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使用支持向量机(SVM)和长短期记忆网络(LSTM)对近地轨道(LEO)常驻空间物体(RSO)的光曲线进行分类

Classification of Low Earth Orbit (LEO) Resident Space Objects' (RSO) Light Curves Using a Support Vector Machine (SVM) and Long Short-Term Memory (LSTM).

作者信息

Qashoa Randa, Lee Regina

机构信息

Department of Earth and Space Science, York University, Toronto, ON M3J 1P3, Canada.

出版信息

Sensors (Basel). 2023 Jul 20;23(14):6539. doi: 10.3390/s23146539.

DOI:10.3390/s23146539
PMID:37514833
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC10384663/
Abstract

Light curves are plots of brightness measured over time. In the field of Space Situational Awareness (SSA), light curves of Resident Space Objects (RSOs) can be utilized to infer information about an RSO such as the type of object, its attitude, and its shape. Light curves of RSOs in geostationary orbit (GEO) have been a main research focus for many years due to the availability of long time series data spanning hours. Given that a large portion of RSOs are in low Earth orbit (LEO), it is of great importance to study trends in LEO light curves as well. The challenge with LEO light curves is that they tend to be short, typically no longer than a few minutes, which makes them difficult to analyze with typical time series techniques. This study presents a novel approach to observational LEO light curve classification. We extract features from light curves using a wavelet scattering transformation which is used as an input for a machine learning classifier. We performed light curve classification using both a conventional machine learning approach, namely a support vector machine (SVM), and a deep learning technique, long short-term memory (LSTM), to compare the results. LSTM outperforms SVM for LEO light curve classification with a 92% accuracy. This proves the viability of RSO classification by object type and spin rate from real LEO light curves.

摘要

光变曲线是随时间测量的亮度图。在空间态势感知(SSA)领域,常驻空间物体(RSO)的光变曲线可用于推断有关RSO的信息,例如物体类型、姿态和形状。由于有长达数小时的长时间序列数据,地球静止轨道(GEO)中RSO的光变曲线多年来一直是主要研究重点。鉴于很大一部分RSO处于低地球轨道(LEO),研究LEO光变曲线的趋势也非常重要。LEO光变曲线的挑战在于它们往往很短,通常不超过几分钟,这使得使用典型的时间序列技术对其进行分析变得困难。本研究提出了一种用于观测LEO光变曲线分类的新方法。我们使用小波散射变换从光变曲线中提取特征,该变换用作机器学习分类器的输入。我们使用传统机器学习方法(即支持向量机(SVM))和深度学习技术(长短期记忆(LSTM))进行光变曲线分类,以比较结果。对于LEO光变曲线分类,LSTM的表现优于SVM,准确率达到92%。这证明了根据真实LEO光变曲线按物体类型和自旋速率对RSO进行分类的可行性。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cbdf/10384663/78d7c902e93b/sensors-23-06539-g008.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cbdf/10384663/626fd8513f5f/sensors-23-06539-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cbdf/10384663/c3bce05fac5d/sensors-23-06539-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cbdf/10384663/ef59f0a9d04c/sensors-23-06539-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cbdf/10384663/0d7f053346fc/sensors-23-06539-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cbdf/10384663/910b76ff36ef/sensors-23-06539-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cbdf/10384663/c7ab848a4833/sensors-23-06539-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cbdf/10384663/02a48e9c249d/sensors-23-06539-g007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cbdf/10384663/78d7c902e93b/sensors-23-06539-g008.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cbdf/10384663/626fd8513f5f/sensors-23-06539-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cbdf/10384663/c3bce05fac5d/sensors-23-06539-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cbdf/10384663/ef59f0a9d04c/sensors-23-06539-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cbdf/10384663/0d7f053346fc/sensors-23-06539-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cbdf/10384663/910b76ff36ef/sensors-23-06539-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cbdf/10384663/c7ab848a4833/sensors-23-06539-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cbdf/10384663/02a48e9c249d/sensors-23-06539-g007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cbdf/10384663/78d7c902e93b/sensors-23-06539-g008.jpg

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