航天工程大学, 北京 101416
刘洋,615323632@qq.com
徐灿,452394317@qq.com
收稿:2026-03-23,
修回:2026-04-08,
录用:2026-07-03,
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刘洋,徐灿,张雅声,等. 基于光度特征的GEO卫星状态分析方法研究[J].光子学报,2026,55(8):0804003
LIU Yang, XU Can, ZHANG YaSheng, et al. GEO Satellite Status Analysis Method Based on Photometric Characteristics[J]. Acta Photonica Sinica, 2026, 55(8):0804003
刘洋,徐灿,张雅声,等. 基于光度特征的GEO卫星状态分析方法研究[J].光子学报,2026,55(8):0804003 DOI: 10.3788/gzxb20265508.0804003. CSTR: 32255.14.gzxb20265508.0804003.
LIU Yang, XU Can, ZHANG YaSheng, et al. GEO Satellite Status Analysis Method Based on Photometric Characteristics[J]. Acta Photonica Sinica, 2026, 55(8):0804003 DOI: 10.3788/gzxb20265508.0804003. CSTR: 32255.14.gzxb20265508.0804003.
在完成实测地球静止轨道目标光度序列处理和状态标记的基础上,对地球静止轨道目标光学散射特性进行分析,提出并建立以时域特征、频域特征和样本熵特征组合的光度序列特征集,并对比传统机器学习方法和深度神经网络方法下各类特征的分类性能。采用多维度特征集后,随机森林、决策树、全连接神经网络、双向长短期记忆网络和支持向量机的分类准确率分别达到94.16%、90.58%、89.71%、89.29%和82.31%。研究成果对于实际工程中有效发现地球静止轨道卫星姿态异常具有支撑作用。
This study aims to develop a robust method for analyzing the attitude status of Geostationary Earth Orbit (GEO) satellites based on photometric data. Due to their high orbital altitude, ground-based telescopes cannot resolve imagery of GEO satellites, making photometric analysis a crucial technique for attitude monitoring. Existing methods primarily rely on time-series analysis but often lack comprehensive multi-dimensional feature extraction and validation. To address this gap, we propose constructing a photometric feature set that integrates time-domain, frequency-domain, and sample entropy characteristics. Furthermore, this study evaluates the classification performance of these features using both traditional machine learning algorithms and deep neural networks. The primary objective is to establish an effective and interpretable feature system that can reliably detect satellite attitude anomalies, thereby providing technical support for practical space situational awareness applications.To achieve this, the research methodology consists of four main components. First, we collected and preprocessed measured photometric data of GEO targets, performing state labeling to create a validated dataset containing both normal and anomalous satellite states. Second, we analyzed the optical scattering characteristics of high Earth orbit space targets to establish a theoretical foundation for feature selection. Based on this analysis, we constructed a multi-dimensional feature set comprising: (1) time-domain features (standard deviation/variance and fluctuation coefficient), which capture statistical characteristics and overall variability of light curves; (2) frequency-domain features (average amplitude, center frequency, and frequency variance), derived from power spectral density analysis to quantify periodic components and energy distribution patterns; and (3) sample entropy, a nonlinear metric that measures time series complexity and randomness. Third, we implemented five classification algorithms: three traditional machine learning methods (Support Vector Machine, Random Forest, and Decision Tree) and two deep neural network approaches (Bidirectional Long Short-Term Memory and Fully Connected Neural Network). Finally, we conducted controlled experiments to evaluate feature effectiveness through average classification accuracy, comparing single-feature performance, time-domain versus frequency-domain features, and the complete multi-dimensional feature set.Experimental results revealed several key findings regarding feature effectiveness. Frequency-domain features demonstrated superior discriminative power, with average amplitude achieving the highest single-feature classification accuracy of approximately 79.54%, significantly outperforming other individual features. The top three performing features were all frequency-domain characteristics, whereas time-domain features and sample entropy showed notably lower accuracy. Sample entropy performed poorly in this task with average accuracy around 60.25%, approaching random classification levels, likely due to measurement noise in normal satellite data increasing entropy values and obscuring distinctions. When comparing feature categories, frequency-domain features consistently outperformed time-domain features across all algorithms, with accuracy advantages of approximately 16 percentage points: Random Forest achieved 90.03% with frequency-domain features versus 73.40% with time-domain features; FCNN reached 86.04% versus 65.39%. Most importantly, the multi-dimensional feature set integrating time-domain, frequency-domain, and sample entropy characteristics achieved the highest classification performance across all algorithms: Random Forest reached 94.16%, Decision Tree achieved 90.58%, FCNN attained 89.71%, SVM reached 82.31%, and Bi-LSTM achieved 80.43%. This represents improvements of 4-6 percentage points over frequency-domain features alone, demonstrating the complementary nature of multi-dimensional features.These findings demonstrate that frequency-domain characteristics serve as the most reliable indicators for detecting GEO satellite attitude anomalies, with average amplitude identified as the optimal single-feature discriminator. The superior performance of frequency-domain features stems from their direct physical connection to satellite dynamics: normal attitude-stabilized satellites exhibit energy concentrated near zero frequency, while anomalous tumbling motion introduces periodic components that disperse spectral energy—a phenomenon that time-domain statistics cannot adequately capture. Multi-dimensional feature fusion significantly enhances classification performance by integrating complementary information: time-domain features capture overall statistical fluctuations, frequency-domain features quantify periodic structural changes, and nonlinear entropy measures signal complexity. These findings provide practical guidance for space object monitoring: prioritizing frequency-domain features while incorporating complementary dimensions offers the most effective approach for photometric-based satellite state diagnosis. Future work should focus on expanding anomalous state sample diversity and exploring alternative complexity metrics better suited to photometric data characteristics.
