Institutional Repository System Of Yunnan Observatories, CAS
| Design and Implementation of a Portable Laser Calibration System for LHAASO-WFCTA | |
Yuan, Guotao1; Sun, Qinning1; Jin, Min1; Xia, Junji1; Liu, Jing1; Min, Zhen2,3; Zhu, Fengrong1; Chen, Long1; Wang, Yang1; Liu, Yu1; Zhang, Yong2; Cao, Zhen2,4,5; Aharonian, F.6,7; An, Q.8,9; Axikegu10; Bai, L. X.11; Bai, Y. X.2,5; Bai, L. X.11; Bai, Y. X.2,5; Bao, Y. W.12; Bastieri, D.13; Bi, X. J.2,4,5; Bi, Y. J.2,5; Cai, H.14; Cai, J. T.13; Cao, Zhe8,9; Chang, J.15; Chang, J. F.2,5,8; Chen, B. M.16; Chen, E. S.2,4,5; Chen, J.11; Chen, Liang2,4,5; Chen, Liang17; Chen, Long10; Chen, M. J.2,5; Chen, M. L.2,5,8; Chen, Q. H.10; Chen, S. H.2,4,5; Chen, S. Z.2,5; Chen, T. L.18; Chen, X. L.2,4,5; Chen, Y.12; Cheng, N.2,5; Cheng, Y. D.2,5; Cui, S. W.16; Cui, X. H.19; Cui, Y. D.20; D’Ettorre Piazzoli, B.21; Dai, B. Z.22; Dai, H. L.2,5,8; Dai, Z. G.9; Danzengluobu18; della Volpe, D.23; Dong, X. J.2,5; Duan, K. K.15; Fan, J. H.13; Fan, Y. Z.15; Fan, Z. X.2,5; Fang, J.22; Fang, K.2,5; Feng, C. F.24; Feng, L.15; Feng, S. H.2,5; Feng, Y. L.15; Gao, B.2,5; Gao, C. D.24; Gao, L. Q.2,4,5; Gao, Q.18; Gao, W.24; Ge, M. M.22; Geng, L. S.2,5; Gong, G. H.25; Gou, Q. B.2,5; Gu, M. H.2,5,8; Guo, F. L.17; Guo, J. G.2,4,5; Guo, X. L.10; Guo, Y. Q.2,5; Guo, Y. Y.2,4,5,15; Han, Y. A.26; He, H. H.2,4,5; He, H. N.15; He, J. C.2,4,5; He, S. L.13; He, X. B.20; He, Y.10; Heller, M.23; Hor, Y. K.20; Hou, C.2,5; Hu, H. B.2,4,5; Hu, S.11; Hu, S. C.2,4,5; Hu, X. J.25; Huang, D. H.10; Huang, Q. L.2,5; Huang, W. H.24; Huang, X. T.24; Huang, X. Y.15; Huang, Z. C.10; Ji, F.2,5; Ji, X. L.2,5,8; Jia, H. Y.10; Jiang, K.8,9; Jiang, Z. J.22; Jin, C.2,4,5; Ke, T.2,5; Kuleshov, D.27; Levochkin, K.27; Li, B. B.16; Li, Cheng8,9; Li, Cong2,5; Li, F.2,5,8; Li, H. B.2,5; Li, H. C.2,5; Li, H. Y.9,15; Li, J.2,5,8; Li, K.2,5; Li, W. L.24; Li, X. R.2,5; Li, Xin8,9; Li, Xin10; Li, Y.11; Li, Y. Z.2,4,5; Li, Zhe2,5; Li, Zhuo28; Liang, E. W.29; Liang, Y. F.29; Lin, S. J.20; Liu, B.9; Liu, C.2,5; Liu, D.24; Liu, H.10; Liu, H. D.26; Liu, J.2,5; Liu, J. L.30; Liu, J. S.20; Liu, J. Y.2,5; Liu, M. Y.18; Liu, R. Y.12; Liu, S. M.10; Liu, W.2,5; Liu, Y.13; Liu, Y. N.25; Liu, Z. X.11; Long, W. J.10; Lu, R.22; Lv, H. K.2,5; Ma, B. Q.28; Ma, L. L.2,5; Ma, X. H.2,5; Mao JR(毛基荣)31 ; Masood, A.10; Min, Z.2,5; Mitthumsiri, W.32; Montaruli, T.23; Nan, Y. C.24; Pang, B. Y.10; Pattarakijwanich, P.32; Pei, Z. Y.13; Qi, M. Y.2,5; Qi, Y. Q.16; Qiao, B. Q.2,5; Qin, J. J.9; Ruffolo, D.32; Rulev, V.27; Sáiz, A.32; Shao, L.16; Shchegolev, O.27,33; Sheng, X. D.2,5; Shi, J. Y.2,5; Song, H. C.28; Stenkin, Yu. V.27,33
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| 会议录名称 | Proceedings of Science |
| 2024-09-27 | |
| 卷号 | 444 |
| DOI | 10.22323/1.444.0498 |
| 产权排序 | 第31完成单位 |
| 收录类别 | EI |
| 会议名称 | 38th International Cosmic Ray Conference, ICRC 2023 |
| 会议日期 | 2023-07-26 |
| 会议地点 | Nagoya, Japan |
