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Gyro / Star Tracker Integration for Satellite High-Accuracy Attitude Determination Considering Relative Sensor Kinematics

机译:陀螺/星跟踪器集成,用于考虑相对传感器运动学的卫星高精度姿态确定

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Gyro / Star tracker integration, usually referred to as gyro-stellar or stellar-inertial estimation is the most common approach for high-precision spacecraft attitude determination. The achievable performance is significantly influenced by relative kinematics between star trackers and gyro unit. The paper analyzes the rejection of this time-variant sensor misalignment. The results show that covariance tuning already improves the achievable attitude performance. But only with state augmentation a significant attitude improvement can be achieved. The presented results are based on Monte Carlo simulations for a typical Earth observation mission.
机译:陀螺仪/恒星跟踪仪集成,通常称为陀螺仪-星体或恒星惯性估计,是高精度航天器姿态确定的最常用方法。星形跟踪器和陀螺仪单元之间的相对运动对可达到的性能有很大的影响。本文分析了这种时变传感器未对准的问题。结果表明,协方差调整已经改善了可实现的姿态性能。但是,只有通过增强状态,才能实现重大的态度改善。给出的结果基于典型的地球观测任务的蒙特卡洛模拟。

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