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 1012 and 1016 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 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 is a full-coverage air shower detector located at the Yangbajing Cosmic Ray ...
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...
The ARGO-YBJ detector, located at high altitude in the Cosmic Ray Observatory of Yangbajing in Tibet...
Cosmic rayphysics in the 10^12–10^15 eV primary energy range is among themain scientific goals of th...
""Cosmic ray physics in the 10121015 eV primary energy range is among the main scientific goals of t...
The energy spectrum and composition of Cosmic Rays (CR) play an important role in the understanding ...
The ARGO-YBJ experiment, located in the Yangbajing Cosmic Ray observatory (4300 m a.s.l. Tibet, P.R....
The study of cosmic ray physic of 1012-1015 primary cosmic energy is one of the main goals of ARGO-Y...
The ARGO-YBJ experiment, located at the Yangbajing Cosmic Ray Laboratory (Tibet, 4300 m a.s.l., 606 ...
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 is a full-coverage air shower detector located at the Yangbajing Cosmic Ray ...
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...
The ARGO-YBJ detector, located at high altitude in the Cosmic Ray Observatory of Yangbajing in Tibet...
Cosmic rayphysics in the 10^12–10^15 eV primary energy range is among themain scientific goals of th...
""Cosmic ray physics in the 10121015 eV primary energy range is among the main scientific goals of t...
The energy spectrum and composition of Cosmic Rays (CR) play an important role in the understanding ...
The ARGO-YBJ experiment, located in the Yangbajing Cosmic Ray observatory (4300 m a.s.l. Tibet, P.R....
The study of cosmic ray physic of 1012-1015 primary cosmic energy is one of the main goals of ARGO-Y...
The ARGO-YBJ experiment, located at the Yangbajing Cosmic Ray Laboratory (Tibet, 4300 m a.s.l., 606 ...
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 is a full-coverage air shower detector located at the Yangbajing Cosmic Ray ...