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Chapter 45 A New Celestial Positioning Model Based on Robust Estimation

机译:第45章一种基于鲁棒估计的新天体定位模型

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摘要

A large field of vision (FOV) star sensor can be used to image multiple celestial bodies at the same time, and then through center extraction of the star point and star patterns matching to realize navigation and positioning. The FOV based method has gradually become the main way of celestial navigation. However, in the process of center extraction, mistakenly identifying image noise as the star point and encountering some abnormal coordinate errors are inevitable. Meanwhile, in the process of star patterns matching, wrong matches are always encountered too. To solve these problems, this paper introduces the Robust Estimation for the first time, and based on it a celestial positioning model is established. The experiment shows that the model can effectively exclude the impact of noise and wrong patching, limit the abnormal observations, and take full advantage of high-precision observation information, by which positioning accuracy is increased from 4.05" to 1.15".
机译:可以使用大视野(FOV)星型传感器同时对多个天体成像,然后通过对星点进行中心提取和匹配星型来实现导航和定位。基于FOV的方法已逐渐成为天体导航的主要方式。然而,在中心提取的过程中,不可避免地会错误地将图像噪声识别为星点并遇到一些异常的坐标误差。同时,在星形匹配过程中,总是会遇到错误的匹配。为了解决这些问题,本文首次引入了鲁棒估计,并在此基础上建立了天体定位模型。实验表明,该模型可以有效地排除噪声和错误补丁的影响,限制异常观测,并充分利用高精度观测信息,将定位精度从4.05“提高到1.15”。

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