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A dynamic range extension system for LHAASOWCDA-1

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摘要 Purpose The main scientific goal of LHAASO-WCDA is to survey gamma-ray sources with energy from 100 GeV to 30 TeV.To observe high-energy shower events,especially to measure the energy spectrum of cosmic rays from 100 TeV to 10 PeV,a dynamic range extension system(WCDA++)is designed to use a 1.5-inch PMT with a dynamic range of four orders of magnitude for each cell in WCDA-1.Method The dynamic range is extended by using these PMTs to measure the effective charge density in the core region of air shower events,which is an important parameter for identifying the composition of primary particles.Result and Conclusion The system has been running for more than one year.In this paper,the details of the design and performance of WCDA++are presented.
作者 F.Aharonian Q.An Axikegu L.X.Bai Y.X.Bai Y.W.Bao D.Bastieri X.J.Bi Y.J.Bi H.Cai J.T.Cai Z.Cao Z.Cao J.Chang J.F.Chang X.C.Chang B.M.Chen J.Chen L.Chen L.Chen L.Chen M.J.Chen M.L.Chen Q.H.Chen S.H.Chen S.Z.Chen T.L.Chen X.L.Chen Y.Chen N.Cheng Y.D.Cheng S.W.Cui X.H.Cui Y.D.Cui B.Z.Dai H.L.Dai Z.G.Dai Danzengluobu D.della Volpe B.D’Ettorre Piazzoli X.J.Dong J.H.Fan Y.Z.Fan Z.X.Fan J.Fang K.Fang C.F.Feng L.Feng S.H.Feng Y.L.Feng B.Gao C.D.Gao Q.Gao W.Gao M.M.Ge L.S.Geng G.H.Gong Q.B.Gou M.H.Gu J.G.Guo X.L.Guo Y.Q.Guo Y.Y.Guo Y.A.Han H.H.He H.N.He J.C.He S.L.He X.B.He Y.He M.Heller Y.K.Hor C.Hou X.Hou H.B.Hu S.Hu S.C.Hu X.J.Hu D.H.Huang Q.L.Huang W.H.Huang X.T.Huang Y.Huang Z.C.Huang F.Ji X.L.Ji H.Y.Jia K.Jiang Z.J.Jiang C.Jin D.Kuleshov K.Levochkin B.B.Li C.Li C.Li F.Li H.B.Li H.C.Li H.Y.Li J.Li K.Li W.L.Li X.Li X.Li X.R.Li Y.Li Y.Z.Li Z.Li Z.Li E.W.Liang Y.F.Liang S.J.Lin B.Liu C.Liu D.Liu H.Liu H.D.Liu J.Liu J.L.Liu J.S.Liu J.Y.Liu M.Y.Liu R.Y.Liu S.M.Liu W.Liu Y.N.Liu Z.X.Liu W.J.Long R.Lu H.K.Lv B.Q.Ma L.L.Ma X.H.Ma J.R.Mao A.Masood W.Mitthumsiri T.Montaruli Y.C.Nan B.Y.Pang P.Pattarakijwanich Z.Y.Pei M.Y.Qi D.Ruffolo V.Rulev A.Sáiz L.Shao O.Shchegolev X.D.Sheng J.R.Shi H.C.Song Yu.V.Stenkin V.Stepanov Q.N.Sun X.N.Sun Z.B.Sun P.H.T.Tam Z.B.Tang W.W.Tian B.D.Wang C.Wang H.Wang H.G.Wang J.C.Wang J.S.Wang L.P.Wang L.Y.Wang R.N.Wang W.Wang W.Wang X.G.Wang X.J.Wang X.Y.Wang Y.D.Wang Y.J.Wang Y.P.Wang Z.Wang Z.Wang Z.H.Wang Z.X.Wang D.M.Wei J.J.Wei Y.J.Wei T.Wen C.Y.Wu H.R.Wu S.Wu W.X.Wu X.F.Wu S.Q.Xi J.Xia J.J.Xia G.M.Xiang G.Xiao H.B.Xiao G.G.Xin Y.L.Xin Y.Xing D.L.Xu R.X.Xu L.Xue D.H.Yan C.W.Yang