ...
First results of the measurement of the interaction cross section between primary protons and air n...
Journal ArticleWe have measured the proton-air inelastic cross section at s 1/2 = 30 TeV by observin...
Applying the recently constructed analytic representation for the pp scattering amplitudes, we prese...
Conclusions are made about the increase with energy of the inelastic proton air cross section σp−air...
In this work we are reporting on the measurement of the proton-air inelastic cross section σp-airine...
Determination of the primary particle mass using air fluorescence or a Cherenkov detector array is o...
The analysis of extensive air shower (EAS) data depends strongly on simulations of the air shower de...
The proton-air cross section in the energy range 1???100 TeV has been measured by the ARGO-YBJ cosmi...