Institutional Repository System Of Yunnan Observatories, CAS
| Characteristics of near-earth thunderstorm electric fields at LHAASO observatory | |
Wang, Peihan1; Huang, Daihui1; Zhou, Xunxiu1; Huang, Zhicheng1; Axi, Kegu1; Chen, Lin1; Cao, Zhen2,3,4; Aharonian, F.5,6; An, Q.7,8; Axikegu9; Bai, L. X.10; Bai, Y. X.2,4; Bao, Y. W.11; Bastieri, D.12; Bi, X. J.2,3,4; Bi, Y. J.2,4; Cai, H.13; Cai, J. T.12; Cao, Zhe7,8; Chang, J.14; Chang, J. F.2,4,7; Chen, B. M.15; Chen, E. S.2,3,4; Chen, J.10; Chen, Liang2,3,4; Chen, Liang16; Chen, Long9; Chen, M. J.2,4; Chen, M. L.2,4,7; Chen, Q. H.9; Chen, S. H.2,3,4; Chen, S. Z.2,4; Chen, T. L.17; Chen, X. L.2,3,4; Chen, Y.11; Cheng, N.2,4; Cheng, Y. D.2,4; Cui, S. W.15; Cui, X. H.18; Cui, Y. D.19; D’Ettorre Piazzoli, B.20; Dai, B. Z.21; Dai, H. L.2,4,7; Dai, Z. G.8; Danzengluobu17; della Volpe, D.22; Dong, X. J.2,4; Duan, K. K.14; Fan, J. H.12; Fan, Y. Z.14; Fan, Z. X.2,4; Fang, J.21; Fang, K.2,4; Feng, C. F.23; Feng, L.14; Feng, S. H.2,4; Feng, Y. L.14; Gao, B.2,4; Gao, C. D.23; Gao, L. Q.2,3,4; Gao, Q.17; Gao, W.23; Ge, M. M.21; Geng, L. S.2,4; Gong, G. H.24; Gou, Q. B.2,4; Gu, M. H.2,4,7; Guo, F. L.16; Guo, J. G.2,3,4; Guo, X. L.9; Guo, Y. Q.2,4; Guo, Y. Y.2,3,4,14; Han, Y. A.25; He, H. H.2,3,4; He, H. N.14; He, J. C.2,3,4; He, S. L.12; He, X. B.19; He, Y.9; Heller, M.22; Hor, Y. K.19; Hou, C.2,4; Hu, H. B.2,3,4; Hu, S.10; Hu, S. C.2,3,4; Hu, X. J.24; Huang, D. H.9; Huang, Q. L.2,4; Huang, W. H.23; Huang, X. T.23; Huang, X. Y.14; Huang, Z. C.9; Ji, F.2,4; Ji, X. L.2,4,7; Jia, H. Y.9; Jiang, K.7,8; Jiang, Z. J.21; Jin, C.2,3,4; Ke, T.2,4; Kuleshov, D.26; Levochkin, K.26; Li, B. B.15; Li, Cheng7,8; Li, Cong2,4; Li, F.2,4,7; Li, H. B.2,4; Li, H. C.2,4; Li, H. Y.8,14; Li, J.2,4,7; Li, K.2,4; Li, W. L.23; Li, X. R.2,4; Li, Xin7,8; Li, Xin9; Li, Y.10; Li, Y. Z.2,3,4; Li, Zhe2,4; Li, Zhuo27; Liang, E. W.28; Liang, Y. F.28; Lin, S. J.19; Liu, B.8; Liu, C.2,4; Liu, D.23; Liu, H.9; Liu, H. D.25; Liu, J.2,4; Liu, J. L.29; Liu, J. S.19; Liu, J. Y.2,4; Liu, M. Y.17; Liu, R. Y.11; Liu, S. M.9; Liu, W.2,4; Liu, Y.12; Liu, Y. N.24; Liu, Z. X.10; Long, W. J.9; Lu, R.21; Lv, H. K.2,4; Ma, B. Q.27; Ma, L. L.2,4; Ma, X. H.2,4; Mao JR(毛基荣)30 ; Masood, A.9; Min, Z.2,4; Mitthumsiri, W.31; Montaruli, T.22; Nan, Y. C.23; Pang, B. Y.9; Pattarakijwanich, P.31; Pei, Z. Y.12; Qi, M. Y.2,4; Qi, Y. Q.15; Qiao, B. Q.2,4; Qin, J. J.8; Ruffolo, D.31; Rulev, V.26; Saiz, A.31; Shao, L.15; Shchegolev, O.26,32; Sheng, X. D.2,4; Shi, J. Y.2,4; Song, H. C.27; Stenkin, Yu. V.26,32; Stepanov, V.26; Su, Y.33; Sun, Q. N.9; Sun, X. N.28; Sun, Z. B.34; Tam, P. H.19
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| 会议录名称 | Proceedings of Science |
| 2022-03-18 | |
| 卷号 | 395 |
| DOI | 10.22323/1.395.0286 |
| 产权排序 | 第30完成单位 |
| 收录类别 | EI |
| 会议名称 | 37th International Cosmic Ray Conference, ICRC 2021 |
| 会议日期 | 2021-07-12 |
| 会议地点 | Virtual, Berlin, Germany |
| 关键词 | Near-earth thunderstorm electric fields LHAASO observatory Cosmic rays Thunderstorm parameter |
| 摘要 | Thunderstorms are common weather phenomena at high altitudes, accompanying with lightning, strong winds and other disasters. During thunderstorms, the strength of atmospheric electric fields could be up to 1000 V/cm or even higher. The intensity fluctuates violently and the polarity could change multiple times. So, direct measurement of the thunderstorm electric field is a quite challenging work. The Large High Altitude Air Shower Observatory (LHAASO), under the construction of a project at Daocheng (4410 m a.s.l., Sichuan, China), is featured with frequent thunderstorms, especially in summer. The distribution of thunderstorm parameters is presented by analyzing the near-earth atmospheric electric field of the LHAASO station in this work. The polarity and intensity variation characteristics of the electric field in the cumulus, mature and dissipating stages of thunderstorm are also discussed. The results show that the thunderstorms mainly occur in the period of a time from late afternoon to evening. They are more frequent and stronger in summer. During the mature stage, the field changes more dramatically. Our results could be helpful in understanding the variations of cosmic rays at LHAASO during thunderstorms, and provide valuable information for studying global thunderstorm activity. © Copyright owned by the author(s). |