HU Yunpeng , LI Kebo , LIANG Yan'gang , et al . Review on strategies of space-based optical space situational awareness [J]. Journal of Systems Engineering and Electronics , 2021 , 32 ( 5 ): 1152 - 1166 .
DAO P . Automated algorithm to detect changes in geostationary satellite's configuration and cross-tagging [C]. Proceedings of the 2015 Advanced Maui Optical and Space Surveillance Technologies Conference (AMOS) , September 15-18, 2015 , Maui, HI, USA . 2015 : 377 .
臧晴 , 邹润 , 侯进永 , 等 . 一种判断卫星姿态变化的数据处理方法及装置 : CN118982736A [P]. 2024-11-19 .
邹润 , 臧晴 , 侯进永 , 等 . 一种分析高轨卫星轨道变化方法及装置 : CN118965227A [P]. 2024-11-15 .
SUKHOV P , YEPISHEV V P , MOTRUNICH I I , et al . Using photometric data to describe the behaviour of objects in geostationary orbit [J]. International Journal of Aerospace System Science and Engineering , 2025 , 1 ( 2 ): 157 - 171 .
LINARES R , FURFARO R , REDDY V . Space objects classification via light-curve measurements using deep convolutional neural networks [J]. The Journal of the Astronautical Sciences , 2020 , 67 : 1063 - 1091 .
LI Weixiao , ZHANG Yu , WANG Jianfeng , et al . Detecting anomalies in space-object light curves using temporal-attention LSTM [J]. Space Habitation , 2025 , 1 ( 2 ): 100007 .
DONG Haoqing , ZHANG Xuguo . Intelligent recognition method for space target based on photometric fingerprint features [J]. Spacecraft Recovery Remote Sensing , 2025 , 46 ( 6 ): 123 - 135 .
董昊卿 , 张绪国 . 基于光度指纹特征的空间目标智能识别方法 [J]. 航天返回与遥感 , 2025 , 46 ( 6 ): 123 - 135 .
MA R . Research on key feature inversion method of space objects based on photometric data from ground observatory [D]. Harbin : Harbin Institute of Technology , 2020 : 26 - 27 .
马若 . 基于地基光度信号的空间目标关键特征反演方法研究 [D]. 哈尔滨 : 哈尔滨工业大学 , 2020 : 8 - 9 .
DU Xiaoping , GENG Wendong , ZHAO Jiguang , et al . Space situational awareness fundamentals [M]. Beijing : National Defense Industry Press , 2017 : 97 - 123 .
杜小平 , 耿文东 , 赵继广 , 等 . 空间态势感知基础 [M]. 北京 : 国防工业出版社 , 2017 : 97 - 123 .
DU Junju . Photometric data acquisition and analysis of space debris [D]. Shandong : Shandong University , 2022 : 26 - 27 .
杜俊举 . 空间碎片光度数据的获取与分析 [D]. 山东 : 山东大学 , 2022 : 26 - 27 .
LI Zhi , XU Can , HUO Yurong , et al . Space target optical characteristics: principles and applications [M]. Beijing : Tsinghua University Press , 2024 : 107 - 110 .
李智 , 徐灿 , 霍俞蓉 , 等 . 空间目标光学特性原理与应用 [M]. 北京 : 清华大学出版社 , 2024 : 107 - 110 .
BOX G E P , JENKINS G M , REINSEL G C . Time series analysis: forecasting and control [M]. WANG Chengzhang, YOU Meifang, HAO Yang, et al., transl. 4th ed . Beijing : China Machine Press , 2011 : 328 - 352 .
乔治·博克斯 , 格威利姆·詹金斯 , 格雷戈里·莱因泽尔 . 时间序列分析: 预测与控制 [M]. 王成璋, 尤梅芳, 郝杨, 等, 译. 4版 . 北京 : 机械工业出版社 , 2011 : 328 - 352 .
WANG Yang , HU Min , DU Xiaoping , et al . Method for function determination of GEO spin stabilized objects by ground-based photometric data [J]. Journal of Beijing University of Aeronautics and Astronautics , 2025 , 51 ( 1 ): 113 - 119 .
王阳 , 胡敏 , 杜小平 , 等 . 地基光度数据判定GEO自旋稳定目标功能方法 [J]. 北京航空航天大学学报 , 2025 , 51 ( 1 ): 113 - 119 .
CHEN Shichao , LUO Feng , HU Chong , et al . Small target detection in sea clutter background based on tsallis entropy of doppler spectrum [J]. Journal of Radars , 2019 , 8 ( 3 ): 344 - 354 .
陈世超 , 罗丰 , 胡冲 , 等 . 基于多普勒谱非广延熵的海面目标检测方法 [J]. 雷达学报 , 2019 , 8 ( 3 ): 344 - 354 .
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