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First generation solar adaptive optics system for 1-m New Vacuum Solar Telescope at Fuxian Solar Observatory
Rao, Chang-Hui1,2; Zhu, Lei1,2; Rao, Xue-Jun1,2; Zhang, Lan-Qiang1,2; Bao, Hua1,2; Ma, Xue-An1,2; Gu, Nai-Ting1,2; Guan, Chun-Lin1,2; Chen, Dong-Hong1,2; Wang, Cheng1,2
刊名RESEARCH IN ASTRONOMY AND ASTROPHYSICS
2016-02-01
卷号16期号:2
关键词adaptive optics high angular resolution sunspots granulation
ISSN号1674-4527
通讯作者Zhu, L (reprint author), Chinese Acad Sci, Key Lab Adapt Opt, Chengdu 610209, Peoples R China
产权排序第三完成单位
英文摘要The first generation solar adaptive optics (AO) system, which consists of a fine tracking loop with a tip-tilt mirror (TTM) and a correlation tracker, and a high-order correction loop with a 37-element deformable mirror (DM), a correlating Shack-Hartmann (SH) wavefront sensor (WFS) based on the absolute difference algorithm and a real time controller (RTC), has been developed and installed at the 1-m New Vacuum Solar Telescope (NVST) that is part of Fuxian Solar Observatory (FSO). Compared with the 37-element solar AO system developed for the 26-cm Solar Fine Structure Telescope, administered by Yunnan Astronomical Observatories, this AO system has two updates: one is the subaperture arrangement of the WFS changed from square to hexagon; the other is the high speed camera of the WFS and the corresponding real time controller. The WFS can be operated at a frame rate of 2100 Hz and the error correction bandwidth can exceed 100 Hz. After AO correction, the averaged residual image motion and the averaged RMS wavefront error are reduced to 0.06 '' and 45 nm, respectively. The results of on-sky testing observations demonstrate better contrast and finer structures of the images taken with AO than those without AO.
学科主题Astronomy & Astrophysics
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]FINE-STRUCTURE TELESCOPE
收录类别SCI
原文出处http://iopscience.iop.org/article/10.1088/1674-4527/16/2/023/meta
语种英语
WOS记录号WOS:000369252500003
内容类型期刊论文
源URL[http://ir.ynao.ac.cn/handle/114a53/9328]  
专题云南天文台_抚仙湖太阳观测站
作者单位1.Key Laboratory on Adaptive Optics, Chinese Academy of Sciences, Shuangliu, Chengdu 610209, China
2.Laboratory on Adaptive Optics, Institute of Optics and Electronics, Chinese Academy of Sciences, Shuangliu, Chengdu 610209, China
3.Yunnan Astronomical Observatories, Chinese Academy of Sciences, Kunming 650011, China
推荐引用方式
GB/T 7714
Rao, Chang-Hui,Zhu, Lei,Rao, Xue-Jun,et al. First generation solar adaptive optics system for 1-m New Vacuum Solar Telescope at Fuxian Solar Observatory[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2016,16(2).
APA Rao, Chang-Hui.,Zhu, Lei.,Rao, Xue-Jun.,Zhang, Lan-Qiang.,Bao, Hua.,...&Liu Z.(2016).First generation solar adaptive optics system for 1-m New Vacuum Solar Telescope at Fuxian Solar Observatory.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,16(2).
MLA Rao, Chang-Hui,et al."First generation solar adaptive optics system for 1-m New Vacuum Solar Telescope at Fuxian Solar Observatory".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 16.2(2016).
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