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Vision-Based Spacecraft Relative Navigation Using Sparse-Grid Quadrature Filter

机译:基于稀疏网格正交滤波器的基于视觉的航天器相对导航

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摘要

In this paper, vision-based relative navigation of two spacecraft is addressed using the sparse-grid quadrature filter. The relative navigation provides the estimates of the relative orbit and relative attitude as well as the gyro biases. It is a challenging problem because of its high nonlinearity and dimensionality. The extended Kalman filter (EKF) and the unscented Kalman filter (UKF) have been used in the past to solve this problem. However, these filters are not accurate enough in the presence of large initial uncertainties or high nonlinearities. Moreover, although other filters, such as the Gauss-Hermite quadrature filter and the particle filter, can be more accurate than the EKF and UKF, they are hard to use in this high-dimensional estimation problem since a large number of quadrature points or particles are required and therefore the computation complexity is prohibitive. It is shown in this paper that the new sparse-grid quadrature filter can achieve much higher estimation accuracy than EKF, UKF, and the cubature Kalman filter without excessive computation load.
机译:在本文中,使用稀疏网格正交滤波器解决了两个航天器基于视觉的相对导航问题。相对导航提供相对轨道和相对姿态以及陀螺仪偏向的估计。由于其高度的非线性和维数,这是一个具有挑战性的问题。过去已使用扩展卡尔曼滤波器(EKF)和无味卡尔曼滤波器(UKF)来解决此问题。但是,在存在较大的初始不确定性或高度非线性的情况下,这些滤波器不够准确。此外,尽管其他滤波器(例如高斯-赫尔姆特正交滤波器和粒子滤波器)比EKF和UKF更为精确,但由于存在大量的正交点或粒子,因此它们很难用于此高维估计问题是必需的,因此计算复杂性令人望而却步。本文表明,新的稀疏网格正交滤波器可以实现比EKF,UKF和库曼卡尔曼滤波器更高的估计精度,而不会增加计算负担。

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