基于方差分量估计的CHAMP重力场恢复方法

基于德国慕尼黑技术大学(TUM)提供的100 d的CHAMP卫星几何法轨道和GFZ提供的加速度计数据,计算出了50×50阶地球重力场模型XISM-CHAMP01,并与EIGEN-CG03C、EIGEN-CHAMP03S、EIGEN2、EIGEN1S、EGM96模型进行了比较。结果表明,XISM-CHAMP01模型精度明显优于相同阶次EGM96模型和EIGEN1S模型,并与EIGEN2模型精度相当。     

使用能量守恒方法恢复CHAMP地球重力场

本文探讨了基于能量守恒方法利用CHAMP卫星精密星历和加速度数据恢复地球重力场模型的原理和方法。给出了地心惯性系下顾及地球自转和非保守力能量损耗的能量守恒方程,并且对日、月摄动位与引潮力附加位的计算方法作了相应的分析,同时介绍了加速度数据的处理方法。基于能量守恒方法,利用2002年1-2月、7-8月和11-12月三个不同时期共180天的CHAMP卫星精密星历和加速度数据恢复了三组50阶次的地球重力场模型GFM01、GFM02和GFM03,并将这些模型与EGM 96重力场模型和GFZ公布的EIGEN-CG01C重力场模型进行比较。结果表明:能量守恒方法恢复的GFM系列模型与EGM 96重力场模型及EIGEN-CG01C重力场模型在低阶位系数上均有较好的一致,但与EIGEN-CG01C模型有更好的一致。这说明了CHAMP卫星对地球中、长波重力场的敏感性,也说明了能量守恒方法恢复低阶地球重力场位系数的有效性。     

利用CHAMP科学轨道数据和星载加速度计数据反演地球重力场

基于卫星动力学理论,采用德国地球科学中心GFZ提供的CHAMP精密轨道数据和星载加速度计数据,反演了36阶地球重力场模型CDS01S。用不同模型之间的位系数差比较模型CDS01S、EIGEN3P、EIGEN1S及EGM96,表明CDS01S模型的位系数最接近于EIGEN3P;比较上述几种模型的位系数精度,表明CDS01S模型的位系数精度高于EGM96;用CDS01S和GGM01C的前30阶位系数分别计算全球2°×2°网格的大地水准面起伏,两者之间的标准偏差为4.7 cm。     

利用现有重力场模型求定CHAMP卫星加速度计修正参数

CHAMP卫星加速度计数据的标定是通过确定其尺度因子和偏差参数来完成的.本文基于能量守恒方程,给出利用现有重力场模型标定CHAMP卫星加速度数据的基本原理和数学模型;提出相邻历元间差分算法,大大简化了观测方程,同时避免积分常量的计算.该算法既能同时解算尺度因子和偏差参数,也可任意求解其中之一.基于实测的CHAMP卫星加速度数据,利用EGM96模型和最新公布的EIGEN-2模型进行计算与比较,验证该方法的有效性.     

利用CHAMP卫星轨道和加速度计数据推求地球重力场模型

本文紧密结合当前卫星重力测量技术的发展需求，围绕利用CHAMP卫星轨道和加速度计数据恢复地球重力场展开研究，重点在CHAMP数据预处理、重力场恢复、正则化算法等方面进行了理论和实践上的系统研究，建立了一套完整的CHAMP重力场恢复理论和算法。论文的主要内容和创新点概括如下：     

利用CHAMP卫星星历及加速度计数据推求地球重力场模型

讨论基于CHAMP卫星星历和加速度计数据推求地球重力场模型的数值微分算法.首先利用牛顿内插公式,根据CHAMP卫星星历观测值求解卫星运动加速度.在计算卫星加速度时,建议采用速度数据内插加速度.扣除其他非地球引力摄动加速度后,基于牛顿运动定律建立观测方程.利用GFZ数据中心提供的24天CHAMP星历数据和加速度计数据解算出50×50阶地球重力场模型,并与EGM96模型进行比较,结果表明两者在低阶位系数上有较好的一致性.     

利用CHAMP卫星轨道和加速度计数据恢复重力场方法概述

回顾了目前利用CHAMP卫星轨道和加速度计数据恢复地球重力场模型的各种方法；从观测值、观测方程和解算方法三个方面，对现有各种CHAMP重力场模型恢复方法进行了详细的归纳与分类，并指出了各方法的优缺点。     

利用CHAMP卫星轨道和加速度计数据推求地球重力场模型

本文紧密结合当前卫星重力测量技术发展需求,围绕利用CHAMP轨道和加速度计数据恢复地球重力场展开研究,重点在CHAMP数据预处理、重力场恢复、正则化算法等方面进行了理论和实践上的系统研究,建立了一套完整的CHAMP重力场恢复理论和算法.论文的主要创新点有:     

改进的能量守恒方法及其在CHAMP重力场恢复中的应用(英文)

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, XISM-CHAMPO1S from the classical energy balance approach, and XISM-CHAMPO2S 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-CHAMPO1S, XISM-CHAMPO2S, EIGEN-CGO3C, EIGEN-CHAMPO3S, EIGEN2, ENIGNIS and EGM96 are made. The results show that the XISM-CHAMPO2S model is more accurate than EGM96, EIGENIS, EIGEN2 and XISM-CHAMPO1S at the same degree and order, and has almost the same accuracy as EIGEN-CHAMPO3S.     

