A Neural Network Star Identification Algorithm Based on Equal-Frequency Binning Radial Feature

Liang Wu, Kaixuan Zhang, Pengyu Hao, Dekun Cao
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Abstract

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.
一种基于等频分形径向特征的神经网络星识别算法
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。
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