First light of solar multi-conjugate adaptive optics at the 1-m new vacuum solar telescope

被引：0

作者：

ChangHui Rao ^{[1
,2
]}

LanQiang Zhang ^{[1
,2
]}

Lin Kong ^{[1
,2
]}

YouMing Guo ^{[1
,2
]}

XueJun Rao ^{[1
,2
]}

Hua Bao ^{[1
,2
]}

Lei Zhu ^{[1
,2
]}

LiBo Zhong ^{[1
,2
]}

机构：

[1] The Key Laboratory on Adaptive Optics, Chinese Academy of Sciences

[2] Institute of Optics and Electronics, Chinese Academy of Sciences

来源：

Science China(Physics,Mechanics & Astronomy) | 2018年 / 08期

基金：

中国国家自然科学基金;

关键词：

D O I：

暂无

中图分类号：

P111.41 [太阳观测仪器]; P182.2 [太阳观测];

学科分类号：

070401 ;

摘要：

Observations play a leading role in any branches of astronomy,including solar physics.In order to solve fundamental problems,such as solar dynamo[1],coronal heating[2]and the triggering of major solar eruptions[3],solar observations with spatial resolution better than 0.1 arcsec are required.Such a goal cannot be achieved without the help of adaptive optics(AO),which eliminates the wavefront distortion caused by atmosphere turbulence[4,5].However,solar observations are performed over an extended field of view

引用

页码：104 / 107

页数：4

共 50 条

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