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改进的能量守恒方法及其在CHAMP重力场恢复中的应用

机译:改进的能量守恒方法及其在CHAMP重力场恢复中的应用

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摘要

An efficient method for gravity field determination from CHAMP orbits and accelerometer data is referred to as the energy balance approach. A new CHAMP gravity field recovery strategy based on the improved energy balance approach is developed in this paper. The method simultaneously solves the spherical harmonic coefficients, daily integration constant, scale and bias parameters. Two 60 degree and order gravitational potential models, XlSM-CHAMPOlS from the classical energy balance approach, and XISM-CHAMP02S from the improved energy balance, are determined using about one year's worth of CHAMP kinematic orbits from TUM and accelerometer data from GFZ. Comparisons among XISM-CHAMP01S, XlSM-CHAMP02S, EIGEN-CG03C, EIGEN-CHAMP03S, EIGEN2, ENIGN1S and EGM96 are made. The results show that the XlSM-CHAMP02S model is more accurate than EGM96, EiGEN1S, EIGEN2 and XISM-CHAMP01S at the same degree and order, and has almost the same accuracy as EIGEN-CHAMP03S.
机译:从Champ轨道和加速度计数据中的一种有效的重力场测定方法被称为能量平衡方法。本文开发了一种基于改进能量平衡方法的新的冠军重力场回收策略。该方法同时解决了球形谐波系数,每日集成常数,尺度和偏置参数。两个60度和订单的重力潜在模型,来自古典能量平衡方法的XLSM-Champol以及来自改善能量平衡的Xism-Champ02s,使用来自GFZ的Tum和加速度计数据的冠军运动轨道约一年的冠军运动轨道。 XISM-CHAMP01S,XLSM-CHAMP02S,EIGEN-CG03C,EIGEN-CHAMP03S,EIGEN2,ENIGN1和EGM96的比较。结果表明,XLSM-CHAMP02S模型比EGM96,EIGEN1,EIGEN2和XISM-CHAMP01S更加准确,定期和秩序,并且与eIGEN-CHAMP03S具有几乎相同的准确性。

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