摘要
仔细分析了近年来怀柔广延大气簇射阵列记录的65万个大气簇射事例,得到了簇射Size(即荷电总粒子数)谱和1015-5×1016eV能段的初级宇宙线微分能谱。此谱呈明显的、平滑过渡的“膝”样结构,拐点在3×1015eV附近.除了“膝”较平滑不象明野谱那样尖锐拐折而外,怀柔谱在绝对流强和“膝”的位置上都与日本明野组吻合得很好.在银河磁场刚度截止模型框架下,怀柔实验Size谱界定的宇宙线质子谱拐折能量Ec的取值范围在160到240TeV之间.
thousands of EAS events recorded by Huairou EAS Array have been analysed carefully. The Size spectrum and primary energy spectrum in the region from 1015 to 1016eV are obtained. The energy spectrum shows a clear and smooth 'Knee' structure around 3×1015eV. Except the smooth steep feature of 'Knee', it is consistent very well with Akeno spectrum. Under the assumption of so-called rigidity dependent cut model, by adjusting the breaking energy Ec of primary proton spectrum in the Monte Carlo simulation and comparing with the experimental spectrum, we found that the proper value of Ec is in the energy range from 160 to 240TeV.
出处
《高能物理与核物理》
CSCD
北大核心
1995年第9期769-774,共6页
High Energy Physics and Nuclear Physics
关键词
宇宙线
广延
大气簇射
EAS阵列
膝区
cosmic ray
extensive air shower (EAS)
EAS array
shower size
energy spectrum of primary cosmic ray
'Knee' structure.