基于类星体星座的时变重力场恢复模拟分析

IF 2.8 3区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS Geophysical Journal International Pub Date : 2024-08-16 DOI:10.1093/gji/ggae273
Youjian Liu, Jiancheng Li, Xinyu Xu, Hui Wei, Zhao Li, Yongqi Zhao
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引用次数: 0

摘要

摘要 时变重力场在理解和分析地球动力过程,特别是物质在地球表面的迁移过程中起着至关重要的作用。然而,目前时空分辨率的限制阻碍了对其的准确表述。在这种情况下,利用巨型低轨道卫星群以高时空分辨率准确恢复时变重力场具有巨大潜力。根据星链星座第一阶段配置的 123 个不同轨道平面上 5199 颗卫星的轨道参数和下一代重力任务中本德尔星座的轨道参数,我们进行了闭环模拟,利用短弧积分法分析了 9 天内时变重力场的恢复能力。数值模拟中考虑了AOHIS信号(大气、海洋、水文、冰和固体地球)、海洋潮汐模型、轨道位置、卫星间距率和加速度计观测数据的混叠误差。与 Bender 星座相比,在不考虑观测噪声的情况下,类 Starlink 星座能有效降低空间和频率域的混叠误差。在考虑观测噪声的情况下,与 Bender 星座相比,Starlink-like 星座还能有效提高时变重力场模型的低度系数(15 度以下)的可靠性,并呈现更高的全度球面谐波解的时间分辨率(9 天以内)。通过合并类星体星座和本德尔星座,可显著降低本德尔星座低度部分的混叠效应,恢复的 30 度以内时变重力场精度可提高约 0.5 ∼ 1 个数量级。我们的研究结果可为未来重力卫星任务的设计提供技术参考。
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Simulation analysis of recovering time-varying gravity fields based on Starlink-like constellation
Summary Time-varying gravity fields play a crucial role in understanding and analyzing geodynamic processes, particularly the migration of matter across the Earth's surface. However, the current limitations in spatiotemporal resolution hinder their accurate representation. In this context, the use of a giant constellation of low-orbit satellites holds great potential for accurately recovering time-varying gravity fields with high spatiotemporal resolution. Based on the orbital parameters of 5199 satellites in 123 different orbital planes in the first phase configuration of the Starlink constellation and the orbital parameters of the Bender constellation in the next generation gravity mission, we conducted a closed-loop simulation to analyze the recovery ability of time-varying gravity field in 9 days using the short-arc integral method. The errors of aliasing AOHIS signal (Atmosphere, Ocean, Hydrology, Ice, and Solid Earth), ocean tide models, orbit positions, inter-satellite range rates, and accelerometer observations were considered in the numerical simulation. Compared with the Bender constellation, the Starlink-like constellation can effectively decrease the aliasing errors in the spatial- and frequency-domain when the observation noise is not considered. The Starlink-like constellation can also effectively improve the reliability of low-degree coefficients (below degree 15) of retrieved time-varying gravity field models and present higher time resolution (within 9 days) for the full degree spherical harmonic solutions than the Bender constellation when the observation noise is considered. The aliasing effect on the low-degree part of the Bender constellation can be significantly decreased by combining the Starlink-like and Bender constellations, and the accuracy of the recovered time-varying gravity field within degree 30 can be improved by about 0.5 ∼ 1 order of magnitude. Our results can provide a technical reference for the design of future gravity satellite mission.
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来源期刊
Geophysical Journal International
Geophysical Journal International 地学-地球化学与地球物理
CiteScore
5.40
自引率
10.70%
发文量
436
审稿时长
3.3 months
期刊介绍: Geophysical Journal International publishes top quality research papers, express letters, invited review papers and book reviews on all aspects of theoretical, computational, applied and observational geophysics.
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