First light of the 1.8-m solar telescope–CLST

查看全文 作　　者：ChangHui [1,2]Rao;NaiTing [1,2]Gu;XueJun [1,2]Rao;Cheng [1,2]Li;LanQiang [1,2]Zhang;JinLong [1]Huang;Lin [1,2]Kong;Ming [1]Zhang;YunTao [1]Cheng;Yi [1,2]Pu;Hua [1,2]Bao;YouMing [1,2]Guo;YangYi [4]Liu;JinSheng [1,2]Yang;LiBo [1,2]Zhong;ChangJun [1,2]Wang;Kai [1]Fang;XiaoJun [1,2]Zhang;DongHong [1,2]Chen;Cheng [1,2]Wang;XinLong [1,2]Fan;ZhiWu [1,2,3]Yan;KeLe [1,2,3]Chen;XiYa [1,2,3]Wei;Lei [1,2]Zhu;Hong [1]Liu;YongJian [1]Wan;Hao [1,2]Xian;WenLi [1,2]Ma

机构地区：[1]Institute of Optics and Electronics,Chinese Academy of Sciences,Chengdu 610209,China;[2]Key Laboratory on Adaptive Optics,Chinese Academy of Sciences,Chengdu 610209,China;[3]University of Chinese Academy of Sciences,Beijing 100049,China;[4]Department of Road Traffic Management,Sichuan Police College,Luzhou 646000,China

出　　处：《Science China(Physics,Mechanics & Astronomy)》索引2020年第63卷第10期,共2页

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)。 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]. 关键词：TELESCOPE ERUPTION OBSERVATIONS

相关文献

参考文献（10）
引证文献（15）
耦合文献（0）

参考文献(10)

引证文献(15)

互联网出版许可证新出网证(渝)字10号全国400电话 - 免长途话费

First light of the 1.8-m solar telescope–CLST

参考文献(10)

引证文献(15)

用户提示