摘要
地下多μ现象的观测是研究“膝”区(1015—1016eV)宇宙线成分的一种重要方法.现有的地下探测器对于成分研究不甚理想,因为它们原本主要是为其它目的而设计的.我们提出一种新的途径:用一个探测器陈列在浅层地下观测多μ事例.这一方法对成分研究具有较高的灵敏度.
The observation of underground multimuon phenomena is an important way for the study of the cosmic ray composition in the 'knee' region (1015-1016 eV). It is noticed that the existing underground detectors are not very ideal for the composihon study because they were originally designed mainly for other aims. A new approach having higher sensitivity for this study by observing multimuon events using a detector array in a shallower depth underground is presented.
出处
《高能物理与核物理》
CSCD
北大核心
1999年第6期584-588,共5页
High Energy Physics and Nuclear Physics
关键词
宇宙线成分
“膝”区
地下多μ现象
探测器
cosmic ray composition, ‘knee' region, underground multimuon phenomena