Chinese Optics, Volume. 18, Issue 1, 121(2025)

Design of constant bias fault observer for fast steering mirrors

Zhi-bin LI1, Jia-nan PAN1, Chong-shang SUN1、*, and Jia-bin WU2
Author Affiliations
  • 1College of Electrical and Automation Engineering, Shandong University of Science and Technology, Qingdao 266590, China
  • 2Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China
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    Fast steering mirror (FSM) typically operates in harsh environments, susceptible to vibrations, temperature fluctuations, and other factors, which can lead to malfunctions. Focusing on the most prevalent constant bias fault, this paper proposes an LMI-based fault observer design method, aiming to enhance the reliability of fault detection and strengthen the stability and anti-interference capabilities of the FSM. Firstly, the model identification method based on Hankel matrix is employed to identify the two-axis fast steering mirror model including the coupling effect. Then, the fault model of the fast steering mirror system is established, and the fault observer of the fast steering mirror is designed by using the LMI-based method. Finally, the proposed method is verified through simulations and experiments. The results indicate that when both axes of the fast steering mirror have constant bias faults in the actuators and sensors, the Riccati-based fault observer can only detect the fault in one axis, while the LMI-based fault observer can detect faults within 0.1 seconds after the fault of the X-axis occurs, and detect faults within 0.06 seconds after the fault of the Y-axis occurs. Therefore, the fault observer designed by the LMI method proposed in this paper can improve the fault detection performance of the fast steering mirror.

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    Zhi-bin LI, Jia-nan PAN, Chong-shang SUN, Jia-bin WU. Design of constant bias fault observer for fast steering mirrors[J]. Chinese Optics, 2025, 18(1): 121

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    Paper Information

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    Received: Jul. 22, 2024

    Accepted: Sep. 30, 2024

    Published Online: Mar. 14, 2025

    The Author Email:

    DOI:10.37188/CO.2024-0136

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