Frequency Characteristics of Primary Mirror Control System in Segmented Ring Solar Telescope

Tai Guo; Yichun Dai; Dehua Yang; Bin Wang; Zhenyu Jin

doi:10.3788/AOS201838.1122001

Journals >Acta Optica Sinica >Volume 38 >Issue 11 >Page 1122001 > Article

Acta Optica Sinica
Vol. 38, Issue 11, 1122001 (2018)

Frequency Characteristics of Primary Mirror Control System in Segmented Ring Solar Telescope

Tai Guo^{1、4、5、*}, Yichun Dai^1、4、*, Dehua Yang³, Bin Wang^1、4、5, and Zhenyu Jin^{1、2、4、*}

Author Affiliations

¹ Yunnan Observatories, Chinese Academy of Sciences, Kunming, Yunnan 650216, China

² Engineering Laboratory on Applied Astronomy of Yunnan, Kunming, Yunnan 650216, China

³ Nanjing University of Aeronautics and Astronautics, Nanjing, Jiangsu 211106, China

⁴ Center for Astronomical Mega-Science, Chinese Academy of Sciences, Beijing 100012, China

⁵ University of Chinese Academy of Sciences, Beijing 100049, China

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DOI: 10.3788/AOS201838.1122001 Cite this Article Set citation alerts

Tai Guo, Yichun Dai, Dehua Yang, Bin Wang, Zhenyu Jin. Frequency Characteristics of Primary Mirror Control System in Segmented Ring Solar Telescope[J]. Acta Optica Sinica, 2018, 38(11): 1122001 Copy Citation Text

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References

Tai Guo, Yichun Dai, Dehua Yang, Bin Wang, Zhenyu Jin. Frequency Characteristics of Primary Mirror Control System in Segmented Ring Solar Telescope[J]. Acta Optica Sinica, 2018, 38(11): 1122001

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