Progress on Solar Multi-Conjugate Adaptive Optics at the New Vacuum Solar Telescope

被引:0
|
作者
Rao, Changhui [1 ,2 ]
Zhang, Lanqiang [1 ,2 ]
Kong, Lin [1 ,2 ]
Rao, Xuejun [1 ,2 ]
Guo, Youming [1 ,2 ]
Bao, Hua [1 ,2 ]
Zhong, Libo [1 ,2 ]
Zhu, Lei [1 ,2 ]
Ma, Xue'an [1 ,2 ]
Li, Mei [1 ,2 ]
Wang, Cheng [1 ,2 ]
Zhang, Xiaojun [1 ,2 ]
Fan, Xinlong [1 ,2 ]
Chen, Donghong [1 ,2 ]
Wang, Xiaoyun [1 ,2 ]
Feng, Zhongyi [1 ,2 ]
Zhang, Xianyu [3 ]
机构
[1] Chinese Acad Sci, Key Lab Adapt Opt, Chengdu 610209, Sichuan, Peoples R China
[2] Chinese Acad Sci, Inst Opt & Elect, Chengdu 610209, Sichuan, Peoples R China
[3] Large Binocular Telescope Observ, 933 N Cherry Ave, Tucson, AZ 85721 USA
来源
ADAPTIVE OPTICS SYSTEMS VI | 2018年 / 10703卷
基金
中国国家自然科学基金;
关键词
Multi-conjugate adaptive optics (MCAO); multi-direction Shack-Hartmann wavefront sensor; NVST; solar observation;
D O I
10.1117/12.2310124
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Multi-conjugate adaptive optics (MCAO) has been proved to obtain the high resolution images with a large field of view in solar observation. A solar MCAO experiment system had been successfully developed and tested at the 1-meter New Vacuum Solar Telescope (NVST) of Fuxian Solar Observatory. It consists of two deformable mirrors (DMs), a multi-direction Shack-Hartmann wavefront sensor (MD-WFS), and a real-time controller. In order to command the two DMs, five guide regions were selected from the MD-WFS to retrieve a three-dimensional measurement of the turbulent volume based on atmospheric tomography. This system saw the first light in October, 2017, and a series of MCAO-corrected high resolution sunspots images were acquired. In this presentation, the MCAO experiment system is introduced, and the observation results are presented. Furthermore, a new MCAO system based on our proposed MCAO configuration with a high order ground layer adaptive optics and low order high altitude correction will be developed for the NVST as a regularly operating instrument for scientific observations of the sun.
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页数:9
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