一种基于特征向量的快速星图识别算法

Qi-Shen Li, Chang-ming Zhu, Jun Guan
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引用次数: 3

摘要

星图中的星星可以看作是一个点模式,我们可以利用点模式的匹配来识别星图。首先提出了平移、旋转和缩放不变性的第n个半径加权平均点(rwmp),然后构造了平移和旋转不变性的基于rwmp的特征向量。通过计算观测到的星图与模式数据库中各星图之间的欧氏距离,得到候选参考星图及其对应的姿态。介绍了验证过程,对识别结果进行了验证。仿真结果表明,在0 ~ 3像素的相同位置噪声水平下,与网格算法相比,该算法的平均识别率提高了3.5%,识别时间减少到1/5。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A fast star pattern recognition algorithm based on feature vector
Stars in a star map can be regarded as a point pattern, and we can utilize the matching of point pattern to recognize the star pattern. First, the nth Radius-Weighted-Mean Points (RWMPs) are proposed which are invariant to translation, rotation and scaling, and then, a RWMP-based feature vector is constructed which is still invariant to translation and rotation. The candidate referenced star images and their corresponding attitudes are obtained by computing the Euclidean distance between the viewed star image and each of the star images in the pattern database. The verification process is introduced to confirm the identification results. The simulation results indicates that the average identification rate of this algorithm can be enhanced 3.5% as compared to the grid algorithm at the same position noise level from 0 to 3 pixels, and the identification time of the proposed algorithm reduces to 1/5.
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