Institutional Repository System Of Yunnan Observatories, CAS
| The Laser calibration system for LHAASO-WFCTA | |
Wang, Y.1; Chen, L.1; Liu, H.1; Sun, Q. N.1; Li, X.1; Xia, J. J.1; Zhu, F. R.1; Geng, L. S.2; Zhang, S. S.2; Zhang, Y.2; Cao, Zhen3,4,5; Aharonian, F.6,7; An, Q.8,9; Axikegu10; Bai, L. X.11; Bai, Y. X.3,5; Bao, Y. W.12; Bastieri, D.13; Bi, X. J.3,4,5; Bi, Y. J.3,5; Cai, H.14; Cai, J. T.13; Cao, Zhe8,9; Chang, J.15; Chang, J. F.3,5,8; Chen, B. M.16; Chen, E. S.3,4,5; Chen, J.11; Chen, Liang3,4,5; Chen, Liang17; Chen, Long10; Chen, M. J.3,5; Chen, M. L.3,5,8; Chen, Q. H.10; Chen, S. H.3,4,5; Chen, S. Z.3,5; Chen, T. L.18; Chen, X. L.3,4,5; Chen, Y.12; Cheng, N.3,5; Cheng, Y. D.3,5; Cui, S. W.16; Cui, X. H.19; Cui, Y. D.20; D’Ettorre Piazzoli, B.21; Dai, B. Z.22; Dai, H. L.3,5,8; Dai, Z. G.9; Danzengluobu18; della Volpe, D.23; Dong, X. J.3,5; Duan, K. K.15; Fan, J. H.13; Fan, Y. Z.15; Fan, Z. X.3,5; Fang, J.22; Fang, K.3,5; Feng, C. F.24; Feng, L.15; Feng, S. H.3,5; Feng, Y. L.15; Gao, B.3,5; Gao, C. D.24; Gao, L. Q.3,4,5; Gao, Q.18; Gao, W.24; Ge, M. M.22; Geng, L. S.3,5; Gong, G. H.25; Gou, Q. B.3,5; Gu, M. H.3,5,8; Guo, F. L.17; Guo, J. G.3,4,5; Guo, X. L.10; Guo, Y. Q.3,5; Guo, Y. Y.3,4,5,15; Han, Y. A.26; He, H. H.3,4,5; He, H. N.15; He, J. C.3,4,5; He, S. L.13; He, X. B.20; He, Y.10; Heller, M.23; Hor, Y. K.20; Hou, C.3,5; Hu, H. B.3,4,5; Hu, S.11; Hu, S. C.3,4,5; Hu, X. J.25; Huang, D. H.10; Huang, Q. L.3,5; Huang, W. H.24; Huang, X. T.24; Huang, X. Y.15; Huang, Z. C.10; Ji, F.3,5; Ji, X. L.3,5,8; Jia, H. Y.10; Jiang, K.8,9; Jiang, Z. J.22; Jin, C.3,4,5; Ke, T.3,5; Kuleshov, D.27; Levochkin, K.27; Li, B. B.16; Li, Cheng8,9; Li, Cong3,5; Li, F.3,5,8; Li, H. B.3,5; Li, H. C.3,5; Li, H. Y.9,15; Li, J.3,5,8; Li, K.3,5; Li, W. L.24; Li, X. R.3,5; Li, Xin8,9; Li, Xin10; Li, Y.11; Li, Y. Z.3,4,5; Li, Zhe3,5; Li, Zhuo28; Liang, E. W.29; Liang, Y. F.29; Lin, S. J.20; Liu, B.9; Liu, C.3,5; Liu, D.24; Liu, H.10; Liu, H. D.26; Liu, J.3,5; Liu, J. L.30; Liu, J. S.20; Liu, J. Y.3,5; Liu, M. Y.18; Liu, R. Y.12; Liu, S. M.10; Liu, W.3,5; Liu, Y.13; Liu, Y. N.25; Liu, Z. X.11; Long, W. J.10; Lu, R.22; Lv, H. K.3,5; Ma, B. Q.28; Ma, L. L.3,5; Ma, X. H.3,5; Mao JR(毛基荣)31 ; Masood, A.10; Min, Z.3,5; Mitthumsiri, W.32; Montaruli, T.23; Nan, Y. C.24; Pang, B. Y.10; Pattarakijwanich, P.32; Pei, Z. Y.13; Qi, M. Y.3,5; Qi, Y. Q.16; Qiao, B. Q.3,5; Qin, J. J.9; Ruffolo, D.32; Rulev, V.27; Sáiz, A.32; Shao, L.16; Shchegolev, O.27,33; Sheng, X. D.3,5; Shi, J. Y.3,5; Song, H. C.28; Stenkin, Yu. V.27,33; Stepanov, V.27; Su, Y.34; Sun, Q. N.10
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| 会议录名称 | Proceedings of Science |
| 2022-03-18 | |
| 卷号 | 395 |
| DOI | 10.22323/1.395.0271 |
| 产权排序 | 第31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 Wide Field-of-view Cherenkov Telescope Array (WFCTA) of Large High Altitude Air Shower Observatory (LHAASO) is designed to measure the Cherenkov and fluorescent light created in the extensive air showers by cosmic rays (CRs) from ∼30 TeV to several EeV. In order to achieve an end-to-end calibration method for WFCTA, three Laser lidar facilities have been installed at LHAASO. They feature two N2 and one YAG Lasers which direct calibrated and pulsed beams into sky. Light scattered from Laser beams produces tracks recorded by the telescope detectors. The Laser calibration systems are used to investigate properties of the atmosphere and air fluorescence. In this paper, we introduce the design and performance of the Laser facilities at an altitude of 4410 m. Great cares were taken to select the data collected by telescopes at clear nights for our analysis. After excluding the inconsistency of all SiPMs of the telescope, we find that the experimental data of the images collected by telescopes agree noticeably well with Monte Carlo’s simulation. © Copyright owned by the author(s). |
| 资助项目 | National Natural Science Foundation of China[11947404] ; Department of Science and Technology of Sichuan Province[2020YFSY0016] ; Department of Science and Technology of Sichuan Province[2021YFSY0031] |