大地测量

CH20051284 基于能量守恒方法恢复CHAMP重力场模型=CHAMP GRAVITY FIELD RECOVERY USING ENERGY CONSER- VATION METHOD／徐天河,杨元喜(西安测绘研究所)／／测绘学报．-2005,34(1)．-1-6 介绍了基于能量守恒定律恢复地球重力场模型的基本原理和算法。指出CHAMP加速度计数据存在的问     

Earth gravity field recovered from CHAMP science orbit and accelerometer data

IntroductionSince the launch of man-made satellite early in1957 ,the research for satellite gravity has beentaken a wide attentioninfield of geodesy .Early ,the ground-based satellite tracking has providedan observational data set which has been used tode…     

Earth gravity field recovered from CHAMP science orbit and accelerometer data

The earth gravity field model CDS01S of degree and order 36 has been recovered from the post processed Science Orbits and on-board accelerometer data of GFZ's CHAMP satellite. The model resolves the geoid with an accuracy of better than 4 cm at a resolution of 700 km half-wavelength. By using the degree difference variances of geopotential coefficients to compare the model CDS01S with EIGEN3P, EIGEN1S and EGM96, the result indicates that the coefficients of CDS01S are most close to those of EIGEN3P. The result of the comparison between the accuracies of geopotential coefficients in the above models, indicates that the accuracy of coefficients in CDS01S is higher than that in EGM96. The geoid undulations of CDS01S and GGM01C up to 30 degrees are calculated and the standard deviation is 4. 7 cm between them.     

Calibration for CHAMP Accelerometer Data Based on Crossover Points of the Satellite

The German CHAlleging Minisatellite Payload （CHAMP） was launched in July 2000. It is the first satellite that provides us with position and accelerometer measurements, with which the gravity field model can be determined. One of the most popular methods for geopotential recovery using the position and accelerometer measurements of CHAMP is the energy conservation method, The main aim of this paper is to determine the scale and bias parameters of CHAMP accelerometer data using the energy conservation method. The basic principle and mathematical model using the crossover points of CHAMP orbit to calibrate the accelerometer data are given based on the energy balance method. The rigorous integral formula as well as its discrete form of the observational equation is presented, This method can be used to estimate only one of the scale and bias parameters or both of them. In order to control the influence of outliers, the robust estimator for the calibration parameters is given. The results of the numerical computations and comparisons using the CHAMP accelerometer data show the validity of the method.     

利用卫星轨迹交叉点标定CHAMP卫星加速度计数据

基于能量守恒方程给出了利用卫星轨迹交叉点标定CHAMP卫星加速度数据的基本原理和方法 ,并给出了其严密的积分公式及其离散化形式。为了控制加速度数据的扰动异常 ,建议采用抗差估计求解参数值 ,并基于实测的CHAMP卫星加速度计数据进行了计算与比较 ,验证了该方法的有效性     

Accuracy analysis for SST gravity field model in China

Taking China as the region for test the potential of the new satellite gravity technique, satelliteto-satellite tracking for improving the accuracy of regional gravity field model is studied. With WDM94 as reference, the gravity anomaly residuals of three models, the latest two GRACE global gravity field model (EIGEN_GRACE02S, GGM02S) and EGM96, are computed and compared. The causes for the differences among the residuals of the three models are discussed. The comparison between the residuals shows that in the selected region, EIGEN_GRACE02S or GGM02S is better than EGM96 in lower degree part (less than 110 degree). Additionally, through the analysis of the model gravity anomaly residuals, it is found that some systematic errors with periodical properties exist in the higher degree part of EIGEN and GGM models, the results can also be taken as references in the validation of the SST gravity data.     

中国区域SST卫星重力场模型精度分析

通过比较最新SST地球重力场模型EIGEN_GRACE02S、GGM02S和EGM96模型在中国区域与WDM94模型重力异常残差的差异，分析差异产生的原因及分布，研究新一代卫星重力方法对于提高区域重力场模型精度的潜力以及存在的问题。结果证明，卫星跟踪卫星方法对于现有模型中低阶部分有明显改善。