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Autonomous navigation for lunar satellite using X-ray pulsars with measurement faults

机译:使用具有测量故障的X射线脉冲星自主导航月球卫星

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摘要

X-ray pulsar-based navigation (XNAV) is a navigation method using celestial X-ray source observations for spacecraft orbit determination. However, if the measurements are not reliable due to any kind of malfunction, the performance of XNAV may result in considerable errors and even divergence. In this study, a new algorithm called robust extended Kalman filter (REKF) is proposed for the lunar satellite autonomous navigation system, which is robust against measurement malfunctions. First, the satellite dynamic model applied perturbations is derived under the J2 perturbation of the Moon. The pulse time-of-arrival (TOA) is used to build the observation model. Second, the performance of XNAV system is discussed by analysing the transformation error of TOA, system observability and controllability. Then, an adaptive measurement noise scale factor (AMNSF) is designed by using the innovation sequence in REKF. Meanwhile, the gain matrix is modified by adding the AMNSF to reduce the influence of malfunction and enhance the robustness of XNAV system. Finally, the simulation results show the proposed navigation scheme is valid and feasible, and it is appropriate for lunar satellite autonomous navigation.
机译:基于X射线脉冲星的导航(XNAV)是一种使用天体X射线源观测值确定航天器轨道的导航方法。但是,如果由于某种故障导致测量结果不可靠,则XNAV的性能可能会导致相当大的误差甚至发散。在这项研究中,针对月球卫星自主导航系统,提出了一种称为鲁棒扩展卡尔曼滤波器(REKF)的新算法,该算法可抵抗测量故障。首先,在月球的J2扰动下推导了应用扰动的卫星动力学模型。脉冲到达时间(TOA)用于建立观测模型。其次,通过分析TOA的转换误差,系统的可观察性和可控制性,讨论了XNAV系统的性能。然后,利用REKF中的创新序列设计了一个自适应测量噪声比例因子(AMNSF)。同时,通过添加AMNSF修改增益矩阵,以减少故障的影响并增强XNAV系统的鲁棒性。仿真结果表明所提出的导航方案是有效可行的,适用于月球卫星自主导航。

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