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作 者:Xin-Hua Ma Yu-Jiang Bi Zhen Cao Ming-Jun Chen Song-Zhan Chen Yao-Dong Cheng Guang-Hua Gong Min-Hao Gu Hui-Hai He Chao Hou Wen-Hao Huang Xing-Tao Huang Cheng Liu Oleg Shchegolev Xiang-Dong Sheng Yuri Stenkin Chao-Yong Wu Han-Rong Wu Sha Wu Gang Xiao Zhi-Guo Yao Shou-Shan Zhang Yi Zhang Xiong Zuo 马欣华;毕玉江;曹臻;陈明君;陈松战;程耀东;龚光华;顾旻皓;何会海;侯超;黄文昊;黄性涛;刘成;Oleg Shchegolev;盛祥东;Yuri Stenkin;吴超勇;吴含荣;武莎;肖刚;姚志国;张寿山;张毅;左雄(Key Laboratory of Particle Astrophyics&Experimental Physics Division&Computing Center,Institute of High Energy Physics,Chinese Academy of Sciences,Beijing 100049,China;TIANFU Cosmic Ray Research Center,Chengdu,Sichuan,China;University of Chinese Academy of Sciences,Beijing 100049,China;Department of Engineering Physics,Tsinghua University,Beijing 100084,China;Institute of Frontier and Interdisciplinary Science,Shandong University,Qingdao 266237,Shandong,China;Institute for Nuclear Research of Russian Academy of Sciences,Moscow 117312,Russia;Moscow Institute of Physics and Technology,Moscow 141700,Russia;Key Laboratory of Dark Matter and Space Astronomy,Purple Mountain Observatory,Chinese Academy of Sciences,Nanjing 210023,Jiangsu,China)
机构地区:[1]Key Laboratory of Particle Astrophyics&Experimental Physics Division&Computing Center,Institute of High Energy Physics,Chinese Academy of Sciences,Beijing 100049,China [2]TIANFU Cosmic Ray Research Center,Chengdu,Sichuan,China [3]University of Chinese Academy of Sciences,Beijing 100049,China [4]Department of Engineering Physics,Tsinghua University,Beijing 100084,China [5]Institute of Frontier and Interdisciplinary Science,Shandong University,Qingdao 266237,Shandong,China [6]Institute for Nuclear Research of Russian Academy of Sciences,Moscow 117312,Russia [7]Moscow Institute of Physics and Technology,Moscow 141700,Russia [8]Key Laboratory of Dark Matter and Space Astronomy,Purple Mountain Observatory,Chinese Academy of Sciences,Nanjing 210023,Jiangsu,China
出 处:《Chinese Physics C》2022年第3期1-35,共35页中国物理C(英文版)
基 金:Supported by National Natural Science Foundation in China(NSFC)(U2031103,U1831208,11805209,11775233);NSFC for Distinguished Young Scholars(12025502);the Science and Technology Department of Sichuan Province(2021YFSY0031);the International Partnership Program of Chinese Academy of Sciences(113111KYSB20170055)。
摘 要:The Large High Altitude Air Shower Observatory(LHAASO)(Fig.1)is located at Mt.Haizi(4410 m a.s.l.,600 g/cm^(2),29°21'27.56"N,100°08'19.66"E)in Daocheng,Sichuan province,P.R.China.LHAASO consists of 1.3 km^(2) array(KM2A)of electromagnetic particle detectors(ED)and muon detectors(MD),a water Cherenkov detector array(WCDA)with a total active area of 78,000 m^(2),18 wide field-of-view air Cherenkov telescopes(WFCTA)and a newly proposed electron-neutron detector array(ENDA)covering 10,000 m^(2).Each detector is synchronized with all the other through a clock synchronization network based on the White Rabbit protocol.The observatory includes an IT center which comprises the data acquisition system and trigger system,the data analysis facility.In this Chapter,all the above-mentioned components of LHAASO as well as infrastructure are described.
关 键 词:LHAASO gamma ray astronomy cosmic ray physics
分 类 号:P172.4[天文地球—天文学] O572.1[理学—粒子物理与原子核物理]
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