中意合作西藏羊八井ARGO-YBJ实验成果概览  

Overview of the Results from ARGO-YBJ Experiment

作　　者：单增罗布[1] 刘茂元[1] 陈天禄[1] 厉海金[1] 宁长春[1] 胡海冰[1] 袁爱芳[1] 雷文华[1] 次仁尼玛[1] 扎西桑珠[1] 丁晓红[1] 扎西次仁[1] 拉巴次仁[1] 孟宪茹[1] 

机构地区：[1]西藏大学宇宙线教育部重点实验室,西藏拉萨850000

出　　处：《西藏大学学报（社会科学版）》2011年第6期17-22,共6页Journal of Tibet University

摘　　要：文章简要介绍了中意合作西藏羊八井ARGO-YBJ宇宙线观测实验的物理目标和探测原理,重点概述了ARGO-YBJ阵列自2007年稳定运行以来在宇宙线实验观测中取得的重要成果,如甚高能γ点源、大尺度各向异性、宇宙线月亮阴影效应和全粒子谱等。In the Current paper,an introduction of the physical experimental goals and detecting the principles of Sino-Italy cooperated Yangbajing ARGO-YBJ Cosmic Ray Observatory in Tibet was given briefly and specially focused on important results of ARGO-YBJ array,such as very High energy γ point sources,large-scale anisotropy,cosmic ray moon shadow effect and the whole particle spectrum,since it has operated stably from year 2007.

关 键 词：宇宙线 γ天文 ARGO-YBJ 

分 类 号：O572.212[理学—粒子物理与原子核物理]