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Study on Fault Detection of Star-Sensor Based on UKF

机译:基于UKF的星传感器故障检测研究

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摘要

The fault detection of star sensor in satellite when no telemetry data from the gyroscope can be obtained is investigated. An algorithm based on the unscented Kalman filter (UKF) is proposed to indicate the occurrence of the fault. By adding the angular speed of the satellite into the state equation, the UKF is designed to estimate the angular and the angular speed of the satellite. After that, a comparison between the measured and the estimated value of both the angular and the angular speed is made. In this way, the star sensor fault can be finally detected. Two fault cases (abrupt constant fault and noise increase fault) are taken into consideration in the simulation to show the validness of the present algorithm. Furthermore, a test verification by using the real telemetry data on orbit is performed to demonstrate that the present algorithm can detect the star sensor fault effectively. In application, the developed fault detection algorithm can be employed in the ground measurement and control station to monitor the star sensor fault such that the fault can be detected immediately and the alarm indicating the occurrence of the fault will be given.
机译:星传感器在卫星故障检测时,可以得到来自陀螺仪没有遥测数据进行了研究。提出了一种基于无味卡尔曼滤波器(UKF)的算法,以指示所述故障的发生。通过将卫星的角速度进入状态方程,UKF被设计来估计角和卫星的角速度。在此之后,所测量的和所估计的值的角度和角速度两者之间进行比较时。这样一来,星敏感器故障可最后检测。两个故障的情况下(突然恒定故障和噪音的增加的故障)被考虑在仿真中示出了本算法的区分有效性。此外,通过使用在轨道上的实际的遥测数据的测试验证被执行以证明本算法可以检测星传感器有效故障。在应用中,将显影的故障检测算法可以在地面的测量和控制站监视星传感器故障,使得故障可立即检测和指示所述故障的发生时的报警将给出被采用。

著录项

  • 作者

    Di Hu; Dan Liu; Guangming Bai;

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  • 年度 2019
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  • 原文格式 PDF
  • 正文语种 chi/zho
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