Flux variations of cosmic ray air showers detected by LHAASO-KM2A during a thunderstorm on June 10, 2021* * Supported in China by National Key R&D program of China , NSFC and in Thailand by RTA6280002 from Thailand Science Research and Innovation
【作者】Aharonian, Felix，An, Q.，None, Axikegu，Bai, Lixin，Bai, Yunxiang，Bao, Yiwei，Bastieri, D.，Bi, X. J.，Bi, Yujiang，Cai, J. T.，Cao, Zhe，Cao, Zhen，Chang, J.，Chang, J. F.，Chen, E. S.，Chen, Liang，Chen, Lin，Chen, Minjun，Chen, M. L.，Chen, Shanhong，Chen, S. Z.，Chen, T. L.，Chen, X. J.，Chen, Yao，Cheng, H. L.，Cheng, Ning，Cheng, Y. D.，Cui, Sh W.，Cui, Xiaohong，Cui, Y. D.，Dai, B. Z.，Dai, H. L.，Dai, Z. G.，None, Danzengluobu，Volpe, Domenico Della，Duan, K. K.，Fan, J. H.，Fan, Y. Z.，Fan, Z. X.，Fang, Jinghong，Fang, K.，Feng, C. F.，Feng, L.，Feng, Shaohui，Feng, X. T.，Feng, Youliang，Gao, Bo，Gao, C. D.，Gao, L. Q.，Gao, Q.，Gao, Wei，Gao, W. K.，Ge, Maomao，Geng, L. S.，Gong, G. H.，Gou, Q. B.，Gu, Minhao，Guo, F. L.，Guo, Junguang，Guo, X. L.，Guo, Yiqin，Guo, Yingying，Han, Y. A.，He, H. H.，He, Haoning，He, S. L.，He, Xinbo，He, Yu，Heller, M.，Hor, Yuen Keung，Hou, Chao，Hou, X.，Hu, Haibing，Hu, Qingqing，Hu, S.，Hu, S. C.，Hu, X. J.，Huang, Daihui，Huang, Wenhao，Huang, X. T.，Huang, Xiaoyuan，Huang, Yan，Huang, Z. C.，Ji, X. L.，Jia, H. Y.，Jia, K.，Jiang, K.，Jiang, Zej
【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, Hefei, 230026, China;8School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Chengdu, 610031, China;9College of Physics, Sichuan University, Chengdu, 610065, China;10School of Astronomy and Space Science, Nanjing University, Nanjing, 210023, China;11Center for Astrophysics, Guangzhou University, Guangzhou, 510006, China;12Key Laboratory of Dark Matter and Space Astronomy, Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, 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, Shijiazhuang, 050024, China;17School of Physics and Astronomy (Zhuhai), School of Physics (Guangzhou), Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, Zhuhai, 510275, China;18School of Physics and Astronomy, Yunnan University, Kunming, 650091, China;19D′epartement de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, Geneva, 1211, Switzerland;20Institute of Frontier and Interdisciplinary Science, Shandong University, Qingdao, 266237, China;21Department of Engineering Physics, Tsinghua University, Beijing, 100084, China;22School of Physics and Microelectronics, Zhengzhou University, Zhengzhou, 450001, China;23Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, China;24Institute for Nuclear Research, Russian Academy of Sciences, Moscow, 117312, Russian Federation;25School of Physics, Peking University, Beijing, 100871, China;26School of Physical Science and Technology, Guangxi University, Nanning, 530004, China;27Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, 200240, China
【年份】2023
【卷号】Vol.47 No.1
【ISSN】1674-1137
【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 a thunderstorm on June 10, 2021. The number of shower events tha...
