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A Maximum Information Rate Quaternion Filter for Spacecraft Attitude Estimation

机译:用于航天器姿态估计的最大信息速率四元数滤波器

摘要

Building on previous works, this paper introduces a novel continuous-time stochastic optimal linear quaternion estimator under the assumptions of rate gyro measurements and of vector observations of the attitude. A quaternion observation model, which observation matrix is rank degenerate, is reduced to a two-dimensional model via a maximum information rate approach. The resulted filter combines the exact treatment of the quaternion process state-dependent noise and the quaternion measurement state-dependent noise under the framework of continuous-time optimal linear filtering. This yields statistically consistent covariance computations within the proposed filter without requiring tuning. The case of white noises in the gyro and vector measurements are considered in this work. This paper also presents the development of a Sun vector determination subsystem for the nanosatelite Delfi-N3xt. Simulations and preliminary experimental validation show that this subsystem, which consists of six four-quadrant Sun sensors, can deliver a Sun-spacecraft line of sight with an averaged equivalent angular error of approximately 0.2 deg without the Earth albedo. The performances of the novel filter are illustrated via extensive Monte-Carlo simulations in the case of Delfi-N3xt, where Sun vector measurements, Earth magnetic measurements and gyro measurements are acquired along a 600 km height Sun synchronous orbit. The proposed filter appears to be insensitive to poor initial conditions and low sampling rates. It converges where a standard extended Kalman filter fails to do so under the same conditions.
机译:在之前的工作的基础上,本文介绍了一种新颖的连续时间随机最优线性四元数估计器,该估计器基于速率陀螺仪测量和姿态矢量观测的假设。通过最大信息速率方法将观测矩阵秩退化的四元数观测模型简化为二维模型。所得的滤波器在连续时间最佳线性滤波的框架下,结合了对四元数过程状态相关噪声和四元数测量状态相关噪声的精确处理。这样就可以在建议的滤波器内进行统计上一致的协方差计算,而无需调整。这项工作考虑了陀螺仪中白噪声和矢量测量的情况。本文还介绍了用于纳米卫星Delfi-N3xt的Sun矢量确定子系统的开发。仿真和初步实验验证表明,该子系统由六个四象限太阳传感器组成,可以在没有地球反照率的情况下提供平均等效角误差约为0.2度的太阳航天器视线。在Delfi-N3xt的情况下,通过广泛的蒙特卡洛模拟对新型滤波器的性能进行了说明,其中沿着600公里高的太阳同步轨道获取了太阳矢量测量,地磁测量和陀螺仪测量。建议的滤波器似乎对不良的初始条件和低采样率不敏感。它会收敛在相同条件下标准扩展卡尔曼滤波器无法做到的地方。

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