YNAO OpenIR  > 星系类星体研究组
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
会议录名称Proceedings of Science
2022-03-18
卷号395
DOI10.22323/1.395.0286
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
学科门类理学 ; 理学::天文学 ; 工学 ; 工学::核科学与技术
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.
条目包含的文件
文件名称/大小 文献类型 版本类型 开放类型 使用许可
Characteristics of n(1206KB)会议论文 开放获取CC BY-NC-SA浏览 请求全文
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[Wang, Peihan]的文章
[Huang, Daihui]的文章
[Zhou, Xunxiu]的文章
百度学术
百度学术中相似的文章
[Wang, Peihan]的文章
[Huang, Daihui]的文章
[Zhou, Xunxiu]的文章
必应学术
必应学术中相似的文章
[Wang, Peihan]的文章
[Huang, Daihui]的文章
[Zhou, Xunxiu]的文章
相关权益政策
暂无数据
收藏/分享
文件名: Characteristics of near-earth thunderstorm electric fields at LHAASO observatory.pdf
格式: Adobe PDF
所有评论 (0)
暂无评论
 

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。