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Bernese GPS Software Version 5.0 - Bernese GNSS Software

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10. Station Coordinates and Velocities<br />

10.1.1 Tectonic Plate Motion<br />

Station coordinates are changing in time due to the steady movement of tectonic plates.<br />

Figure 10.8 shows the present day major tectonic plates. This movement must be taken<br />

into account in <strong>GNSS</strong> analyses. Station coordinates (especially of reference sites) should<br />

therefore always be propagated from the reference epoch to the observation epoch based on<br />

corresponding station velocities. This ensures consistency with the IGS satellite orbits and<br />

prevents network deformations induced by moving plates.<br />

If unavailable from other sources (e.g., the IERS), reasonable station velocities may be<br />

derived from a model. One such model is the NNR-NUVEL-1A [DeMets et al., 1994], complying<br />

with the IERS Conventions [McCarthy and Petit, 2004].<br />

The <strong>Bernese</strong> <strong>GPS</strong> <strong>Software</strong> offers corresponding programs to compute model velocities<br />

and to propagate coordinates, namely NUVELO and COOVEL. Both are described in Section<br />

10.6.<br />

10.1.2 Solid Earth Tides, Pole Tides, and Permanent Tides<br />

Effects of solid Earth tides have to be taken into account because they are at least one order<br />

of magnitude larger than the accuracies currently achieved for <strong>GNSS</strong>-derived coordinates.<br />

The <strong>Bernese</strong> <strong>GPS</strong> <strong>Software</strong> <strong>Version</strong> <strong>5.0</strong> adheres to the IERS Conventions 2003 [McCarthy<br />

and Petit, 2004] to model the solid Earth tides. The “step 1” and “step 2” corrections are<br />

implemented.<br />

The effects of the solid Earth pole tide are modeled according to the IERS Conventions<br />

2003, too, adopting mean values of 0.033” and 0.331” for x and y pole, respectively.<br />

In accordance with common geodetic practice, estimated coordinates are freed from all tidal<br />

corrections including the permanent tide. To obtain coordinate values that correspond to<br />

the mean over long periods the permanent tide must be added to the estimated coordinates.<br />

Handling of the permanent tide can be changed in the subroutine ${LG}/TIDE2000.f. A<br />

description of the “permanent problem of the permanent tide” is given, e.g., in [Ekman,<br />

1995].<br />

Note, that positions for all stations are corrected for tides. The only exception are stations<br />

that are flagged with SPACEBORNE in Section TYPE 005: HANDLING STATION TYPES.<br />

Typically these are Low Earth orbiters equipped with <strong>GNSS</strong> receivers.<br />

10.1.3 Ocean Tidal Loading Effects<br />

Another important site displacement effect is the crustal deformation caused by the changing<br />

mass distribution due to ocean tides (ocean tidal loading). A file containing station-specific<br />

coefficients for the magnitude of the ocean loading effect (amplitude and phase shift for the<br />

eleven most important constituents) may be selected where necessary (programs <strong>GPS</strong>EST,<br />

<strong>GPS</strong>SIM, and CLKEST). Although this file is not mandatory its use is strongly recommended<br />

because otherwise vertical and horizontal corrections will not be applied. Nodal modulations<br />

are not accounted for in <strong>Version</strong> <strong>5.0</strong> .<br />

Page 212 AIUB

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