Han Wang , Guoyi Zhang , Luyuan Wang , Siyang Chen , Zhihua Shen , Xia Yang , Xiangpeng Xu , Xiaohu Zhang
{"title":"Anomalous individuals searching framework for space debris detection in single optical astronomical image","authors":"Han Wang , Guoyi Zhang , Luyuan Wang , Siyang Chen , Zhihua Shen , Xia Yang , Xiangpeng Xu , Xiaohu Zhang","doi":"10.1016/j.asr.2024.11.057","DOIUrl":null,"url":null,"abstract":"<div><div>With the growing concern over space debris, effective space surveillance is significant to prevent potential collisions. Traditional approaches often design specific algorithms for distinct surveillance tasks, thereby neglecting the shared aspects across these tasks. Such methods frequently exhibit limited robustness, particularly when confronted with external interference or shifts in scene dynamics. This study introduces a space debris detection framework within single astronomical image, conceptualizing the task as an anomalous individuals searching challenge. The framework is structured around three core modules: individuals extraction, feature extraction and anomaly detection. Utilizing this framework, a versatile methodology is designed, which has been rigorously tested across two primary observational contexts. According to the similarity between ideal and actual imaging, our method begins by extracting sources within a normalized correlation space. It then compiles a comprehensive feature matrix for each source, encompassing motion, intensity, and morphological attributes. By exploiting the inherent low-rank characteristics and sparsity of the feature matrix, we identify foundational feature vectors for stars. Anomalous sources are subsequently identified via the Mahalanobis distance, facilitating the identification of targets. The method is validated through both simulated and actual observed datasets, with 97.7% average detection accuracy, outperforms than eight classical methods across various scenarios. Given the modular nature of the framework, each component can be refined to accommodate more complex situations. Moreover, the uniform anomaly scores generated offer valuable confidence for subsequent tracking algorithms, which underscore the potential of the framework in advancing practical space surveillance endeavors.</div></div>","PeriodicalId":50850,"journal":{"name":"Advances in Space Research","volume":"75 4","pages":"Pages 3820-3837"},"PeriodicalIF":2.8000,"publicationDate":"2025-02-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Advances in Space Research","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0273117724011888","RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
With the growing concern over space debris, effective space surveillance is significant to prevent potential collisions. Traditional approaches often design specific algorithms for distinct surveillance tasks, thereby neglecting the shared aspects across these tasks. Such methods frequently exhibit limited robustness, particularly when confronted with external interference or shifts in scene dynamics. This study introduces a space debris detection framework within single astronomical image, conceptualizing the task as an anomalous individuals searching challenge. The framework is structured around three core modules: individuals extraction, feature extraction and anomaly detection. Utilizing this framework, a versatile methodology is designed, which has been rigorously tested across two primary observational contexts. According to the similarity between ideal and actual imaging, our method begins by extracting sources within a normalized correlation space. It then compiles a comprehensive feature matrix for each source, encompassing motion, intensity, and morphological attributes. By exploiting the inherent low-rank characteristics and sparsity of the feature matrix, we identify foundational feature vectors for stars. Anomalous sources are subsequently identified via the Mahalanobis distance, facilitating the identification of targets. The method is validated through both simulated and actual observed datasets, with 97.7% average detection accuracy, outperforms than eight classical methods across various scenarios. Given the modular nature of the framework, each component can be refined to accommodate more complex situations. Moreover, the uniform anomaly scores generated offer valuable confidence for subsequent tracking algorithms, which underscore the potential of the framework in advancing practical space surveillance endeavors.
期刊介绍:
The COSPAR publication Advances in Space Research (ASR) is an open journal covering all areas of space research including: space studies of the Earth''s surface, meteorology, climate, the Earth-Moon system, planets and small bodies of the solar system, upper atmospheres, ionospheres and magnetospheres of the Earth and planets including reference atmospheres, space plasmas in the solar system, astrophysics from space, materials sciences in space, fundamental physics in space, space debris, space weather, Earth observations of space phenomena, etc.
NB: Please note that manuscripts related to life sciences as related to space are no more accepted for submission to Advances in Space Research. Such manuscripts should now be submitted to the new COSPAR Journal Life Sciences in Space Research (LSSR).
All submissions are reviewed by two scientists in the field. COSPAR is an interdisciplinary scientific organization concerned with the progress of space research on an international scale. Operating under the rules of ICSU, COSPAR ignores political considerations and considers all questions solely from the scientific viewpoint.