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Monocular-vision-based spacecraft relative state estimation under dual number algebra

机译:双数代数下基于单目视觉的航天器相对状态估计

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This paper develops a relative state estimation method for two spacecraft based on monocular vision measurement, where the leader spacecraft of three-dimensional shape is observed by a calibrated camera fixed on the follower spacecraft. The two-dimensional image of the leader spacecraft with multiple geometric features is obtained by the camera. Multiple geometric features including points, lines and circles are described under dual number algebra, and the observation models are proposed based on the geometric projection relationships of these features. By the proposed method, the geometric features appeared on the leader spacecraft can be employed to estimate the relative state between the two spacecraft. Another contribution of this paper is to develop a six-degree-of-freedom relative motion dynamics using dual number. The dynamics model describes the relative motion between arbitrary points on the spacecraft, and both the kinematically and dynamically coupling effects are considered. Based on the derived process model and observation model, an extended Kalman filter is presented to estimate the relative state between the two spacecraft. In addition, an unscented Kalman filter is also developed to avoid complicated calculation of derivations. Finally, numerical simulations are performed to evaluate the proposed EKF and UKF approaches based on multiple geometric feature measurement. Simulation results verify the effectiveness of the proposed method, and show that by using EKF or UKF technique, the relative translation and rotation estimation errors converge rapidly with the desired high estimation accuracy. Comparison simulations are made with the situations using less feature measurement, which demonstrate that employing multiple feature measurement provides superior estimation performance than methods with less feature measurement.
机译:本文开发了一种基于单眼视觉测量的两航天器的相对状态估计方法,其中,通过固定在从动航天器上的校准摄像机观察三维形状的前导航天器。带有多个几何特征的前导航天器的二维图像是通过摄像头获得的。在双数代数下描述了包括点,线和圆的多个几何特征,并基于这些特征的几何投影关系提出了观测模型。通过提出的方法,可以将出现在前导航天器上的几何特征用于估计两个航天器之间的相对状态。本文的另一个贡献是利用双数建立了六自由度的相对运动动力学。动力学模型描述了航天器上任意点之间的相对运动,并考虑了运动学和动态耦合效应。基于导出的过程模型和观测模型,提出了扩展的卡尔曼滤波器来估计两个航天器之间的相对状态。此外,还开发了无味卡尔曼滤波器,以避免复杂的导数计算。最后,进行了数值模拟,以基于多个几何特征测量评估提出的EKF和UKF方法。仿真结果验证了该方法的有效性,并表明通过使用EKF或UKF技术,相对平移和旋转估计误差可以快速收敛,并具有所需的高估计精度。在使用较少特征量的情况下进行了比较仿真,这表明与使用较少特征量的方法相比,使用多重特征量可提供更好的估计性能。

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