| 会议赞助商 | et al.; Institute for Cosmic Ray Research (ICRR) Univeristy of Tokyo; International Union of Pure and Applied Physics (IUPAP); JPS; Nagoya Convention and Visitors Bureau; Nagoya University |
| 摘要 | The Wide Field of View Cherenkov Telescope Array (WFCTA), situated in the harsh environment of Daocheng, is established to investigate ultrahigh energy cosmic rays. To enhance the calibration of WFCTA, a portable laser calibration system has been developed, which provides specified energy and direction of the YAG laser. Special designs, including power system, north calibration, and rotating system, have been implemented to ensure the proper functioning of the portable laser calibration system. The aluminum alloy of the entire frame and the vibration damper provide robust anti-impact ability and safety during transportation to different observation locations. A temperature control facility has been employed to meet the operational temperature requirement of electronic equipment. Various sensors have been utilized to monitor environmental parameters, the energy of YAG laser pulses, azimuth and pitch angles, and other parameters in real-time. The auto-control program is communicated wirelessly to avoid any manual interference with the system. The field experiment results have confirmed the reliability of the system and its ability to meet the calibration requirements of WFCTA. © Copyright owned by the author(s) under the terms of the Creative Commons. |
| 资助项目 | National Key Research and Development Program of China[2021YFA0718403];National Natural Science Foundation of China[12105233];National Natural Science Foundation of China[12173039] |
| 项目资助者 | National Key Research and Development Program of China[2021YFA0718403] ; National Natural Science Foundation of China[12105233, 12173039] |
| 语种 | 英语 |
| 学科领域 | 天文学 ; 天体物理学 ; 高能天体物理学 ; 星系与宇宙学 |
| 文章类型 | Conference article (CA) |
| URL | 查看原文 |
| EI入藏号 | 20245117555776 |
| EI主题词 | Laser safety |
| EI分类号 | 713.1 Amplifiers - 744 Lasers - 901.3 Engineering Research - 914.1 Accidents and Accident Prevention |
| 引用统计 | |
| 文献类型 | 会议论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/27915 |
| 专题 | 星系类星体研究组 |
| 作者单位 | 1.School of Physical Science and Technology, Southwest Jiaotong University, Sichuan Province, Chengdu, 611756, 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.TIANFU Cosmic Ray Research Center, Institute of HighEnergy Physics, Chinese Academy of Sciences, Sichuan Province, Chengdu, 610000, 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 2, 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", Complesso Universitario di Monte Sant’Angelo, via Cinthia, Napoli, 80126, Italy; 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 | Yuan, Guotao,Sun, Qinning,Jin, Min,et al. Design and Implementation of a Portable Laser Calibration System for LHAASO-WFCTA[C],2024. |
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| Design and Implement（2145KB） | 会议论文 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | ||
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