Performance of a scintillation detector array operated with LHAASO-KM2A electronics

Performance of a scintillation detector array operated with LHAASO-KM2A electronics
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使用 LHAASO-KM2A 电子设备操作的闪烁探测器阵列的性能

DOI:
10.1007/s10686-018-9588-z
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发表时间:
2018-04
影响因子:
3
通讯作者:
Y
Y
中科院分区:
物理与天体物理4区
文献类型:
--
作者:
Wang Zhen;Guo Yiqing;Cai Hui;Chang Jinfan;Chen Tianlu;Danzengluobu;Feng Youliang;Gao Qi;Gou Quanbu;Guo Yingying;Hou Chao;Hu Hongbo;Labaciren;Liu Cheng;Li Haijin;Liu Jia;Liu Maoyuan;Qiao Bingqiang;Qian Xiangli;Sheng Xiangdong;Tian Zhen;Wang Qun;Xue Liang;Y

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2016年底,羊八井国际宇宙线观测站安装了一个由115个探测器组成的闪烁探测器阵列,面积约为20000 m2,并从那时起一直在采集数据。该阵列配备了大型高海拔空气簇射天文台平方公里复合阵列(LHAASO-KM 2A)的电子设备,目前是LHAASO-KM 2A最大的调试和测试平台。此外,该阵列被用来研究一个宽视场的空气切伦科夫望远镜的性能,提供准确的信息,簇射的核心,方向和能量等,这项工作主要是处理闪烁探测器阵列。详细描述了实验装置和离线标定。然后,将数据与蒙特卡罗(MC)模拟进行了彻底的比较,并获得了良好的一致性。采用奇偶法测量了簇射方向和核心的分辨率。最后,对预期的月球和太阳的宇宙射线阴影(CR)的成功观测验证了测量的角分辨率。
A scintillation detector array composed of 115 detectors and covering an area of about 20000 m2was installed at the end of 2016 at the Yangbajing international cosmic ray observatory and has been taking data since then. The array is equipped with electronics from Large High Altitude Air Shower Observatory Square Kilometer Complex Array (LHAASO-KM2A) and, in turn, currently serves as the largest debugging and testing platform for the LHAASO-KM2A. Furthermore, the array was used to study the performance of a wide field-of-view air Cherenkov telescope by providing accurate information on the shower core, direction and energy, etc. This work is mainly dealing with the scintillation detector array. The experimental setup and the offline calibration are described in detail. Then, a thorough comparison between the data and Monte Carlo (MC) simulations is presented and a good agreement is obtained. With the even-odd method, the resolutions of the shower direction and core are measured. Finally, successful observations of the expected Moon’s and Sun’s shadows of cosmic rays (CRs) verify the measured angular resolution.
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