基于无气味卡尔曼滤波的航天器相对姿态鲁棒估计

IF 6.5 1区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Mohammed Atallah, Mohamed Okasha, Ossama Abdelkhalik, Tarek N. Dief
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引用次数: 0

摘要

提出了一种考虑非加性过程噪声和测量噪声的航天器相对姿态估计方法。采用扭扭模型来表示飞行器的追星器相对于目标的六自由度运动,用追星器体框架表示。twistor模型利用Modified Rodrigues Parameters (MRPs)以最少的参数表示姿态,消除了四元数模型中存在的归一化约束。此外,它将相对位置和姿态合并在一个模型中,解决了状态的运动耦合并简化了估计器的设计。尽管已有许多姿态估计算法,但许多算法依赖于对加性噪声假设的简化。本文通过推导出两种方法来精确逼近具有非加性噪声系统的过程噪声和测量噪声协方差矩阵,增强了非加性噪声算法的鲁棒性和收敛性。第一种方法利用斯特林插值公式(Stirling Interpolation Formula, SIF)得到等效的过程噪声和测量噪声协方差矩阵。第二种方法采用状态噪声补偿(SNC)法推导等效过程噪声协方差矩阵,利用SIF法计算等效测量噪声协方差矩阵。这些方法被整合到UKF框架中,用于估计近距离操作中航天器的相对姿态,并通过两种场景进行演示:一种是使用位置传感二极管(psd)的合作目标,另一种是使用激光雷达进行三维成像的非合作目标。这些方法的有效性通过蒙特卡罗模拟与文献中的其他方法进行了验证,展示了它们更快的收敛性和鲁棒性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Robust twistor-based spacecraft relative pose estimation using unscented Kalman filter

This paper presents new methods for spacecraft relative pose estimation using the Unscented Kalman Filter (UKF), taking into account non-additive process and measurement noises. A twistor model is employed to represent the spacecraft’s relative 6-DOF motion of the chaser with respect to the target, expressed in the chaser body frame. The twistor model utilizes Modified Rodrigues Parameters (MRPs) to represent attitude with a minimal number of parameters, eliminating the need for the normalization constraint that exists in the quaternion-based model. Additionally, it incorporates both relative position and attitude in a single model, addressing kinematic coupling of states and simplifying the estimator design. Despite numerous existing pose estimation algorithms, many rely on the simplification of additive noise assumptions. This work enhances the robustness and improves the convergence of non-additive noise algorithms by deriving two methods to accurately approximate process and measurement noise covariance matrices for systems with non-additive noises. The first method utilizes the Stirling Interpolation Formula (SIF) to obtain equivalent process and measurement noise covariance matrices. The second method employs State Noise Compensation (SNC) to derive the equivalent process noise covariance matrix and uses SIF to compute the equivalent measurement noise covariance matrix. These methods are integrated into the UKF framework for estimating the relative pose of spacecraft in proximity operations, demonstrated through two scenarios: one with a cooperative target using Position Sensing Diodes (PSDs) and another with an uncooperative target using LiDAR for 3-D imaging. The effectiveness of these methods is validated against others in the literature through Monte Carlo simulations, showcasing their faster convergence and robust performance.

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来源期刊
Astrodynamics
Astrodynamics Engineering-Aerospace Engineering
CiteScore
6.90
自引率
34.40%
发文量
32
期刊介绍: Astrodynamics is a peer-reviewed international journal that is co-published by Tsinghua University Press and Springer. The high-quality peer-reviewed articles of original research, comprehensive review, mission accomplishments, and technical comments in all fields of astrodynamics will be given priorities for publication. In addition, related research in astronomy and astrophysics that takes advantages of the analytical and computational methods of astrodynamics is also welcome. Astrodynamics would like to invite all of the astrodynamics specialists to submit their research articles to this new journal. Currently, the scope of the journal includes, but is not limited to:Fundamental orbital dynamicsSpacecraft trajectory optimization and space mission designOrbit determination and prediction, autonomous orbital navigationSpacecraft attitude determination, control, and dynamicsGuidance and control of spacecraft and space robotsSpacecraft constellation design and formation flyingModelling, analysis, and optimization of innovative space systemsNovel concepts for space engineering and interdisciplinary applicationsThe effort of the Editorial Board will be ensuring the journal to publish novel researches that advance the field, and will provide authors with a productive, fair, and timely review experience. It is our sincere hope that all researchers in the field of astrodynamics will eagerly access this journal, Astrodynamics, as either authors or readers, making it an illustrious journal that will shape our future space explorations and discoveries.
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