基于直线与摆卫星编队组合的新一代hip-3s地球重力场模型精确建立

ZHENG Wei, XU Hou-Ze, LI Zhao-Wei, WU Fan
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引用次数: 1

摘要

由于干扰星间距离测量对地球重力场恢复精度的敏感性优于星间距离测量,本文建立了一种新的干扰星间距离法(DIRM)的观测方程。在此基础上,有效地验证了新一代“内摆-混合-三星”(HIP-3S)编队的轨道稳定性。研究结果表明,HIP-3S的形成足够稳定,可以进一步提高未来地球重力场模型的精度。最后,利用现有的GRACE-2S直线地层和基于新DIRM的下一代HIP-3S组合地层精确恢复了120度和120阶的地球重力场,在120度处的累积大地面高度误差分别为2.271×10−1 m和1.923×10−3 m。研究结果表明,未来HIP-3S的形成有助于建立具有更高精度和空间分辨率的下一代地球重力场模型。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
PRECISE ESTABLISHMENT OF THE NEXT-GENERATION EARTH GRAVITY FIELD MODEL FROM HIP-3S BASED ON COMBINATION OF INLINE AND PENDULUM SATELLITE FORMATIONS

Because the sensitivity of the disturbing intersatellite range measurements to the recovery accuracy of the Earth's gravitational field is superior to that of the intersatellite range measurements, the observation equation of a new Disturbing Intersatellite Range Method (DIRM) is created in this study. Then the orbital stability of the next-generation Hybrid-Inline-Pendulum-Three-Satellite (HIP-3S) formation is efficiently verified. The research results indicate that the HIP-3S formation is sufficiently steady for further enhancing the accuracy of the future Earth gravity field model. Finally, the Earth's gravitational field complete up to degree and order 120 is precisely recovered by the current GRACE-2S inline formation and the next-generation HIP-3S combined formation based on the new DIRM, and the cumulative geoid height errors are 2.271×10−1 m and 1.923×10−3 m at degree 120, respectively. The study results show that the future HIP-3S formation is helpful for producing the next-generation Earth gravity field model with higher accuracy and spatial resolution.

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