| 项目资助者 | National Natural Science Foundation of China[11947404] ; Department of Science and Technology of Sichuan Province[2020YFSY0016,2021YFSY0031] |
| 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 | 20225113275756 |
| EI主题词 | Fluorescence |
| EI分类号 | 657 Space Physics - 657.2 Extraterrestrial Physics and Stellar Phenomena - 741.1 Light/Optics - 744.1 Lasers, General - 744.8 Laser Beam Interactions - 804.2 Inorganic Compounds - 922.2 Mathematical Statistics |
| 引用统计 | |
| 文献类型 | 会议论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/25688 |
| 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, 611756, China; 2.Key Laboratory of Particle Astrophysics, Institute of High Energy Physics of the Chinese Academy of Sciences, Beijing, 100049, China; 3.Key Laboratory of Particle Astrophyics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, 100049, China; 4.University of Chinese Academy of Sciences, Beijing, 100049, China; 5.TIANFU Cosmic Ray Research Center, Sichuan, Chengdu, China; 6.Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin, 02, Ireland; 7.Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg, 69029, Germany; 8.State Key Laboratory of Particle Detection and Electronics, China; 9.University of Science and Technology of China, Anhui, Hefei, 230026, China; 10.School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Sichuan, Chengdu, 610031, China; 11.College of Physics, Sichuan University, Sichuan, Chengdu, 610065, China; 12.School of Astronomy and Space Science, Nanjing University, Jiangsu, Nanjing, 210023, China; 13.Center for Astrophysics, Guangzhou University, Guangdong, Guangzhou, 510006, China; 14.School of Physics and Technology, Wuhan University, Hubei, Wuhan, 430072, China; 15.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing, 210023, China; 16.Hebei Normal University, Hebei, Shijiazhuang, 050024, China; 17.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China; 18.Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Tibet, Lhasa, 850000, China; 19.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China; 20.School of Physics and Astronomy, School of Physics (Guangzhou), Sun Yat-sen University, Guangdong, Zhuhai, 519000, China; 21.Dipartimento di Fisica dell’Università di Napoli `‘Federico II 22.School of Physics and Astronomy, Yunnan University, Yunnan, Kunming, 650091, China; 23.D’epartement de Physique Nucl’eaire et Corpusculaire, Facult’e de Sciences, Universit’e de Gen‘eve, 24 Quai Ernest Ansermet, Geneva, 1211, Switzerland; 24.Institute of Frontier and Interdisciplinary Science, Shandong University, Shandong, Qingdao, 266237, China; 25.Department of Engineering Physics, Tsinghua University, Beijing, 100084, China; 26.School of Physics and Microelectronics, Zhengzhou University, Henan, Zhengzhou, 450001, China; 27.Institute for Nuclear Research of Russian Academy of Sciences, Moscow, 117312, Russia; 28.School of Physics, Peking University, Beijing, 100871, China; 29.School of Physical Science and Technology, Guangxi University, Guangxi, Nanning, 530004, China; 30.Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, 200240, China; 31.Yunnan Observatories, Chinese Academy of Sciences, Yunnan, Kunming, 650216, China; 32.Department of Physics, Faculty of Science, Mahidol University, Bangkok, 10400, Thailand; 33.Moscow Institute of Physics and Technology, Moscow, 141700, Russia; 34.Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing, 210023, China; 35.National Space Science Center, Chinese Academy of Sciences, Beijing, 100190, China |
| 推荐引用方式 GB/T 7714 | Wang, Y.,Chen, L.,Liu, H.,et al. The Laser calibration system for LHAASO-WFCTA[C]:Sissa Medialab Srl,2022. |
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| 文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
| The Laser calibratio（3354KB） | 会议论文 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | ||
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