Chinese Optics Letters, Volume. 14, Issue 10, 100102(2016)

Prototype of solar ground layer adaptive optics at the 1  m New Vacuum Solar Telescope

Lin Kong1,2,3, Lanqiang Zhang1,2、*, Lei Zhu1,2, Hua Bao1,2, Youming Guo1,2, Xuejun Rao1,2, Libo Zhong1,2, and Changhui Rao1,2
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(7)
    Optical layout of the GLAO system. TM: tilt mirror.
    Hardware scheme of real-time controller for the GLAO system.
    Matching arrangement of the DM’s actuators and the subapertures of MD-SHWFS.
    Five-guide star solar MD-SHWFS arrangement of the GLAO and the corresponding areas in the far field.
    Sunspot without AO (left) and with GLAO (right) closed loop for active area NOAA 12480 (705.7 at 0.6 nm).
    Contrast of corresponding areas (a) without AO and (b) with GLAO.
    Granulation contrast for open loop and GLAO closed loop in a period of time (150 images).
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    Lin Kong, Lanqiang Zhang, Lei Zhu, Hua Bao, Youming Guo, Xuejun Rao, Libo Zhong, Changhui Rao, "Prototype of solar ground layer adaptive optics at the 1  m New Vacuum Solar Telescope," Chin. Opt. Lett. 14, 100102 (2016)

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    Paper Information

    Category: Atmospheric and oceanic optics

    Received: Jun. 11, 2016

    Accepted: Aug. 19, 2016

    Published Online: Aug. 2, 2018

    The Author Email: Lanqiang Zhang (lqzhang@ioe.ac.cn)

    DOI:10.3788/COL201614.100102

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