Chinese Optics Letters, Volume. 8, Issue 10, 966(2010)

37-element solar adaptive optics for 26-cm solar fine structure telescope at Yunnan Astronomical Observatory

Changhui Rao1,2, Lei Zhu1,2, Xuejun Rao1,2, Chunlin Guan1,2, Donghong Chen1,2, Jun Lin3, and Zizhong Liu3
Author Affiliations
  • 1Key Laboratory on Adaptive Optics, Chinese Academy of Sciences, Chengdu 610209, China
  • 2Laboratory on Adaptive Optics, Institute of Optics and Electronics, Chinese Academy of Sciences, Chengdu 610209, China
  • 3Yunnan Astronomical Observatory, National Astronomical Observatories,Chinese Academy of Sciences, Kunming 650011, China
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    A 37-element solar adaptive optics (AO) system was built and installed at the 26-cm solar fine structure telescope of Yunnan Astronomical Observatory. The AO system is composed of a fine tracking loop with a tip/tilt mirror and a correlation tracker, a high-order correction loop with a 37-element deformable mirror, a correlating Shack-Hartmann wavefront sensor based on the absolute difference algorithm, and a real time controller. The system was completed on Sep. 28, 2009 and was used to obtain AO-corrected highresolution solar images. The contrast and resolution of the images are clearly improved after wavefront correction by AO. To the best of out knowledge, this system is the first solar AO system in China.

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    Changhui Rao, Lei Zhu, Xuejun Rao, Chunlin Guan, Donghong Chen, Jun Lin, Zizhong Liu. 37-element solar adaptive optics for 26-cm solar fine structure telescope at Yunnan Astronomical Observatory[J]. Chinese Optics Letters, 2010, 8(10): 966

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    Paper Information

    Received: Jan. 14, 2010

    Accepted: --

    Published Online: Oct. 19, 2010

    The Author Email:

    DOI:10.3788/COL20100810.0966

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