Opto-Electronic Engineering, Volume. 45, Issue 3, 170733(2018)

Development of solar adaptive optics

Rao Changhui1,2、*, Zhu Lei1,2, Zhang Lanqiang1,2, Rao Xuejun1,2, Bao Hua1,2,3, Kong Lin1,2, Guo Youming1,2, Zhong Libo1,2, Ma Xuean1,2, Li Mei1,2, Wang Cheng1,2, Zhang Xiaojun1,2, Fan Xinlong1,2, Wang Xiaoyun1,2, Fan Muwen1,2, Chen Donghong1,2, and Feng Zhongyi1,2
Author Affiliations
  • 1[in Chinese]
  • 2[in Chinese]
  • 3[in Chinese]
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    Solar images with high spatial resolution, high temporal resolution across a large field of view (FoV) are aspired for solar physics and space weather. Ground-based high spatial resolution imaging of the Sun is severely limited by wavefront disturbances induced by the Earth’s atmosphere turbulence. Therefore, solar adaptive optics aims at these requirements and it has revitalized ground-based solar astronomy at existing telescopes. Meanwhile, multi-conjugate adaptive optics has been proved to overcome the anisoplanatism and obtain the high resolution images with a large field of view in solar observation by compensating for the turbulence with several deformable mirrors conjugated to different heights. In this review, we give some summarization of the development of solar adaptive abroad, and emphatically introduce several adaptive optics systems in China and the progress of large FoV adaptive optics.

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    Rao Changhui, Zhu Lei, Zhang Lanqiang, Rao Xuejun, Bao Hua, Kong Lin, Guo Youming, Zhong Libo, Ma Xuean, Li Mei, Wang Cheng, Zhang Xiaojun, Fan Xinlong, Wang Xiaoyun, Fan Muwen, Chen Donghong, Feng Zhongyi. Development of solar adaptive optics[J]. Opto-Electronic Engineering, 2018, 45(3): 170733

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    Paper Information

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    Received: Dec. 28, 2017

    Accepted: --

    Published Online: May. 3, 2018

    The Author Email: Changhui Rao (chrao@ioe.ac.cn)

    DOI:10.12086/oee.2018.170733

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