排序方式: 共有73条查询结果,搜索用时 531 毫秒
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针对转动惯量未知的非合作目标的姿态角速度估计问题,将解算得到的非合作目标的惯性姿态作为测量信息,估计姿态角速度和姿态动力学参数(即转动惯量比).首先,应用非线性控制系统的几何理论对待估计的状态扩展系统进行能观性分析.然后,利用UKF设计相应的滤波估计算法.仿真结果表明,本文所设计的方法能够精确估计出非合作目标的姿态角速度与转动惯量比. 相似文献
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因为X射线敏感器不能分辨具体的脉冲,X射线脉冲星导航方法存在整脉冲周期模糊数问题.现有求解周期模糊数的方法过程复杂,计算量大.本文在飞行器估计位置十分精确的假设下,提出了无周期模糊数的X射线脉冲星迭代滤波导航方法.UKF滤波器基于轨道动力学给出探测器的估计位置,以脉冲到达标称位置和估计位置的时间差作为反馈,进行迭代滤波,最终得到探测器的真实位置和速度估计.仿真表明,该方法能在火星探测器的日心转移轨道上实现高精度的导航,其精度可达到位置误差5km和速度误差0.5m/s. 相似文献
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Bang-Zhao Zhou Xiao-Feng Liu Guo-Ping Cai Yun-Meng Liu Pan Liu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(1):496-511
Capturing an uncontrolled space target is a tremendously challenging research topic. Target capture by a space robot can be well planned according to predicted motion of the target. In this paper, motion prediction of an uncontrolled space target is studied and a motion prediction algorithm is proposed. In the proposed algorithm, firstly a method for identifying the parameters of motion state and inertial property of the target is established; and then through substituting the identified parameters into the dynamic equations of the target, the motion of the target can be predicted as the solution of the equations. In the identification of the parameters, the unscented Kalman filter (UKF) is applied. In order to support the UKF, a method for estimating noise level of the observation data is developed, so our motion prediction algorithm is noise adaptive. A practical convergent criterion is also designed to determine the time when the estimated result of the UKF is accurate enough, such that the predicted motion is credible enough. After that, the accuracy of the prediction is further improved by an optimization method. In the end of this paper, numerical simulations are done to verify the validity of the proposed motion prediction algorithm. Simulation results indicate that the proposed algorithm is able to predict the motion of the target precisely. 相似文献
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基于地磁场测量估计卫星姿态的UKF算法 总被引:1,自引:0,他引:1
提出了利用UKF(Unscented Kalman Filter)处理地磁场测量数据进行低轨道(LEO)卫星自主定姿的算法。通过使用估计姿态、轨道参数和国际地磁场参考(IGRF)计算得到的地磁矢量与三轴磁强计(TAM)的测量矢量之差作为更新信息,可以实现实时的姿态角和角速度估计。针对卫星稳态定姿、大角度快速机动的定姿以及姿态失控状态下的定姿等三种任务,分别用UKF和传统的EKF(Extended Kalman Filter)进行了数值仿真。仿真结果显示出本文提出的定姿算法的优越性。 相似文献
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