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Research on the impact factors of GRACE precise orbit determination by dynamic method

机译:动态方法确定GRACE精确轨道的影响因素研究

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With the successful use of GPS-only-based POD (precise orbit determination), more and more satellites carry onboard GPS receivers to support their orbit accuracy requirements. It provides continuous GPS observations in high precision, and becomes an indispensable way to obtain the orbit of LEO satellites. Precise orbit determination of LEO satellites plays an important role for the application of LEO satellites. Numerous factors should be considered in the POD processing. In this paper, several factors that impact precise orbit determination are analyzed, namely the satellite altitude, the time-variable earth's gravity field, the GPS satellite clock error and accelerometer observation. The GRACE satellites provide ideal platform to study the performance of factors for precise orbit determination using zero-difference GPS data. These factors are quantitatively analyzed on affecting the accuracy of dynamic orbit using GRACE observations from 2005 to 2011 by SHORDE software. The study indicates that: (1) with the altitude of the GRACE satellite is lowered from 480 km to 460 km in seven years, the 3D (three-dimension) position accuracy of GRACE satellite orbit is about 3~4 cm based on long spans data; (2) the accelerometer data improves the 3D position accuracy of GRACE in about 1 cm; (3) the accuracy of zero-difference dynamic orbit is about 6 cm with the GPS satellite clock error products in 5 min sampling interval and can be raised to 4 cm, if the GPS satellite clock error products with 30 s sampling interval can be adopted. (4) the time-variable part of earth gravity field model improves the 3D position accuracy of GRACE in about 0.5-1.5 cm. Based on this study, we quantitatively analyze the factors that affect precise orbit determination of LEO satellites. This study plays an important role to improve the accuracy of LEO satellites orbit determination.
机译:随着仅基于GPS的POD(精确的轨道确定)的成功使用,越来越多的卫星携带GPS接收器来满足其轨道精度要求。它可以提供高精度的连续GPS观测,并成为获得LEO卫星轨道的必不可少的方法。 LEO卫星的精确轨道确定对于LEO卫星的应用起着重要作用。 POD处理中应考虑许多因素。本文分析了影响精确轨道确定的几个因素,即卫星高度,时变地球重力场,GPS卫星时钟误差和加速度计观测。 GRACE卫星为研究使用零差GPS数据进行精确轨道确定的因子的性能提供了理想的平台。通过使用SHORDE软件从2005年至2011年进行的GRACE观测,对影响动态轨道精度的这些因素进行了定量分析。研究表明:(1)随着GRACE卫星的高度在7年内从480 km降低到460 km,基于长跨度,GRACE卫星轨道的3D(三维)定位精度约为3〜4 cm数据; (2)加速度计数据将GRACE的3D定位精度提高了约1 cm; (3)如果采用30 s采样间隔的GPS卫星时钟误差乘积,零差动轨的精度在5分钟采样间隔内以GPS卫星时钟误差乘积为6 cm左右,可以提高到4 cm。 。 (4)重力场模型的时变部分将GRACE的3D定位精度提高了约0.5-1.5 cm。基于这项研究,我们定量分析了影响LEO卫星精确轨道确定的因素。这项研究对于提高LEO卫星轨道确定的准确性具有重要作用。

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