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
相关论文
共 11 条
  • [1] A CHAMP-only gravity field model from kinematic orbits using the energy integral -: art. no. 2037
    Gerlach, C
    Földvary, L
    Svehla, D
    Gruber, T
    Wermuth, M
    Sneeuw, N
    Frommknecht, B
    Oberndorfer, H
    Peters, T
    Rothacher, M
    Rummel, R
    Steigenberger, P
    [J]. GEOPHYSICAL RESEARCH LETTERS, 2003, 30 (20) : SDE7 - 1
  • [2] High-resolution gravity field modeling with full variance-covariance matrices
    Gruber, T
    [J]. JOURNAL OF GEODESY, 2001, 75 (9-10) : 505 - 514
  • [3] The determination of gravitational potential differences from satellite-to-satellite tracking
    Jekeli, C
    [J]. CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY, 1999, 75 (02) : 85 - 101
  • [4] Kenyon S, 2002, IAG SYMP, V123, P391
  • [5] LEMOINE FG, 1998, NASATP199820686
  • [6] The CHAMP-only Earth gravity field model EIGEN-2
    Reigber, C
    Schwintzer, P
    Neumayer, KH
    Barthelmes, F
    König, R
    Förste, C
    Balmino, G
    Biancale, R
    Lemoine, JM
    Loyer, S
    Bruinsma, S
    Perosanz, F
    Fayard, T
    [J]. INTEGRATED SPACE GEODETIC SYSTEMS AND SATELLITE DYNAMICS, 2003, 31 (08): : 1883 - 1888
  • [7] Reigber C., 1999, Boll. Geof. Teor. Appl, V40, P285
  • [8] REIGBER C, 2003, UNPUB J GEODYN
  • [9] Kinematic precise orbit determination for gravity field determination
    Svehla, D
    Rothacher, M
    [J]. Window on the Future of Geodesy, 2005, 128 : 181 - 188
  • [10] Svehla D., 2003, ADV GEOSCIENCES, V1, P47, DOI DOI 10.5194/ADGEO-1-47-2003