Recent advances in remote sensing and in computer hardware made it feasible to produce the numerical weather models of the atmosphere with high temporary and spatial resolution. We expect that the accuracy and resolution of these models will improve in the future. The output of these models represents the 4D field of the atmospheric parameters. Therefore, the path delay can be computed directly from this field by numerical integration without using inaccurate regression models.
The motivation of this project is to derive a rigorous and computationally efficient algorithm for computing the slant path delay through the 4D, inhomogeneous, elliptical atmosphere designed for processing space geodesy observations on a global, dense network; to validate this model using space geodesy observation; and to develop a procedure for automatic update of the slant path delays in order to use it for routine data analysis of radioastronomy and space geodesy observations. The algorithm is intended to be used in a service of the slant path delay computation for processing VLBI, GPS, and DORIS observations.
The same slant path delays in binary format are available as well.
Web page was prepared by Leonid Petrov
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Last update: 2010.02.12_22:36:10