First light of the 1.8-m solar telescope–CLST

作     者：ChangHui Rao NaiTing Gu XueJun Rao Cheng Li LanQiang Zhang JinLong Huang Lin Kong Ming Zhang YunTao Cheng Yi Pu Hua Bao YouMing Guo YangYi Liu JinSheng Yang LiBo Zhong ChangJun Wang Kai Fang XiaoJun Zhang DongHong Chen Cheng Wang XinLong Fan ZhiWu Yan KeLe Chen XiYa Wei Lei Zhu Hong Liu YongJian Wan Hao Xian WenLi Ma ChangHui Rao;NaiTing Gu;XueJun Rao;Cheng Li;LanQiang Zhang;JinLong Huang;Lin Kong;Ming Zhang;YunTao Cheng;Yi Pu;Hua Bao;YouMing Guo;YangYi Liu;JinSheng Yang;LiBo Zhong;ChangJun Wang;Kai Fang;XiaoJun Zhang;DongHong Chen;Cheng Wang;XinLong Fan;ZhiWu Yan;KeLe Chen;XiYa Wei;Lei Zhu;Hong Liu;YongJian Wan;Hao Xian;WenLi Ma

作者机构：Institute of Optics and ElectronicsChinese Academy of SciencesChengdu 610209China Key Laboratory on Adaptive OpticsChinese Academy of SciencesChengdu 610209China University of Chinese Academy of SciencesBeijing 100049China Department of Road Traffic ManagementSichuan Police CollegeLuzhou 646000China 

出 版 物：《Science China(Physics,Mechanics & Astronomy)》 (中国科学：物理学、力学、天文学（英文版）)

年 卷 期：2020年第63卷第10期

页      面：133-134页

核心收录：

学科分类：07[理学] 070401[理学-天体物理] 0704[理学-天文学] 

基　　金：supported by the National Natural Science Foundation of China(Grant No.11727805) the Youth Innovation Promotion Association,Chinese Academy of Sciences(Grant No.2018412) 

主　　题：telescope eruption observations 

摘      要：Large-aperture solar telescopes play an important role in solar observations and research,and require high temporal and spatial resolution[1].To solve some fundamental problems such as the solar dynamo,coronal heating,and the triggering of major solar eruptions,the spatial resolution for solar-atmosphere observation should reach at least 0.1 arcsec[2].