By Stuart Turner
1987 Springer. Lecture Notes in Earth Sciences 12. Lg.8vo., 393pp., wraps. the rest lessen on reduce fore-edge, VG. moderate hide put on; no proprietor marks.
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Extra info for Applied geodesy: global positioning system : networks, particle accelerators, mathematical geodesy
4. COMPARISONOF SATELLITE AND TERRESTRIAL OBSERVATION RESULTS The f i r s t possibility to achieve a s s e r t i o n s on accuracies of s a t e l l i t e observations in comparison to t e r r e s t r i a l aided network network observations is the simple comparison of s p e c i f i c r e s u l t s obtained from the i n d i v i d u a l adjustments of the t e r r e s t r i a l and s a t e l l i t e observations, respectively. The coordinates of those adjustments can be compared with each o t h e r a f t e r a 7-parameter s i m i l a r i t y t r a n s f o r m a t i o n which s p l i t s o f f network e x t e r n a l e f f e c t s caused f o r i n - stance by a d i f f e r e n t T_sdX = T_sdX T = Tx - geodetic datum.
6) (1967). S. K. Jordan, Self-consistent statistical models for the gravity anomaly, vertical deflections, and undulation of the geold, J. Geophys. , 77 (20), 3660-3670, (1972). GPS ORBIT DETERMINATION USING THE DOUBLE DIFFERENCE PHASE OBSERVABLE G. Beutler Astronomical Institute, After University of Berne, Switzerland discussing vehicles orbital precision a review of simple but orbital biases elimination-) requirements correct procedures orbit for GPS space determination is given. The (and 1984 Alaska GPS experiment and the 1985 High Precision Baseline Test (HPBL-Test) are presented techniques as typical are mandatory.
F r o m A p r i l 2 t o A p r i l 5. - i = arc length in days. - k = number of r a d i a t i o n p r e s s u r e p a r a m e t e r s estimated. 46 (c) Coordinates An independent check of the quality of the estimated orbits the coordinates (as obtained in the various solutions) is possible by comparing for the stations Hat Creek, Owens Valley, Mammoth Lake, Austin and Dahlgren, because these reciever locations were estimated without constraints in all program runs. If our orbits would be good to - let us say - i ppm, we would expect differences of up to 4 meters in the different solutions, since we have baselines of up to 4000 km.