旋转小卫星的磁强计姿态估计

Halil Ersin Söken, S. Sakai
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引用次数: 1

摘要

自旋稳定提供了一种简单的姿态控制解决方案,特别是对于微型和纳米卫星,并且在许多任务中具有很大的实施潜力。提出了一种自旋卫星姿态估计算法。该算法松散地基于Bar-Itzhack和Harman提出的滤波器。利用简单的卡尔曼滤波(KF)算法,仅利用磁力计测量,估计了卫星的自转轴和速率。为了提高磁强计自转轴估计的精度,采用偏置估计算法对磁强计测量结果进行了校正。两种算法,姿态滤波和磁强计偏置估计,通过合并它们作为一个单一的KF算法,以一种简单的方法集成。因此,提出了一种估计自旋参数和磁强计偏置项的伪线性KF算法。通过数值模拟对该算法进行了验证。对结果进行了详细的讨论,并对算法的实现提出了建议。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Magnetometer only attitude estimation for spinning small satellites
Spin-stabilization offers a simple attitude control solution, specifically for micro and nanosatellites, and has a large potential for implementation on numerous missions. This paper proposes an attitude estimation algorithm for spin satellites. The algorithm is loosely based on a filter proposed by Bar-Itzhack and Harman. Using a simple Kalman filter (KF) algorithm and only the magnetometer measurements, the spin axis and rate of the satellite are estimated. To improve the spin axis estimation accuracy the magnetometer measurements are corrected with a bias estimation algorithm. Two algorithms, the attitude filter and the magnetometer bias estimator, are integrated with a straightforward approach by merging them as a single KF algorithm. As a result, a pseudo-linear KF algorithm that estimates the spin parameters together with magnetometer bias terms is proposed. The algorithm is tested for a hypothetical nanosatellite via numerical simulations. The results are discussed in detail and suggestions for implementation of the algorithm are given.
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