一种基于等频分形径向特征的神经网络星识别算法

Liang Wu, Kaixuan Zhang, Pengyu Hao, Dekun Cao
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引用次数: 0

摘要

星识别算法是星敏感器的核心算法。大视场星敏感器拍摄的星图中假星数量增加,星的位置偏移严重。提出了一种基于等频分形径向特征的神经网络星识别算法。EFB-RF是一个强大的恒星模式。采用浅表神经网络对EFB-RF进行分类。结果表明,该算法对定位噪声、假星和缺星具有较强的鲁棒性。该算法在1像素位置噪声下识别率可达99.92%,在5%假星情况下识别率可达99.37%。当缺失恒星的比例为15%时,可以达到99.97%。结果表明,该算法对大视场条件下的噪声、假星和缺星具有较强的鲁棒性,可以帮助星敏感器在复杂的空间环境下正常工作。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A Neural Network Star Identification Algorithm Based on Equal-Frequency Binning Radial Feature
Star identification algorithm is the core algorithm of star sensor. The number of false stars in the star image taken by the star sensor with wide Field-Of-View will increase, and the position of star will be seriously offset. This paper proposes a neural network star identification algorithm based on equal-frequency binning radial feature (EFB-RF). The EFB-RF is a robust star pattern. A superficial neural network is used to classify EFB-RF. The results show that our algorithm is robust to position noise, false stars, and missing stars. The identification rate of our algorithm can reach 99.92% under 1 pixel position noise, and it can reach 99.37% under 5% false stars. When the percentage of missing stars is 15%, it can reach 99.97%. The results show this algorithm is robust to position noise, false star and missing star in a wide-FOV, and it can help star sensor work properly in complex space environment.
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