F.F.Yang J.Y.Yang L.L.Yang M.J.Yang R.Z.Yang S.B.Yang Y.H.Yao Z.G.Yao Y.M.Ye L.Q.Yin N.Yin X.H.You Z.Y.You Y.H.Yu Q.Yuan H.D.Zeng T.X.Zeng W.Zeng Z.K.Zeng M.Zha X.X.Zhai B.B.Zhang H.M.Zhang H.Y.Zhang J.L.Zhang J.W.Zhang L.Zhang L.Zhang L.X.Zhang P.F.Zhang P.P.Zhang R.Zhang S.R.Zhang S.S.Zhang X.Zhang X.P.Zhang Y.Zhang Y.Zhang Y.F.Zhang Y.L.Zhang B.Zhao J.Zhao L.Zhao L.Z.Zhao S.P.Zhao F.Zheng Y.Zheng B.Zhou H.Zhou J.N.Zhou P.Zhou R.Zhou X.X.Zhou C.G.Zhu F.R.Zhu H.Zhu K.J.Zhu X.Zuo
机构地区 Key Laboratory of Particle Astrophyics&Experimental Physics Division&Computing Center University of Chinese Academy of Sciences TIANFU Cosmic Ray Research Center State Key Laboratory of Particle Detection and Electronics University of Science and Technology of China Department of Engineering Physics National Astronomical Observatories National Space Science Center School of Physics Center for Astrophysics School of Physics and Astronomy&School of Physics(Guangzhou) School of Physical Science and Technology Hebei Normal University School of Physics and Microelectronics School of Astronomy and Space Science Key Laboratory of Dark Matter and Space Astronomy Institute of Frontier and Interdisciplinary Science Key Laboratory for Research in Galaxies and Cosmology Tsung-Dao Lee Institute&School of Physics and Astronomy School of Physical Science and Technology&School of Information Science and Technology College of Physics Key Laboratory of Cosmic Rays(Tibet University) School of Physics and Technology School of Physics and Astronomy Yunnan Observatories Dublin Institute for Advanced Studies Max-Planck-Institut for Nuclear Physics Dipartimento di Fisica dell’Universitàdi Napoli“Federico II” Institute for Nuclear Research of Russian Academy of Sciences Moscow Institute of Physics and Technology Département de Physique Nucléaire et Corpusculaire Department of Physics
出处 《Radiation Detection Technology and Methods》 CSCD 2021年第4期520-530,共11页 辐射探测技术与方法（英文）
基金 This research work is also supported by following grants.The National Key R&D program of China under the Grant 2018YFA0404201,2018YFA0404202 and 2018YFA0404203 by the National Natural Science Foundation of China(NSFC Grants Nos.12022502,No.11905227,No.U1931112,No.11635011,No.11761141001,No.Y811A35,No.11675187,No.U1831208,No.11873005) by the Key R&D Program of SiChuan Province under the Grant 2019ZYZF0001 in Thailand by RTA6280002 from Thailand Science Research and Innovation.
关键词 LHAASO-WCDA WCDA++ Water Cherenkov detector PERFORMANCE
分类号 O57 [理学—粒子物理与原子核物理]
  • 相关文献

