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QLEKF的木星探测环绕段自主导航方法

Research on an Autonomous Navigation Method for the Orbital Phase of Jupiter Probe Based on QLEKF

  • 摘要: 针对木星探测复杂环境导致的噪声不确定性对滤波性能的影响,基于多个木星卫星相对视线方向信息建立了光学自主导航方案,采用单滤波器简化的Q学习扩展卡尔曼滤波(Q Learning Extend Kalman Filter,QLEKF)算法对探测器位置和速度进行估计。QLEKF-single(单滤波器Q学习扩展卡尔曼滤波)基于单个EKF滤波器新息设计奖励函数,通过Q学习算法自适应地选择噪声协方差阵的取值,利用SoftMax策略进行动作选择,最终通过EKF实现系统状态的迭代估计。仿真通过随机生成初始状态估计和测量噪声,对木星真实的轨道动力学模型进行简化,验证了在噪声不确定影响条件下,QLEKF-single算法相较于传统滤波方法有效提高了导航精度;与QLEKF算法相比,在精度变化不大的情况下,运行时间减少了10%以上。

     

    Abstract: Jupiter exploration is of critical importance for comprehending the solar system’s evolution and utilizing planetary gravity for deep space missions. To address the challenge of noise uncertainty affecting filtering performance in Jupiter’s complex environment, an optical autonomous navigation scheme is established based on the relative line-of-sight information from multiple Jovian moons, using a simplified QLEKF(Q-Learning Extended Kalman Filter)algorithm with a single filter to estimate the position and velocity of the probe. The QLEKF-single(Single Filter Q-learning Extended Kalman Filter)designs a reward function based on the innovation of a single EKF filter. The Q-learning algorithm adaptively selects the values of the noise covariance matrix, while the SoftMax strategy is employed for action selection, ultimately achieving iterative system state estimation by EKF filter. Through simulation by randomly generating initial state estimates and measurement noise, the simplified model of Jupiter's real orbital dynamics was verified. It demonstrated that in scenarios with noise uncertainty, the QLEKF-single algorithm effectively improved navigation accuracy compared to traditional filtering methods. Moreover, compared to the QLEKF algorithm, the run time was reduced by more than 10% with little change in accuracy.

     

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