THE KAISERSLAUTERN MULTISCALE GEOPOTENTIAL MODEL SWITCH-03 FROM ORBIT PERTURBATIONS OF THE SATELLITE CHAMP AND ITS COMPARISON TO THE MODELS EGM96, UCPH2002_02_0.5, EIGEN-1S AND EIGEN-2

Show simple item record

dc.contributor.author Fengler M.J.
dc.contributor.author Freeden W.
dc.contributor.author Michel V.
dc.date.accessioned 2022-09-22T08:19:12Z
dc.date.available 2022-09-22T08:19:12Z
dc.date.issued 2004
dc.identifier https://elibrary.ru/item.asp?id=6524300
dc.identifier.citation Geophysical Journal International, 2004, 157, 2, 499-514
dc.identifier.issn 0956-540X
dc.identifier.uri https://repository.geologyscience.ru/handle/123456789/38688
dc.description.abstract Observed orbit perturbations of the near-Earth orbiting satellite CHAMP are analysed to recover the long-wavelength features of the Earth's gravitational potential. More precisely, by tracking the low-flying satellite CHAMP using the high-flying satellites of the Global Positioning System (GPS) the kinematic orbit of CHAMP is obtainable from GPS tracking observations, i.e. the ephemeris in Cartesian coordinates in an Earth-fixed coordinate frame (WGS84) becomes available.
dc.description.abstract In this study we are concerned with two tasks: first we present new methods for pre-processing, modelling and analysing the emerging tracking data. Then, in a first step we demonstrate the strength of our approach by applying it to simulated CHAMP orbit data. In a second step we present results obtained by operating on a data set derived from real CHAMP data.
dc.description.abstract The modelling is mainly based on a connection between non-bandlimited spherical splines and least-square adjustment techniques to take into account the non-sphericity of the trajectory. Furthermore, harmonic regularization wavelets for solving the underlying satellite-to-satellite tracking (SST) problem are used within the framework of multiscale recovery of the Earth's gravitational potential leading to SWITCH-03 (Spline and Wavelet Inverse Tikhonov regularized CHamp data). Further we show how regularization parameters can be adapted adequately to a specific region thereby improving a globally resolved model. Finally we compare the developed model with the EGM96 model, model UCPH2002_02_0.5 from the University of Copenhagen and the GFZ models EIGEN-1s and EIGEN-2.
dc.subject CHAMP POST-PROCESSED SCIENCE ORBIT DATA
dc.subject REGIONAL GRAVITATIONAL FIELD RECOVERY
dc.subject SPHERICAL SPLINES
dc.subject TIKHONOV WAVELET REGULARIZATION
dc.title THE KAISERSLAUTERN MULTISCALE GEOPOTENTIAL MODEL SWITCH-03 FROM ORBIT PERTURBATIONS OF THE SATELLITE CHAMP AND ITS COMPARISON TO THE MODELS EGM96, UCPH2002_02_0.5, EIGEN-1S AND EIGEN-2
dc.type Статья


Files in this item

This item appears in the following Collection(s)

  • ELibrary
    Метаданные публикаций с сайта https://www.elibrary.ru

Show simple item record