The ARGO-YBJ experiment has been in full and stable data taking at the Yangbajing cosmic ray observatory (Tibet, P.R. China, 4300 m a.s.l.) for more than five years. The detector has been designed in order to explore the Cosmic Ray (CR) spectrum in an energy range from few TeV up to several PeV. The high segmentation of the detector allows a detailed measurement of the lateral particle distribution which can be exploited on order to identify showers produced by primaries of different mass. The results of the measurement of the all-particle and proton plus helium energy spectra in the energy region between 1012 and 1016 eV are discussed
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, located at the Yangbajing Cosmic Ray Laboratory (Tibet, 4300 m a.s.l., 606 ...
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 energy spectrum and composition of Cosmic Rays (CR) play an important role in the understanding ...
The ARGO-YBJ experiment is a full-coverage air shower detector operating at the Yangbajing Internati...
The ARGO-YBJ experiment has been in stable data taking for more than five years at the Yangbajing co...
The ARGO-YBJ experiment, located in the Yangbajing Cosmic Ray observatory (4300 m a.s.l. Tibet, P.R....
The ARGO-YBJ experiment is a full-coverage air shower detector located at the Yangbajing Cosmic Ray ...
Cosmic rayphysics in the 10^12–10^15 eV primary energy range is among themain scientific goals of th...
The ARGO-YBJ detector, located at high altitude in the Cosmic Ray Observatory of Yangbajing in Tibet...
""Cosmic ray physics in the 10121015 eV primary energy range is among the main scientific goals of t...
The ARGO–YBJ experiment is a full-coverage air shower detector located at the Yangbajing Cosmic Ray...
The study of cosmic ray physic of 1012-1015 primary cosmic energy is one of the main goals of ARGO-Y...
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, located at the Yangbajing Cosmic Ray Laboratory (Tibet, 4300 m a.s.l., 606 ...
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 energy spectrum and composition of Cosmic Rays (CR) play an important role in the understanding ...
The ARGO-YBJ experiment is a full-coverage air shower detector operating at the Yangbajing Internati...
The ARGO-YBJ experiment has been in stable data taking for more than five years at the Yangbajing co...
The ARGO-YBJ experiment, located in the Yangbajing Cosmic Ray observatory (4300 m a.s.l. Tibet, P.R....
The ARGO-YBJ experiment is a full-coverage air shower detector located at the Yangbajing Cosmic Ray ...
Cosmic rayphysics in the 10^12–10^15 eV primary energy range is among themain scientific goals of th...
The ARGO-YBJ detector, located at high altitude in the Cosmic Ray Observatory of Yangbajing in Tibet...
""Cosmic ray physics in the 10121015 eV primary energy range is among the main scientific goals of t...
The ARGO–YBJ experiment is a full-coverage air shower detector located at the Yangbajing Cosmic Ray...
The study of cosmic ray physic of 1012-1015 primary cosmic energy is one of the main goals of ARGO-Y...
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, located at the Yangbajing Cosmic Ray Laboratory (Tibet, 4300 m a.s.l., 606 ...