Gravity model TUM-2sp based on the energy balance approach and kinematic CHAMP orbits (CROSBI ID 29672)
Prilog u knjizi | izvorni znanstveni rad
Podaci o odgovornosti
Földvary, L. ; Švehla, Dražen ; Gerlach, Ch. ; Wermuth, M. ; Gruber, Th. ; Rummel, R. ; Rothacher, M. ; Frommknecht, B. ; Peters, Th. ; Steigenberger, P.
engleski
Gravity model TUM-2sp based on the energy balance approach and kinematic CHAMP orbits
We have used one year of CHAMP data for deriving a gravity field model based on he energy balance approach. In order to avoid the use of any a priori gravity field 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 on-board 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 EIGE-2 model.
One year CHAMP data, gravity field, energy balance approach
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Podaci o prilogu
13-18-x.
objavljeno
Podaci o knjizi
Earth Observation with CHAMP - Results from Three Years in Orbit
Reigber, Ch. ; Lühr, H. ; Schwintzer, P. ; Wickert, J.
Heidelberg: Springer
2004.
3-540-22804-7