Add to ORKGThe primary cosmic ray proton, helium and CNO fluxes in the energy range 80-300 TeV are studied at the Na- tional Gran Sasso Laboratories by means of EAS-TOP and MACRO detectors. Proton and helium (’p+He’) and proton, helium and CNO (’p+He+CNO’) primaries are selected at 80 TeV, and at 250 TeV respec- tively. Results of this measurement have been interpreted using three different interaction models (QGSJET, SYBILL and DPMJET) inside the CORSIKA framework. Results using all interaction models show a domi- nance of the helium component in the 80-300 TeV region
The primary cosmic ray (CR) proton, helium and CNO fluxes in the energy range 80–300 TeV are studied...
The primary cosmic ray (CR) proton, helium and CNO fluxes in the energy range 80-300 TeV are studied...
The primary cosmic ray (CR) proton, helium and CNO fluxes in the energy range 80–300 TeV are studied...
The primary cosmic ray proton, helium and CNO fluxes in the energy range 80-300 TeV are studied at t...
The primary cosmic ray (CR) proton, helium and CNO fluxes in the energy range 80–300 TeV are studied...
The primary cosmic ray (CR) proton, helium and CNO fluxes in the energy range 80-300 TeV are studied...
The primary cosmic ray (CR) proton, helium and CNO fluxes in the energy range 80–300 TeV are studied...
The primary cosmic ray proton, helium and CNO fluxes in the energy range 80-300 TeV are studied at t...
The primary cosmic ray (CR) proton, helium and CNO fluxes in the energy range 80–300 TeV are studied...
The primary cosmic ray (CR) proton, helium and CNO fluxes in the energy range 80-300 TeV are studied...
The primary cosmic ray (CR) proton, helium and CNO fluxes in the energy range 80–300 TeV are studied...