参考文献2

二级参考文献7

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共引文献29

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  • 2Yinghui Guo,Shicong Zhang,Mingbo Pu,Qiong He,Jinjin Jin,Mingfeng Xu,Yaxin Zhang,Ping Gao,Xiangang Luo.Spin-decoupled metasurface for simultaneous detection of spin and orbital angular momenta via momentum transformation[J].Light(Science & Applications),2021,10(4):636-647. 被引量：16
  • 3Xiao-Jie Wang,Zhi-Guo Yao,Min Zha,Ming-Jun Chen,Bo Gao,De-Zhi Huang,Hui-Cai Li,Jin-Yan Liu,Wen-Ying Liao,Han-Rong Wu,For the LHAASO collaboration.Trigger and noise filtering algorithms for the LHAASO water Cherenkov detector array[J].Radiation Detection Technology and Methods,2017,1(2):37-50. 被引量：1
  • 4F.Aharonian,Q.An,Axikegu,L.X.Bai,Y.X.Bai,Y.W.Bao,D.Bastieri,X.J.Bi,Y.J.Bi,H.Cai,J.T.Cai,Z.Cao,Z.Cao,J.Chang,J.F.Chang,X.C.Chan,B.M.Chen,J.Chen,L.Chen,L.Chen,L.Chen,M.J.Chen,M.L.Chen,Q.H.Chen,S.H.Chen,S.Z.Chen,T.L.Chen,X.L.Chen,Y.Chen,N.Chen,Y.D.Chen,S.W.Cui,X.H.Cui,Y.D.Cui,B.Z.Dai,H.L.Dai,Z.G.Dai,Danzengluobu,D.della Volpe,B.D’Ettorre Piazzoli,X.J.Don,J.H.Fan,Y.Z.Fan,Z.X.Fan,J.Fang,K.Fan,C.F.Feng,L.Feng,S.H.Fen,Y.L.Feng,B.Gao,C.D.Gao,Q.Gao,W.Gao,M.M.Ge,L.S.Gen,G.H.Gong,Q.B.Gou,M.H.Gu,J.G.Guo,X.L.Guo,Y.Q.Guo,Y.Y.Guo,Y.A.Han,H.H.He,H.N.He,J.C.He,S.L.He,X.B.He,Y.He,M.Heller,Y.K.Hor,C.Hou,X.Hou,H.B.Hu,S.Hu,S.C.Hu,X.J.Hu,D.H.Huang,Q.L.Huan,W.H.Huang,X.T.Huang,Z.C.Huang,F.Ji,X.L.Ji,H.Y.Jia,K.Jiang,Z.J.Jiang,C.Jin,D.Kuleshov,K.Levochkin,B.B.Li,C.Li,C.Li,F.Li,H.B.Li,H.C.Li,H.Y.Li,J.Li,K.Li,W.L.Li,X.Li,X.Li,X.R.Li,Y.Li,Y.Z.Li,Z.Li,Z.Li,E.W.Liang,Y.F.Liang,S.J.Lin,B.Liu,C.Liu,D.Liu,H.Liu,H.D.Liu,J.Liu,J.L.Liu,J.S.Liu,J.Y.Liu,M.Y.Liu,R.Y.Liu,S.M.Liu,W.Liu,Y.N.Liu,Z.X.Liu,W.J.Long,R.Lu,H.K.Lv,B.Q.Ma,L.L.Ma,X.H.Ma,J.R.Mao,A.Masood,W.Mitthumsiri,T.Montaruli,Y.C.Nan,B.Y.Pang,P.Pattarakijwanich,Z.Y.Pei,M.Y.Qi,D.Ruffolo,V.Rulev,A.Sáiz,L.Shao,O.Shchegolev,X.D.Shen,J.R.Shi,H.C.Song,Yu.V.Stenkin,V.Stepanov,Q.N.Sun,X.N.Sun,Z.B.Sun,P.H.T.Tam,Z.B.Tang,W.W.Tian,B.D.Wan,C.Wang,H.Wang,H.G.Wang,J.C.Wang,J.S.Wang,L.P.Wang,L.Y.Wan,R.N.Wang,W.Wang,W.Wang,X.G.Wang,X.J.Wan,X.Y.Wang,Y.D.Wan,Y.J.Wan,Y.P.Wang,Z.Wang,Z.Wang,Z.H.Wang,Z.X.Wang,D.M.Wei,J.J.Wei,Y.J.Wei,T.Wen,C.Y.Wu,H.R.Wu,S.Wu,W.X.Wu,X.F.Wu,S.Q.Xi,J.Xia,J.J.Xia,G.M.Xiang,G.Xiao,H.B.Xiao,G.G.Xin,Y.L.Xin,Y.Xing,D.L.Xu,R.X.Xu,L.Xue,D.H.Yan,C.W.Yang,F.F.Yang,J.Y.Yang,L.L.Yang,M.J.Yan,R.Z.Yang,S.B.Yang,Y.H.Yao,Z.G.Yao,Y.M.Ye,L.Q.Yin,N.Yin,X.H.You,Z.Y.You,Y.H.Yu,Q.Yuan,H.D.Zeng,T.X.Zeng,W.Zeng,Z.K.Zeng,M.Zha,X.X.Zhai,B.B.Zhang,H.M.Zhang,H.Y.Zhang,J.L.Zhang,J.W.Zhang,L.Zhang,L.Zhang,L.X.Zhang,P.F.Zhang,P.P.Zhang,R.Zhang,S.R.Zhang,S.S.Zhan,X.Zhang,X.P.Zhan,Y.Zhan,Y.Zhang,Y.F.Zhang,Y.L.Zhan,B.Zhao,J.Zhao,L.Zhao,L.Z.Zhao,S.P.Zhao,F.Zheng,Y.Zheng,B.Zhou,H.Zhou,J.N.Zhou,P.Zhou,R.Zhou,X.X.Zhou,C.G.Zhu,F.R.Zhu,H.Zhu,K.J.Zhu,X.Zuo,The LHAASO Collaboration.Line-of-shower trigger method to lower energy threshold for GRB detection using LHAASO-WCDA[J].Radiation Detection Technology and Methods,2021,5(4):531-541.
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