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基于星敏感器测量矢量的角速度估计

Angular velocity estimation from measurement vectors of star tracker.

作者信息

Liu Hai-bo, Yang Jun-cai, Yi Wen-jun, Wang Jiong-qi, Yang Jian-kun, Li Xiu-jian, Tan Ji-chun

机构信息

National University of Defense Technology, Changsha, Hunan, 410073, China.

出版信息

Appl Opt. 2012 Jun 1;51(16):3590-8. doi: 10.1364/AO.51.003590.

Abstract

In most spacecraft, there is a need to know the craft's angular rate. Approaches with least squares and an adaptive Kalman filter are proposed for estimating the angular rate directly from the star tracker measurements. In these approaches, only knowledge of the vector measurements and sampling interval is required. The designed adaptive Kalman filter can filter out noise without information of the dynamic model and inertia dyadic. To verify the proposed estimation approaches, simulations based on the orbit data of the challenging minisatellite payload (CHAMP) satellite and experimental tests with night-sky observation are performed. Both the simulations and experimental testing results have demonstrated that the proposed approach performs well in terms of accuracy, robustness, and performance.

摘要

在大多数航天器中,需要了解航天器的角速率。提出了采用最小二乘法和自适应卡尔曼滤波器的方法,用于直接从星跟踪器测量值中估计角速率。在这些方法中,只需要矢量测量值和采样间隔的知识。所设计的自适应卡尔曼滤波器可以在没有动态模型和惯性并矢信息的情况下滤除噪声。为了验证所提出的估计方法,基于具有挑战性的微型卫星有效载荷(CHAMP)卫星的轨道数据进行了仿真,并进行了夜空观测的实验测试。仿真和实验测试结果均表明,所提出的方法在准确性、鲁棒性和性能方面表现良好。

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