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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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10.5 Precise Point Positioning<br />

10.5 Precise Point Positioning<br />

The precise point positioning (PPP) is a special case of zero-difference processing. As opposed<br />

to other applications, the satellite clock corrections are not estimated (or differenced<br />

out) but assumed to be known. They are introduced in the processing together with orbit<br />

information and Earth orientation parameters. Parameters left to estimate are station clock<br />

corrections, coordinates, and troposphere parameters.<br />

This modus operandi has several consequences:<br />

• PPP is not a differential technique. The geodetic datum must not be defined by means<br />

of any constraints on reference stations. It is given by the introduced orbit and clock<br />

information and can not be changed.<br />

• Consistency of introduced orbit, EOP, and satellite clock information is of utmost<br />

importance to reach high accuracy. It is mandatory to use the information from the<br />

same source. Mixing of orbits and clocks from different Analysis Centers degrades the<br />

PPP results.<br />

• The models used to estimate the orbits and clock corrections should be the same as<br />

the models implemented in the actual analysis software. This issue poses no problem<br />

when IGS or CODE products are used together with the <strong>Bernese</strong> <strong>GPS</strong> <strong>Software</strong>.<br />

The quality of the introduced information should be as good as possible for PPP as all<br />

errors directly propagate in the results. One kind of inconsistencies may arise when using<br />

orbits from other sources as CODE, e.g., from the IGS. CODE final orbits can be fitted by<br />

program ORBGEN on the sub-cm level whereas this can not be guaranteed for other orbit<br />

products due to slightly different orbit models employed. In such cases the orbit fit may<br />

be improved by setting up not only one but several orbital arcs per day, e.g., two or four<br />

(“ORBGEN 5: Orbital Arc Definition”).<br />

Furthermore, the satellite clock corrections should be used as provided and not be interpolated.<br />

Thus, data processing is limited to the sampling rate of the clock corrections.<br />

I.e., using satellite clock information from IGS clock RINEX files means a data sampling<br />

of 5 min, only. CODE provides high-rate satellite clocks with a sampling of 30 s allowing<br />

higher sampling rates. Use these clocks together with CODE orbits. Section 14.3.1 describes<br />

the necessary steps to extract satellite clock corrections from clock RINEX files.<br />

PPP is a very fast and efficient means to generate good station coordinates. Nevertheless,<br />

it is not possible to reach a coordinate quality as obtained from a network analysis. This<br />

is mainly due to two facts, the impossibility to resolve phase ambiguities and the neglect<br />

of correlations between stations and clock corrections. The latter needs some further explanations:<br />

in a network solution all parameters are estimated to fit all observation data<br />

best possible under consideration of all correlations. This is not the case for a PPP, where<br />

the influence of the stations on the satellite clocks can not be accounted for anymore. As<br />

a consequence, in particular for local and regional networks, small modeling deficiencies<br />

(e.g., concerning troposphere modeling) may be absorbed in the satellite clocks estimated<br />

implicitly in a double-difference solution while this mechanism does not work for PPP. A<br />

network solution is therefore the first choice to obtain highest quality positioning results.<br />

<strong>Bernese</strong> <strong>GPS</strong> <strong>Software</strong> <strong>Version</strong> <strong>5.0</strong> Page 231

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