Flux Variations of Cosmic Ray Air Showers Detected by LHAASO-KM2A During aThunderstorm on 10 June 2021

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【作者】Aharonian, F.，An, Q.，Axikegu，Bai, L.X.，Bai, Y.X.，Bao, Y.W.，Bastieri, D.，Bi, X.J.，Bi, Y.J.，Cai, J.T.，Cao, Zhe，Cao, Zhen，Chang, J.，Chang, J.F.，Chen, E.S.，Chen, Liang，Chen, Long，Chen, M.J.，Chen, M.L.，Chen, S.H.，Chen, S.Z.，Chen, T.L.，Chen, X.J.，Chen, Y.，Cheng, H.L.，Cheng, N.，Cheng, Y.D.，Cui, S.W.，Cui, X.H.，Cui, Y.D.，Dai, B.Z.，Dai, H.L.，Dai, Z.G.，Danzengluobu，Della Volpe, D.，Uan, K.K.，Fan, J.H.，Fan, Y.Z.，Fan, Z.X.，Fang, J.，Fang, K.，Feng, C.F.，Feng, L.，Feng, S.H.，Feng, X.T.，Eng, Y.L.，Gao, B.，Gao, C.D.，Gao, L.Q.，Gao, Q.，Gao, W.，Gao, W.K.，Ge, M.M.，Geng, L.S.，Gong, G.H.，Gou, Q.B.，Gu, M.H.，Guo, F.L.，Guo, J.G.，Guo, X.L.，Guo, Y.Q.，Guo, Y.Y.，Han, Y.A.，He, H.H.，He, H.N.，He, S.L.，He, X.B.，He, Y.，Heller, M.，Hor, Y.K.，Hou, C.，Hou, X.，Hu, H.B.，Hu, Q.，Hu, S.，Hu, S.C.，Hu, X.J.，Huang, D.H.，Huang, W.H.，Huang, X.T.，Huang, X.Y.，Huang, Y.，Huang, Z.C.，Ji, X.L.，Ia, H.Y.，Jia, K.，Jiang, K.，Jiang, Z.J.，Jin, M.，Kang, M.M.，Ke, T.，Kuleshov, D.，Li, B.B
【作者单位】¹Key Laboratory of Particle Astrophyics, Experimental Physics Division, Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing; 100049, China;²University of Chinese Academy of Sciences, Beijing; 100049, China;³Tianfu Cosmic Ray Research Center, Sichuan, Chengdu, China;⁴Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2, Ireland;⁵Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg; 69029, Germany;⁶State Key Laboratory of Particle Detection and Electronics, China;⁷University of Science and Technology of China, Anhui, Hefei; 230026, China;⁸School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Sichuan, Chengdu; 610031, China;⁹College of Physics, Sichuan University, Sichuan, Chengdu; 610065, China;¹⁰School of Astronomy and Space Science, Nanjing University, Jiangsu, Nanjing; 210023, China;¹¹Center for Astrophysics, Guangzhou University, Guangdong, Guangzhou; 510006, China;¹²Key Laboratory of Dark Matter and Space Astronomy, Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing; 210023, China;¹³Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai; 200030, China;¹⁴Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Tibet, Lhasa; 850000, China;¹⁵National Astronomical Observatories, Chinese Academy of Sciences, Beijing; 100101, China;¹⁶Hebei Normal University, Hebei, Shijiazhuang; 050024, China;¹⁷School of Physics and Astronomy, Sino-French Institute of Nuclear Engineering and Technology, Sun Yat-sen University, Zhuhai; 519000, China;¹⁸Dipartimento di Fisica, Dell'Università di Napoli Federico II, Complesso Universitario di Monte Sant'Angelo, via Cinthia, Napoli; 80126, Italy;¹⁹School of Physics and Astronomy, Yunnan University, Yunnan, Kunming; 650091, China;²⁰Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, Geneva; 1211, Switzerland;²¹Institute of Frontier and Interdisciplinary Science, Shandong University, Shandong, Qingdao; 266237, China;²²Department of Engineering Physics, Tsinghua University, Beijing; 100084, China;²³School of Physics and Microelectronics, Zhengzhou University, Henan, Zhengzhou; 450001, China;²⁴Yunnan Observatories, Chinese Academy of Sciences, Yunnan, Kunming; 650216, China;²⁵Institute for Nuclear Research of Russian Academy of Sciences, Moscow; 117312, Russia;²⁶School of Physics, Peking University, Beijing; 100871, China;²⁷School of Physical Science and Technology, Guangxi University, Guangxi, Nanning; 530004, China;²⁸Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai; 200240, China;²⁹Department of Physics, Faculty of Science, Mahidol University, Bangkok; 10400, Thailand;³⁰Moscow Institute of Physics and Technology, Moscow; 141700, Russia;³¹National Space Science Center, Chinese Academy of Sciences, Beijing; 100190, China;³²School of Physics (Guangzhou), Sun Yat-sen University, Guangdong, Guangzhou; 510275, China
【年份】2022
【摘要】 The Large High Altitude Air Shower Observatory has three sub-arrays, KM2A, WCDA and WFCTA. The flux variations of cosmic ray air showers were studied by analyzing the KM2A data during the thunderstorm on 10 June 2021. The number of shower events tha...
【文献类型】期刊

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