Calculating the quasi-periodic distant retrograde orbit under the ephemeris model based on the adaptive two-level differential correction

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Yujie Chen, Yanwei Zhu, Meichen Chan, Chenyuan Qiao, Haipeng Qiu
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引用次数: 0

Abstract

Research on the dynamics of multi-body motion in the Earth-Moon space is a crucial area in current spacecraft motion studies. Distant Retrograde Orbits (DROs) are highly valuable trajectories in the Earth-Moon space. Under the ephemeris model, DROs will become quasi-periodic. Efficiently computing quasi-periodic DROs in the ephemeris model is a pressing issue. This paper addresses the problems of high computational time cost and significant divergence over multiple orbit cycles when calculating quasi-periodic DROs under the ephemeris model and proposes an adaptive two-level differential correction algorithm based on differential evolution. The traditional two-level differential correction selects patch points at equal intervals, while the DRO states are different with different amplitudes, choosing patch points at equal intervals is simple but not suitable for most DRO. Each quasi-periodic DRO should have its own patch points position. The adaptive two-level differential correction algorithm firstly uses differential evolution to obtain the optimal solution of the position of the patch points and then two-level differential correction is played. This algorithm significantly improving both computational efficiency and orbital convergence. Simulation results show that this algorithm significantly reduces computational costs and achieves better convergence compared to traditional two-level differential correction algorithm. This study has a reference value for the design of long-term quasi-periodic DRO, and provides a new idea for the selection strategy of patch points in the two-level differential correction algorithm and the multiple shooting algorithm.

Abstract Image

基于自适应两级差分校正的星历模型下的准周期远距离逆行轨道计算
地月空间多体运动动力学研究是当前航天器运动研究的一个重要领域。遥远逆行轨道是地月空间中非常有价值的轨道。在星历模型下,ro将变成准周期的。有效地计算星历模型中的准周期ro是一个迫切需要解决的问题。针对星历模型下拟周期ro计算时计算时间大、多轨道周期发散大的问题,提出了一种基于差分进化的自适应两级差分校正算法。传统的两级差分校正选择等间隔的贴片点,而不同幅度的贴片状态不同,选择等间隔的贴片点简单,但不适合大多数的贴片点。每个准周期DRO应该有自己的贴片点位置。自适应两级差分校正算法首先利用差分进化得到补丁点位置的最优解,然后进行两级差分校正。该算法显著提高了计算效率和轨道收敛性。仿真结果表明,与传统的两级差分校正算法相比,该算法显著降低了计算量,具有更好的收敛性。该研究对长期准周期DRO的设计具有参考价值,并为两级差分校正算法和多次射击算法中的补点选择策略提供了新的思路。
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来源期刊
Astrophysics and Space Science
Astrophysics and Space Science 地学天文-天文与天体物理
CiteScore
3.40
自引率
5.30%
发文量
106
审稿时长
2-4 weeks
期刊介绍: Astrophysics and Space Science publishes original contributions and invited reviews covering the entire range of astronomy, astrophysics, astrophysical cosmology, planetary and space science and the astrophysical aspects of astrobiology. This includes both observational and theoretical research, the techniques of astronomical instrumentation and data analysis and astronomical space instrumentation. We particularly welcome papers in the general fields of high-energy astrophysics, astrophysical and astrochemical studies of the interstellar medium including star formation, planetary astrophysics, the formation and evolution of galaxies and the evolution of large scale structure in the Universe. Papers in mathematical physics or in general relativity which do not establish clear astrophysical applications will no longer be considered. The journal also publishes topically selected special issues in research fields of particular scientific interest. These consist of both invited reviews and original research papers. Conference proceedings will not be considered. All papers published in the journal are subject to thorough and strict peer-reviewing. Astrophysics and Space Science features short publication times after acceptance and colour printing free of charge.
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