Calculating collision probability for long-term satellite encounters through the reachable domain method

IF 2.7 1区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Astrodynamics Pub Date : 2022-03-08 DOI:10.1007/s42064-021-0119-8
Changxuan Wen, Dong Qiao
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引用次数: 6

Abstract

Satellite encounters during close operations, such as rendezvous, formation, and cluster flights, are typical long-term encounters. The collision probability in such an encounter is a primary safety concern. In this study, a parametric method is proposed to compute the long-term collision probability for close satellite operations with initial state uncertainty. Random relative state errors resulting from system uncertainty lead to possible deviated trajectories with respect to the nominal one. To describe such a random event meaningfully, each deviated trajectory sample should be mapped to a unique and time-independent element in a random variable (RV) space. In this study, the RV space was identified as the transformed state space at a fixed initial time. The physical dimensions of both satellites were characterized by a combined hard-body sphere. Transforming the combined hard-body sphere into the RV space yielded a derived ellipsoid, which evolved over time and swept out a derived collision volume. The derived collision volume was solved using the reachable domain method. Finally, the collision probability was computed by integrating a probability density function over the derived collision volume. The results of the proposed method were compared with those of a nonparametric computation-intensive Monte Carlo method. The relative difference between the two results was found to be < 0.6%, verifying the accuracy of the proposed method.

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利用可达域法计算卫星长期碰撞概率
在交会、编队和集群飞行等近距离操作中,卫星遭遇是典型的长期遭遇。这种碰撞的碰撞概率是一个主要的安全问题。本文提出了一种计算具有初始状态不确定性的卫星近距离运行长期碰撞概率的参数化方法。由系统不确定性引起的随机相对状态误差可能导致轨迹偏离标称轨迹。为了有意义地描述这样的随机事件,每个偏离的轨迹样本都应该映射到随机变量(RV)空间中唯一且与时间无关的元素。本文将RV空间识别为固定初始时间的变换状态空间。这两颗卫星的物理尺寸特点是一个合并的硬体球体。将合并的硬体球体转换为RV空间产生了派生椭球,该椭球随着时间的推移而演变,并清除了派生的碰撞体积。采用可达域法求解得到的碰撞体积。最后,通过在导出的碰撞体积上积分概率密度函数来计算碰撞概率。将该方法的结果与非参数计算密集型蒙特卡罗方法的结果进行了比较。两个结果的相对差值为<0.6%,验证了所提出方法的准确性。
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来源期刊
Astrodynamics
Astrodynamics Engineering-Aerospace Engineering
CiteScore
6.90
自引率
34.40%
发文量
32
期刊介绍: Astrodynamics is a peer-reviewed international journal that is co-published by Tsinghua University Press and Springer. The high-quality peer-reviewed articles of original research, comprehensive review, mission accomplishments, and technical comments in all fields of astrodynamics will be given priorities for publication. In addition, related research in astronomy and astrophysics that takes advantages of the analytical and computational methods of astrodynamics is also welcome. Astrodynamics would like to invite all of the astrodynamics specialists to submit their research articles to this new journal. Currently, the scope of the journal includes, but is not limited to:Fundamental orbital dynamicsSpacecraft trajectory optimization and space mission designOrbit determination and prediction, autonomous orbital navigationSpacecraft attitude determination, control, and dynamicsGuidance and control of spacecraft and space robotsSpacecraft constellation design and formation flyingModelling, analysis, and optimization of innovative space systemsNovel concepts for space engineering and interdisciplinary applicationsThe effort of the Editorial Board will be ensuring the journal to publish novel researches that advance the field, and will provide authors with a productive, fair, and timely review experience. It is our sincere hope that all researchers in the field of astrodynamics will eagerly access this journal, Astrodynamics, as either authors or readers, making it an illustrious journal that will shape our future space explorations and discoveries.
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