The Pierre Auger Observatory: Perspectives on ultra-high energy cosmic rays

Atmospheric aerosols at the Pierre Auger Observatory : characterization and effect on the energy estimation for ultra-high energy cosmic rays... 1.2 Extensive

VEM-peak and C is a scale factor obtained from Monte Carlo simulation of the shower development [56]. In the present section, an effort is made to quantify the

The Pierre Auger Collaboration has measured the proton-air cross-section, σ p−air , for particle production at ultra-high energies using hybrid data1. This cross-section is

After presenting the Southern Auger site and its current status, we will describe the recent Auger results on the anisotropy studies, and the first estimate of the UHECR spectrum..

Pierre Auger Collaboration (2019), Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory. Pierre

L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des

L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des

In the full Monte Carlo approach, because of the systematic uncertainties and the lack of knowledge of the mass composition of cosmic rays in this energy range, the spectrum has