Titlebook: Earth Observation with CHAMP; Results from Three Y Christoph Reigber,Hermann Lühr,Jens Wickert Book 2005 Springer-Verlag Berlin Heidelberg

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A New Method to Detect and Estimate CHAMP Clock Bias Change Cycle Slipference between two neighboring epoch phase observations includes real CHAMP-GPS distance change, CHAMP clock receiver bias change, cycle slip and other corrections. Real CHAMP-GPS distance change can be obtained at a relatively high precision from a dynamic orbit. As a result, the CHAMP GPS receive

GUMP

Comparison of Different Stochastic Orbit Modeling Techniquesthe performance of different pseudo-stochastic orbit parametrizations (instantaneous velocity changes and piecewise constant accelerations) and probe the range between dynamic and heavily reduced dynamic orbits. Internal indicators like formal accuracies of orbit positions, comparisons with orbits c

Aura231

一窩小鳥

organism

CHAMP Gravity Field Solutions and Geophysical Constraint Studiestion. 1.5 years of CHAMP data from May 2001 through February 2003 are used for monthly gravity solutions as well as a mean solution based on 6 months of data, employing the energy conservation principle and an efficient conjugate gradient inversion technique. The mean CHAMP gravity field model, OSU0

我悲傷

Application of Eigenvalue Decomposition in the Parallel Computation of a CHAMP 100x100 Gravity Fieldas applied to the CHAMP normal matrix . {xc[2]} to perform an Eigenvalue Decomposition (EVD) analysis. The EIGEN1S solution is based on the Tikhonov regularization method of approximating the ill-conditioned system of equations in a subspace of lower rank. In the EVD solution, poorly determined line

廣大

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https://doi.org/10.1007/b138105Atmosphere sounding; CHAMP satellite mission; Earth System; Earth gravity field; Geomagnetism; Gravity; Io