面向地球重力场精细反演的时空极倾斜空间任务架构

B. Elsaka
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引用次数: 1

摘要

在过去的几年里,未来的卫星重力任务(fgm)已经被深入研究,以超越之前成功的GRACE和目前的GRACE后续卫星任务。以往的研究已经对不同轨道高度为几公里、不同重复轨道周期的两对卫星组合(这里称为PI-FGM,即像GRACE任务一样的单极卫星对与另一倾斜卫星对的组合)重力场恢复进行了研究。本文提出了一种新颖的设计思路,即采用平移的ST-FGM轨道参数,设计具有相同极型轨道高度的FGM倾斜卫星对,以避免FGM结构中两颗倾斜卫星对之间可能发生的碰撞风险。重复轨道问题将通过手稿加以考虑,并将设置为尽可能相同,以进行公平比较。全尺寸仿真分析结果表明,新设计的位移时空极斜(ST-FGM)任务结构基本优于两对不同轨道高度卫星(即PI-FGM任务结构)。在重力场恢复方面,ST-FGM架构反演的大地水准面高度标准差约为17.0 mm,具有更好的各向同性误差分布。ST-FGM和PI-FGM任务架构在grace -类地层方面分别提供了约80和60倍的总体改进,在半径400公里处使用高斯滤波器的平滑重力解方面分别提供了约2.4和1.8倍的改进。因此,位移时空极倾角(ST-FGM)作为稳定的任务架构值得推荐,并可作为未来的重力任务之一考虑。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Spatio-Temporal Polar-Inclined Space Mission Architecture for a Refined Retrieve of the Earth’s Gravity Field
Future satellite gravity missions (FGMs) have been intensively studied during the last recent years for the era beyond the successful previous GRACE and current GRACE Follow-on satellite missions. Previous studies have investigated the gravity field recovery derived from combined two satellite-pairs (referred here as PI-FGM, a single polar satellite-pair like the GRACE mission combined with another inclined satellite-pair) with different orbital heights of few kilometers and different repeat orbital periods. In this contribution, new innovative idea is introduced by designing the inclined satellite-pair of the FGM at the same orbital height of the polar-type with shifted spatio-temporal (ST-FGM) orbital parameters to avoid any possible collision risk between the two satellite-pairs, polar and inclined, of the FGM architecture. The repeat orbits issue will be taken into consideration through the manuscript and will be set as identical as possible for a fair comparison. The findings through a full-scale simulation analysis show that the new design of shifted spatio-temporal polar-inclined (ST-FGM) mission architecture basically outperforms the two satellite-pairs having different orbital heights (i.e. the PI-FGM mission configuration). Regarding the gravity field recovery, the ST-FGM architecture retrieves the geoid heights with standard deviations of about 17.0 mm providing more isotropic error distribution. An overall improvement by a factor of about 80 and 60 is provided by the ST-FGM and PI-FGM mission architectures, respectively, with respect to the GRACE-like formation and a factor of about 2.4 and 1.8, respectively, with respect to the smoothed gravity solution using the Gaussian filter at radius 400 km. Therefore, the shifted spatio-temporal polar-inclined (ST-FGM) is worthy recommended as stable mission architecture and would be considered as one of the future gravity missions.
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