Chinese Optics Letters, Volume. 13, Issue 12, 120101(2015)

Second generation solar adaptive optics for 1-m New Vacuum Solar Telescope at the Fuxian Solar Observatory

Changhui Rao1,2, Lei Zhu1,2、*, Xuejun Rao1,2, Lanqiang Zhang1,2, Hua Bao1,2, Lin Kong1,2,3, Youming Guo1,2, Xue’an Ma1,2, Mei Li1,2, Cheng Wang1,2, Xiaojun Zhang1,2, Xinlong Fan1,2, Donghong Chen1,2, Zhongyi Feng1,2, Xiaoyun Wang1,2, Naiting Gu1,2, and Zhiyong Wang1,2,3
Author Affiliations
  • 1The Key Laboratory on Adaptive Optics, Chinese Academy of Sciences, Chengdu 610209, China
  • 2The Laboratory on Adaptive Optics, Institute of Optics and Electronics, Chinese Academy of Sciences, Chengdu 610209, China
  • 3University of Chinese Academy of Sciences, Beijing 100049, China
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    Figures & Tables(5)
    Optical diagram of the NVST.
    Optical layout of the AO system.
    Matching arrangement of the DM’s actuators and the subapertures of the WFS.
    Simultaneous photosphere (a,b) and chromosphere (c,d) images without/with AO.
    Contrast of the granulation in the photosphere image without/with AO.
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    Changhui Rao, Lei Zhu, Xuejun Rao, Lanqiang Zhang, Hua Bao, Lin Kong, Youming Guo, Xue’an Ma, Mei Li, Cheng Wang, Xiaojun Zhang, Xinlong Fan, Donghong Chen, Zhongyi Feng, Xiaoyun Wang, Naiting Gu, Zhiyong Wang. Second generation solar adaptive optics for 1-m New Vacuum Solar Telescope at the Fuxian Solar Observatory[J]. Chinese Optics Letters, 2015, 13(12): 120101

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    Paper Information

    Category: Atmospheric and oceanic optics

    Received: Aug. 25, 2015

    Accepted: Oct. 27, 2015

    Published Online: Sep. 12, 2018

    The Author Email: Lei Zhu (zhulei_cas@aliyun.com)

    DOI:10.3788/COL201513.120101

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