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Bernese GPS Software Version 5.0 - Bernese GNSS Software

Bernese GPS Software Version 5.0 - Bernese GNSS Software

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5.2 Preparation of Earth Orientation Parameters<br />

5.2.1 General Dataset Names<br />

5.2 Preparation of Earth Orientation Parameters<br />

A set of EOP is required to perform the transformation from the Earth-fixed to the celestial<br />

system or vice versa. As described in the following sections the programs PRETAB and<br />

BRDTAB compute a table of satellite positions in the inertial frame from the available orbit<br />

information (usually precise orbits in an Earth-fixed frame, e.g., IGS00). Therefore, the<br />

EOP file corresponding to the orbits used has to be specified in the appropriate input field<br />

(option “Pole file”) of all program input panels.<br />

If IGS precise orbits are used the corresponding EOP files are available at the global<br />

data centers (see Section 4.12.2). The Earth rotation parameters associated with the IGS<br />

ephemeris files are computed using a weighted average of all available center-specific ERP<br />

files 2 . The ERP files stemming from CODE may be downloaded via anonymous ftp, too<br />

(see Section 4.12.1). Be aware that in contrast to the naming rules of the <strong>Bernese</strong> environment<br />

all these files contain pole information in IGS format although their extension is ERP<br />

(see also Section 22.7.7)! The pole files in IGS or IERS format have to be transformed into<br />

the <strong>Bernese</strong> pole format. This task is performed by program POLUPD with options to be<br />

discussed in detail later.<br />

If other than IGS precise orbits are used (and no specific ERP files are available), it is<br />

recommended to use the IERS C04 pole. C04 is a continuous, slightly low pass filtered<br />

series at daily intervals and can be interpolated linearly. Oscillations in UT1 and in the<br />

length of day due to zonal tides for periods under 35 days, as well as the 14-day terms in dψ<br />

and dε are present in full size in the series [Dick and Richter, 2001]. In Section 4.5 sources<br />

for downloading EOP files are provided.<br />

Nutation model and subdaily pole model coefficients are read from files located in the<br />

directory ${X}/GEN. To be consistent with the IERS Conventions 2003 [McCarthy and Petit,<br />

2004] useIAU2000 as the nutation model approved by the International Astronomical Union<br />

(IAU) and IERS2000 for the model describing the subdaily tidal variations of the pole and<br />

the rotation of the Earth. Specify these values in all program input panels for the options<br />

“Nutation model” and “Subdaily pole model” respectively.<br />

The two models must be equal in the programs generating a standard orbit (PRETAB<br />

and ORBGEN) and in the programs using the standard orbit information. The names of<br />

the models are written into the headers of the ERP files, the tabular orbit files, and the<br />

standard orbit files. All programs reading standard orbit and Earth orientation information<br />

check the consistency of the nutation and subdaily models.<br />

5.2.2 Update of Pole Information<br />

In order to obtain the most accurate EOP information covering the span of your <strong>GPS</strong> campaign<br />

you are forced to update the file containing the Earth rotation parameter information,<br />

whenever more consistent (with the precise orbit data) and/or more recent values become<br />

2 The term Earth rotation parameters (ERP) is used for a 3-parameter subset of the EOP which comprises<br />

polar motion (xp, yp) and UT1.<br />

<strong>Bernese</strong> <strong>GPS</strong> <strong>Software</strong> <strong>Version</strong> <strong>5.0</strong> Page 85

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