| 资助项目 | National Natural Science Foundation of China[11475141] ; National Natural Science Foundation of China[12047576] ; National Natural Science Foundation of China[U2031101] |
| 项目资助者 | National Natural Science Foundation of China[11475141,12047576,U2031101] |
| 语种 | 英语 |
| 学科领域 | 天文学 ; 天体物理学 ; 高能天体物理学 ; 核科学技术 |
| 文章类型 | Conference article (CA) |
| 出版者 | Sissa Medialab Srl |
| URL | 查看原文 |
| EI入藏号 | 20225113275810 |
| EI主题词 | Observatories |
| EI分类号 | 443.1 Atmospheric Properties - 657 Space Physics - 657.2 Extraterrestrial Physics and Stellar Phenomena |
| 引用统计 | |
| 文献类型 | 会议论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/25682 |
| 专题 | 星系类星体研究组 |
| 作者单位 | 1.School of Physical Science and Technology, Southwest Jiaotong University, Chengdu, 610031, China; 2.Key Laboratory of Particle Astrophyics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, 100049, China; 3.University of Chinese Academy of Sciences, Beijing, 100049, China; 4.TIANFU Cosmic Ray Research Center, Sichuan, Chengdu, China; 5.Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin, 02, Ireland; 6.Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg, 69029, Germany; 7.State Key Laboratory of Particle Detection and Electronics, China; 8.University of Science and Technology of China, Anhui, Hefei, 230026, China; 9.School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Sichuan, Chengdu, 610031, China; 10.College of Physics, Sichuan University, Sichuan, Chengdu, 610065, China; 11.School of Astronomy and Space Science, Nanjing University, Jiangsu, Nanjing, 210023, China; 12.Center for Astrophysics, Guangzhou University, Guangdong, Guangzhou, 510006, China; 13.School of Physics and Technology, Wuhan University, Hubei, Wuhan, 430072, China; 14.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing, 210023, China; 15.Hebei Normal University, Hebei, Shijiazhuang, 050024, China; 16.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China; 17.Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Tibet, Lhasa, 850000, China; 18.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China; 19.School of Physics and Astronomy, School of Physics (Guangzhou), Sun Yat-sen University, Guangdong, Zhuhai, 519000, China; 20.Dipartimento di Fisica dell’Universit‘a di Napoli 21.School of Physics and Astronomy, Yunnan University, Yunnan, Kunming, 650091, China; 22.D’epartement de Physique Nucl’eaire et Corpusculaire, Facult’e de Sciences, Universit’e de Gen‘eve, 24 Quai Ernest Ansermet, Geneva, 1211, Switzerland; 23.Institute of Frontier and Interdisciplinary Science, Shandong University, Shandong, Qingdao, 266237, China; 24.Department of Engineering Physics, Tsinghua University, Beijing, 100084, China; 25.School of Physics and Microelectronics, Zhengzhou University, Henan, Zhengzhou, 450001, China; 26.Institute for Nuclear Research of Russian Academy of Sciences, Moscow, 117312, Russia; 27.School of Physics, Peking University, Beijing, 100871, China; 28.School of Physical Science and Technology, Guangxi University, Guangxi, Nanning, 530004, China; 29.Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, 200240, China; 30.Yunnan Observatories, Chinese Academy of Sciences, Yunnan, Kunming, 650216, China; 31.Department of Physics, Faculty of Science, Mahidol University, Bangkok, 10400, Thailand; 32.Moscow Institute of Physics and Technology, Moscow, 141700, Russia; 33.Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing, 210023, China; 34.National Space Science Center, Chinese Academy of Sciences, Beijing, 100190, China |
| 推荐引用方式 GB/T 7714 | Wang, Peihan,Huang, Daihui,Zhou, Xunxiu,et al. Characteristics of near-earth thunderstorm electric fields at LHAASO observatory[C]:Sissa Medialab Srl,2022. |
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