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

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

Tai Guo1,4,5、*, Yichun Dai1,4、*, Dehua Yang3, Bin Wang1,4,5, and Zhenyu Jin1,2,4、*
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
  • show less
    Figures & Tables(19)
    Schematic of 8-m-RST primary mirror system. (a) Top view; (b) sensor, controller and actuator; (c) segmented mirror, support system, actuator and truss
    Finite element model of 8-m-RST
    Schematic of pulsed wind speed field
    Two unobservable control modes of primary mirror system. (a) Focus mode; (b) global axial translation mode
    Schematic of synchronous sampling for edge and tilt sensors
    Modeling chart of primary mirror and its control system
    Bode diagram of open-loop system. (a) Input: mode 1, output: mode 1 and mode 2; (b) 72 modes
    Two most sensitive control modes of primary mirror system in 8-m-RST. (a) Mode 1; (b) mode 2
    Bode diagram of system. (a) Continuous time system; (b) discrete time system; (c) Bode diagrams of open-loop and closed-loop systems for mode 1
    Step response for mode 1
    Nichols chart of unity gain system. (a) Continuous time system; (b) discrete time system (sampling period is 0.1 s)
    Nichols charts of system when relative stablity requirment is satisfied. (a) Continuious time system, integral gain of 3.3; (b) samping time of 0.05 s, integral gain of 2.0; (c) samping time of 0.1 s,integral gain of 1.3; (d) samping time of 0.2 s, integral gain of 0.71
    Spectrum of pulsed wind speed field
    Bode diagram of disturbance input for primary mirror control system. (a) Open-loop state; (b) closed-loop state
    Step response of disturbance input for mode 1 as example
    Error signals under wind disturbance. (a) Error of Mode 1; (b) error of mode 67; (c) error of actuator; (d) RMSE of actuators
    Mode 67
    Power spectra of error signals under wind disturbance. (a) Mode 1; (b) mode 67; (c) actuator; (d) RMSE
    • Table 1. Sampling period, integral gain and control bandwidth for 4 systems in Fig. 12

      View table

      Table 1. Sampling period, integral gain and control bandwidth for 4 systems in Fig. 12

      Tt /sKIBandwidth /Hz
      Continuous3.30.46
      0.052.00.30
      0.11.30.20
      0.20.710.12
    Tools

    Get Citation

    Copy Citation Text

    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

    Download Citation

    EndNote(RIS)BibTexPlain Text
    Save article for my favorites
    Paper Information

    Category: Optical Design and Fabrication

    Received: Mar. 6, 2018

    Accepted: May. 29, 2018

    Published Online: May. 9, 2019

    The Author Email:

    DOI:10.3788/AOS201838.1122001

    Topics