Acta Optica Sinica, Volume. 38, Issue 11, 1122001(2018)
Frequency Characteristics of Primary Mirror Control System in Segmented Ring Solar Telescope
Fig. 1. Schematic of 8-m-RST primary mirror system. (a) Top view; (b) sensor, controller and actuator; (c) segmented mirror, support system, actuator and truss
Fig. 4. Two unobservable control modes of primary mirror system. (a) Focus mode; (b) global axial translation mode
Fig. 7. Bode diagram of open-loop system. (a) Input: mode 1, output: mode 1 and mode 2; (b) 72 modes
Fig. 8. Two most sensitive control modes of primary mirror system in 8-m-RST. (a) Mode 1; (b) mode 2
Fig. 9. 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
Fig. 11. Nichols chart of unity gain system. (a) Continuous time system; (b) discrete time system (sampling period is 0.1 s)
Fig. 12. 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
Fig. 14. Bode diagram of disturbance input for primary mirror control system. (a) Open-loop state; (b) closed-loop state
Fig. 16. Error signals under wind disturbance. (a) Error of Mode 1; (b) error of mode 67; (c) error of actuator; (d) RMSE of actuators
Fig. 18. Power spectra of error signals under wind disturbance. (a) Mode 1; (b) mode 67; (c) actuator; (d) RMSE
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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
Category: Optical Design and Fabrication
Received: Mar. 6, 2018
Accepted: May. 29, 2018
Published Online: May. 9, 2019
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