The ARGO-YBJ experiment, located at the Yangbajing Cosmic Ray Laboratory (Tibet, 4300 m a.s.l., 606 g/cm2) has an high segmentation that allows the detection of air showers with greater detail and lower energy threshold (a few hundred GeV) compared to other EAS arrays. The spectrum of the primary Cosmic Ray light (p+He) component in the energy range ∼10 - 100 TeV is measured selecting quasi-vertical showers with the reconstructed core position located in a 40×40 m2 fiducial area. The results are compared with other measurements carried out with direct methods
The ARGO-YBJ experiment is taking data at the Yangbajing International Cosmic Rays Observatory locat...
Cosmic rayphysics in the 10^12–10^15 eV primary energy range is among themain scientific goals of th...
The energy spectrum and composition of Cosmic Rays (CR) play an important role in the understanding ...
The ARGO-YBJ experiment, located at the Yangbajing Cosmic Ray Laboratory (Tibet, 4300 m a.s.l., 606 ...
The ARGO-YBJ experiment, located at the Yangbajing Cosmic Ray Laboratory (Tibet, 4300 m a.s.l., 606 ...
The study of cosmic rays below 1015 eV is one of the main goals of the ARGO-YBJ experiment. In this ...
The study of cosmic ray physic of 1012-1015 primary cosmic energy is one of the main goals of ARGO-Y...
The study of cosmic rays physic of 1012 -1015 primary cosmic energy is one of the main goals of ARGO...
The ARGO-YBJ experiment detects extensive air showers in a wide energy range by means of a full-cove...
The ARGO-YBJ experiment has been in full and stable data taking at the Yangbajing cosmic ray observa...
The energy spectrum and composition of Cosmic Rays (CR) play an important role in the understanding ...
The combined measurement of the cosmic ray (CR) energy spectrum and anisotropy in their arrival dire...
The ARGO-YBJ detector, located at high altitude in the Cosmic Ray Observatory of YangBaJing in Tibet...
The combined measurement of the cosmic ray (CR) energy spectrum and anisotropy in their arrival dire...
The ARGO-YBJ detector, located at high altitude in the Cosmic Ray Observatory of YangBaJing in Tibet...
The ARGO-YBJ experiment is taking data at the Yangbajing International Cosmic Rays Observatory locat...
Cosmic rayphysics in the 10^12–10^15 eV primary energy range is among themain scientific goals of th...
The energy spectrum and composition of Cosmic Rays (CR) play an important role in the understanding ...
The ARGO-YBJ experiment, located at the Yangbajing Cosmic Ray Laboratory (Tibet, 4300 m a.s.l., 606 ...
The ARGO-YBJ experiment, located at the Yangbajing Cosmic Ray Laboratory (Tibet, 4300 m a.s.l., 606 ...
The study of cosmic rays below 1015 eV is one of the main goals of the ARGO-YBJ experiment. In this ...
The study of cosmic ray physic of 1012-1015 primary cosmic energy is one of the main goals of ARGO-Y...
The study of cosmic rays physic of 1012 -1015 primary cosmic energy is one of the main goals of ARGO...
The ARGO-YBJ experiment detects extensive air showers in a wide energy range by means of a full-cove...
The ARGO-YBJ experiment has been in full and stable data taking at the Yangbajing cosmic ray observa...
The energy spectrum and composition of Cosmic Rays (CR) play an important role in the understanding ...
The combined measurement of the cosmic ray (CR) energy spectrum and anisotropy in their arrival dire...
The ARGO-YBJ detector, located at high altitude in the Cosmic Ray Observatory of YangBaJing in Tibet...
The combined measurement of the cosmic ray (CR) energy spectrum and anisotropy in their arrival dire...
The ARGO-YBJ detector, located at high altitude in the Cosmic Ray Observatory of YangBaJing in Tibet...
The ARGO-YBJ experiment is taking data at the Yangbajing International Cosmic Rays Observatory locat...
Cosmic rayphysics in the 10^12–10^15 eV primary energy range is among themain scientific goals of th...
The energy spectrum and composition of Cosmic Rays (CR) play an important role in the understanding ...