Detailed Description
Implement the formula for the displacement of a point fixed to the solid Earth due to the solid Earth tides resulting from the influence of the Sun and Moon. Reference IERS Conventions (1996) found in IERS Technical Note 21 (IERS). NB. Currently only the largest terms are implemented, yielding a result accurate to the millimeter level. Specifically, IERS pg 61 eq 8 and IERS pg 65 eq 17, (this includes removing the permanent component). Class SolarSystem may be used to get Solar and Lunar ephemeris information, including position and mass ratios.
Definition in file SolidEarthTides.cpp.
Include dependency graph for SolidEarthTides.cpp:
Go to the source code of this file.
Namespaces | |
| gnsstk | |
| For Sinex::InputHistory. | |
Functions | |
| Triple | gnsstk::computePolarTides (const Position &site, const EphTime &ttag, double xp, double yp, const IERSConvention &iers) |
| Triple | gnsstk::computeSolidEarthTides (const Position &site, const EphTime &ttag, const Position &Sun, const Position &Moon, double EMRAT, double SERAT, const IERSConvention &iers) |