The ARGO-YBJ detector, located at high altitude in the Cosmic Ray Observatory of YangBaJing in Tibet (4300 m asl, about 600 g/cm2 of atmospheric depth) provides the opportunity for the study, with unprecedented resolution, of cosmic ray physics in the primary energy region between 10^12 and 10^16 eV. Preliminary results of the measurements of the all-particle and light-component (i.e. protons and helium) energy spectra between approximately 5 TeV and 5 PeV are reported and discussed
The ARGO-YBJ experiment, located at the Yangbajing Cosmic Ray Laboratory (Tibet, 4300 m a.s.l., 606 ...
The ARGO–YBJ experiment is a full-coverage air shower detector located at the Yangbajing Cosmic Ray...
The ARGO-YBJ experiment detects extensive air showers in a wide energy range by means of a full-cove...
The ARGO-YBJ detector, located at high altitude in the Cosmic Ray Observatory of Yangbajing in Tibet...
The ARGO-YBJ detector, located at high altitude in the Cosmic Ray Observatory of Yangbajing in Tibet...
The ARGO-YBJ experiment has been in stable data taking for more than five years at the Yangbajing co...
The ARGO-YBJ experiment has been in full and stable data taking at the Yangbajing cosmic ray observa...
The ARGO-YBJ experiment is a full-coverage air shower detector operating at the Yangbajing Internati...
Cosmic rayphysics in the 10^12–10^15 eV primary energy range is among themain scientific goals of th...
The study of cosmic ray physic of 1012-1015 primary cosmic energy is one of the main goals of ARGO-Y...
""Cosmic ray physics in the 10121015 eV primary energy range is among the main scientific goals of t...
The ARGO-YBJ experiment, located in the Yangbajing Cosmic Ray observatory (4300 m a.s.l. Tibet, P.R....
The energy spectrum and composition of Cosmic Rays (CR) play an important role in the understanding ...
The study of cosmic rays physic of 1012 -1015 primary cosmic energy is one of the main goals of ARGO...
The ARGO-YBJ experiment is a full-coverage air shower detector located at the Yangbajing Cosmic Ray ...
The ARGO-YBJ experiment, located at the Yangbajing Cosmic Ray Laboratory (Tibet, 4300 m a.s.l., 606 ...
The ARGO–YBJ experiment is a full-coverage air shower detector located at the Yangbajing Cosmic Ray...
The ARGO-YBJ experiment detects extensive air showers in a wide energy range by means of a full-cove...
The ARGO-YBJ detector, located at high altitude in the Cosmic Ray Observatory of Yangbajing in Tibet...
The ARGO-YBJ detector, located at high altitude in the Cosmic Ray Observatory of Yangbajing in Tibet...
The ARGO-YBJ experiment has been in stable data taking for more than five years at the Yangbajing co...
The ARGO-YBJ experiment has been in full and stable data taking at the Yangbajing cosmic ray observa...
The ARGO-YBJ experiment is a full-coverage air shower detector operating at the Yangbajing Internati...
Cosmic rayphysics in the 10^12–10^15 eV primary energy range is among themain scientific goals of th...
The study of cosmic ray physic of 1012-1015 primary cosmic energy is one of the main goals of ARGO-Y...
""Cosmic ray physics in the 10121015 eV primary energy range is among the main scientific goals of t...
The ARGO-YBJ experiment, located in the Yangbajing Cosmic Ray observatory (4300 m a.s.l. Tibet, P.R....
The energy spectrum and composition of Cosmic Rays (CR) play an important role in the understanding ...
The study of cosmic rays physic of 1012 -1015 primary cosmic energy is one of the main goals of ARGO...
The ARGO-YBJ experiment is a full-coverage air shower detector located at the Yangbajing Cosmic Ray ...
The ARGO-YBJ experiment, located at the Yangbajing Cosmic Ray Laboratory (Tibet, 4300 m a.s.l., 606 ...
The ARGO–YBJ experiment is a full-coverage air shower detector located at the Yangbajing Cosmic Ray...
The ARGO-YBJ experiment detects extensive air showers in a wide energy range by means of a full-cove...