Institutional Repository System Of Yunnan Observatories, CAS
| Measurement of muon contents in cosmic ray shower with LHAASO-KM2A around knee region | |
Zhang, Hengying1; Feng, Cunfeng1; Feng, Xiaoting1; Wang, Liping1; He, Huihai2,3,4; Ma, Lingling2,4; Chen, Songzhan2,4; Li, Cong2,4; 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, Liang2,3,4,16; 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; Feng, C. F.1; Feng, L.14; Fang, K.2,4; Feng, S. H.2,4; Feng, Y. L.14; Gao, B.2,4; Gao, C. D.1; Gao, L. Q.2,3,4; Gao, Q.17; Gao, W.1; Ge, M. M.21; Geng, L. S.2,4; Gong, G. H.23; 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.24; 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.23; Huang, D. H.9; Huang, Q. L.2,4; Huang, W. H.1; Huang, X. T.1; 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.25; Levochkin, K.25; Li, B. B.15; Li, Cheng7,8; 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.1; Li, X. R.2,4; Li, Xin7,8,9; Li, Y.10; Li, Y. Z.2,3,4; Li, Zhe2,4; Li, Zhuo26; Liang, E. W.27; Liang, Y. F.27; Lin, S. J.19; Liu, B.8; Liu, C.2,4; Liu, D.1; Liu, H.9; Liu, H. D.24; Liu, J.2,4; Liu, J. L.28; 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.23; Liu, Z. X.10; Long, W. J.9; Lu, R.21; Lv, H. K.2,4; Ma, B. Q.26; Ma, L. L.2,4; Ma, X. H.2,4; Mao JR(毛基荣)29 ; Masood, A.9; Min, Z.2,4; Mitthumsiri, W.30; Montaruli, T.22; Nan, Y. C.1; Pang, B. Y.9; Pattarakijwanich, P.30; Pei, Z. Y.12; Qi, M. Y.2,4; Qi, Y. Q.15; Qiao, B. Q.2,4; Qin, J. J.8; Ruffolo, D.30; Rulev, V.25; Sáiz, A.30; Shao, L.15; Shchegolev, O.25,31; Sheng, X. D.2,4; Shi, J. Y.2,4; Song, H. C.26; Stenkin, Yu. V.25,31; Stepanov, V.25; Su, Y.32; Sun, Q. N.9; Sun, X. N.27; Sun, Z. B.33; Tam, P. H.19; Tang, Z. B.7,8
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| 会议录名称 | Proceedings of Science |
| 2022-03-18 | |
| 卷号 | 395 |
| DOI | 10.22323/1.395.0352 |
| 产权排序 | 第29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 |
| 摘要 | The number of muons observed at the ground from air showers is sensitive to the mass composition of cosmic ray and hadronic interaction model. Large High Altitude Air Shower Observatory is a hybrid extensive air shower array and the KM2A is a sub-array covering an area of 1 km2, consisting of electromagnetic detectors and muon detectors, can measure the muon content and shower size of the air shower simultaneously with high precision for cosmic rays in the knee region. The muon detector of KM2A is the most powerful muon detector in the current cosmic ray observatory on the ground. We made a detailed comparison of experimental and simulated data. The simulation does for EPOS model. © Copyright owned by the author(s). |
| 资助项目 | National Natural Science Foundation of China[11775131] ; National Natural Science Foundation of China[U1931108] |
| 项目资助者 | National Natural Science Foundation of China[11775131, U1931108] |
| 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 | 20230213367644 |
| EI主题词 | Cosmic rays |
| EI分类号 | 657 Space Physics - 657.2 Extraterrestrial Physics and Stellar Phenomena - 944.7 Radiation Measuring Instruments |
| 引用统计 | |
| 文献类型 | 会议论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/25739 |
| 专题 | 星系类星体研究组 |
| 作者单位 | 1.Institute of Frontier and Interdisciplinary Science, Shandong University, Shandong, Qingdao, 266237, 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, 2, Dublin, 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, Università di Napoli `‘Federico II 21.School of Physics and Astronomy, Yunnan University, Yunnan, Kunming, 650091, China; 22.Dèpartement de Physique Nuclèaire et Corpusculaire, Facultè de Sciences, Universitde ` Gen‘eve, 24 Quai Ernest Ansermet, Geneva, 1211, Switzerland; 23.Department of Engineering Physics, Tsinghua University, Beijing, 100084, China; 24.School of Physics and Microelectronics, Zhengzhou University, Henan, Zhengzhou, 450001, China; 25.Institute for Nuclear Research, Russian Academy of Sciences, Moscow, 117312, Russia; 26.School of Physics, Peking University, Beijing, 100871, China; 27.School of Physical Science and Technology, Guangxi University, Guangxi, Nanning, 530004, China; 28.Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, 200240, China; 29.Yunnan Observatories, Chinese Academy of Sciences, Yunnan, Kunming, 650216, China; 30.Department of Physics, Faculty of Science, Mahidol University, Bangkok, 10400, Thailand; 31.Moscow Institute of Physics and Technology, Moscow, 141700, Russia; 32.Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing, 210023, China; 33.National Space Science Center, Chinese Academy of Sciences, Beijing, 100190, China |
| 推荐引用方式 GB/T 7714 | Zhang, Hengying,Feng, Cunfeng,Feng, Xiaoting,et al. Measurement of muon contents in cosmic ray shower with LHAASO-KM2A around knee region[C]:Sissa Medialab Srl,2022. |
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| Measurement of muon （1112KB） | 会议论文 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | ||
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