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Inertia tensor estimation for a rigid nadir pointing satellite based on star tracker

机译:基于明星跟踪器的刚性Nadir指向卫星的惯性张量估计

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摘要

Accurate inertia properties information is important to reach an optimized estimation of attitude and precise control of a rigid spacecraft. Unfortunately, the satellite is succumbing several influences that can affect the inertia properties, such as fiiel consumption and sloshing. Thus, mis work inspects me use of star tracker to estimate the attitude, angular velocity and moment of inertia for a rigid nadir pointing satellite by employing extended Kalman filter, without any prior information about the nominal inertia matrix. The proposed estimator is applied in nadir pointing mode and without any constant control torque to avoid the attitude tumbling during the estimation phase, which in turn leads to a catastrophic failure of the satellite missioa The simulation results are compared to three other approaches and validated by Monte Carlo method that elucidates the good performance of the suggested approach and demonstrates its efficiency in satellite inertia tensor and attitude estimation even in worst situations.
机译:准确的惯性属性信息对于达到刚性航天器的态度和精确控制的优化估算非常重要。不幸的是,卫星正在削弱几种影响,这可能会影响惯性性质,例如Fiiel消费和晃动。因此,误工作我使用星象跟踪仪的通过使用扩展卡尔曼滤波器来估计姿态,角速度和转动惯量对于刚性最低点指向卫星检查,没有关于标称惯性矩阵的任何先验信息。所提出的估计是在最低点指向模式和没有任何恒定控制扭矩施加于避免姿势期间的推定相位,这反过来又导致在卫星missioa的灾难性故障的仿真结果进行比较,以其他三种方法和用Monte验证翻滚蒙特卡罗方法阐明了建议的方法的良好性能,并展示了其在卫星惯性张和态度评价效率,即使在最糟糕的情况。

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