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
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].
发文机构：Institute of Optics and Electronics Key Laboratory on Adaptive Optics University of Chinese Academy of Sciences Department of Road Traffic Management
关键词：TELESCOPEERUPTIONOBSERVATIONS
分类号： P111.2[天文地球—天文学]
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