高效的卫星定轨算法

M. El-Mahy
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引用次数: 3

摘要

当卫星穿过夜空时,它们看起来就像移动的星星,观测者可以用双筒望远镜、巨型雷达和大型摄像机精确地跟踪它们。本文将迭代扩展卡尔曼滤波(IEKF)应用于低空(300 km)、近圆(e=0.0003)、倾角为50/spl°/的卫星定轨问题。这颗卫星受到明显的扰动加速度的影响。利用地面雷达的实际卫星跟踪数据,计算了算法的性能、精度、效率、估计误差和预测误差。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Efficient satellite orbit determination algorithm
Satellites as they cross the night sky look like moving stars, which can be accurately tracked by an observer with binoculars as well as by giant radars and large cameras. In this paper, the iterated extended Kalman filter (IEKF) is applied to the problem of satellite orbit determination for a low altitude (300 km), nearly circular (e=0.0003), orbit with an inclination of 50/spl deg/. The satellite is subject to significant perturbing accelerations. The performance, accuracy, efficiency, estimation errors, and prediction errors of the algorithm are calculated using actual satellite tracking data obtained from ground based radars.
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