Conveners
Parallel Session H
- Piera Luisa Ghia (LPNHE-CNRS, Paris)
Paolo Montini
(ROMA3)
01/10/2014, 17:00
oral
The ARGO-YBJ experiment is a full coverage air shower detector operated at the Yangbajing international cosmic ray observatory. The detector has been in stable data taking in its full configuration since November 2007 to February 2013. The high altitude and the high segmentation and spacetime resolution offer the possibility to explore the cosmic ray energy spectrum in a very wide range, from...
Prof.
Vasily Prosin
(Skobeltsyn Institute of Nuclear Physics of Lomonosov Moscow State University)
01/10/2014, 17:20
oral
EAS Cherenkov light array Tunka-133 with ~3 km2 geometric area operated since 2009. Five winter seasons of data acquisition (~107 triggers) and high quality of information permitted us to reconstruct primary energy spectrum and mass composition in the energy range 6•1015 to 1018 eV. This energy range is the most important for understanding of transition from Galactic to extragalactic CR. The...
Prof.
Daniele Fargion
(INFN and Dipt Fisica Sapienza)
01/10/2014, 17:50
UHECR (Ultra High Energy Cosmic Rays) are reaching a large sample of events both in the South (by AUGER) and recently also in the North terrestrial emisphere (by TA, Terrestrial Array Telescope). The latter events are showing an apparent wide Hot Spot clustering toward an unexpected area of the sky. Some tentative correlation with Ursa Major Cluster has been offered: however the remarkable...
