Gravity model TUM-2Sp based on the energy balance approach and kinematic CHAMP orbits

被引:18
作者
Földváry, L [1 ]
Svehla, D [1 ]
Gerlach, C [1 ]
Wermuth, M [1 ]
Gruber, T [1 ]
Rummel, R [1 ]
Rothacher, M [1 ]
Frommknecht, B [1 ]
Peters, T [1 ]
Steigenberger, P [1 ]
机构
[1] Tech Univ, Inst Astron & Phys Geodasie, Munich, Germany
来源
EARTH OBSERVATION WITH CHAMP: RESULTS FROM THREE YEARS ORBIT | 2005年
关键词
gravity field; energy integral; kinematic orbit;
D O I
10.1007/3-540-26800-6_2
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
We have used one year of CHAMP data for deriving a gravity field model based on the energy balance approach. In order to avoid the use of any a priori gravity information; purely kinematic orbits have been computed from GPS measurements only subsequently, velocities have been derived from these kinematic positions by two different methods namely smoothing splines and Newton-Gregory interpolation. Using the principle of energy conservation, the satellite S positions and velocities are transformed into gravitational potential. CHAMP onboard micro-accelerometry is used to correct, for surface forces. For spherical harmonic analysis the so-called direct approach has been implemented using the full normal equation matrix. The model, called TUM2Sp, was found to be a more accurate gravity field than EIGEN-2 model.
引用
收藏
页码:13 / 18
页数:6
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