轨道不确定性估计支持自主空间碎片观测

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
H. Jiang, J. Liu, H. Cheng
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引用次数: 0

摘要

空间碎片的不断增加给现有空间系统和人类空间飞行带来了巨大的冲击风险。准确了解空间碎片轨道传播误差对于空间监视网络任务分配、连接分析等多种用途都是必不可少的。不幸的是,传播误差不适用于双线元素(TLE)。本文提出了一种基于神经网络模型的TLE不确定性估计方法。将目标属性、空间环境和预测时间跨度作为网络的输入,将下程方向、法线方向和法线方向的传播误差作为网络的输出。为了保证选定的训练轨道不稳定,只使用碎片和火箭体。通过一些具有连续TLE数据的对象验证了该网络的有效性。结果表明,该方法具有精度高、计算速度快、鲁棒性好等优点,适用于星表中任何目标,特别是新发射的目标。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
ORBITAL UNCERTAINTY ESTIMATION SUPPORT FOR AUTONOMOUS SPACE DEBRIS OBSERVATION
The continually increased space debris have posed great impact risks to existing space systems and human space flight. Accurate knowledge of propagation errors of space debris orbit is essential for many types of uses, such as space surveillance network tasking, conjunction analysis etc. Unfortunately, propagation error is not available for a two-line element (TLE). In this paper, a new TLE uncertainty estimation method based on neural network model is proposed. Object properties, space environment and predicted time-span are considered as the input of the network, the propagation errors in the direction of downrange, normal and conormal are as the output of the network. In order to assure the chosen orbit for training is not stable, only debris and rocket bodies are used. The network's effciency is demonstrated with some objects with continuous TLE data. Overall, the method proves accurate, computationally fast, and robust, and is applicable to any object in the satellite catalogue, especially for those newly launched objects.
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来源期刊
Revista Mexicana de Astronomia y Astrofisica
Revista Mexicana de Astronomia y Astrofisica 地学天文-天文与天体物理
CiteScore
1.30
自引率
10.00%
发文量
14
审稿时长
>12 weeks
期刊介绍: The Revista Mexicana de Astronomía y Astrofísica, founded in 1974, publishes original research papers in all branches of astronomy, astrophysics and closely related fields. Two numbers per year are issued and are distributed free of charge to all institutions engaged in the fields covered by the RMxAA.
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