Gyroless attitude and rate estimation of small satellites using singular value decomposition and extended Kalman filter

C. Hajiyev, Demet Cilden, Y. Somov
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引用次数: 11

Abstract

This paper describes the development of a gyroless attitude determination system that can rely on magnetometer and sun sensor measurements and achieve good accuracy. Vectors coming from the selected sensor data and developed models can be placed in Wahba's problem. The system uses Singular Value Decomposition (SVD) method to minimize the Wahba's loss function and determine the attitude of the satellite. In order to obtain the attitude of the satellite with desired accuracy an extended Kalman filter (EKF) for satellite's angular motion parameter estimation is designed. The EKF uses this attitude information as the measurements for providing more accurate attitude estimates even when the satellite is in eclipse. The “attitude angle error covariance matrix” calculated for the estimations of the SVD method are regarded as the measurement noise covariance for the EKF. The SVD and EKF algorithms are combined to estimate the attitude angles and angular velocities, respectively. The algorithm can be used for low-cost small satellites where using high power consuming, expensive, and fragile gyroscopes for determining spacecraft attitude are not reasonable.
基于奇异值分解和扩展卡尔曼滤波的小卫星无陀螺姿态和速率估计
本文介绍了一种基于磁强计和太阳敏感器测量的无陀螺姿态测量系统的研制,该系统具有良好的精度。来自选定的传感器数据和开发的模型的向量可以放在Wahba的问题中。该系统采用奇异值分解(SVD)方法最小化Wahba损失函数,确定卫星姿态。为了获得精度要求的卫星姿态,设计了一种扩展卡尔曼滤波(EKF)用于卫星角运动参数估计。EKF使用这些姿态信息作为测量,即使在卫星处于日食状态时也能提供更准确的姿态估计。将SVD方法估计得到的“姿态角误差协方差矩阵”作为EKF的测量噪声协方差。结合SVD算法和EKF算法分别估计姿态角和角速度。该算法可用于低成本小卫星,在这种情况下,使用高功耗、昂贵且易损坏的陀螺仪来确定航天器姿态是不合理的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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