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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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20. Processing Examples<br />

• Save the results in a kinematic coordinate file (option “Kinematic coordinates” in<br />

panel “CODSPP 1.3: Output Files” )<br />

PID 302 PPPEDT P:<br />

• Introduce the kinematic solution from the previous step using option “Kinematic<br />

coordinates” in panel “<strong>GPS</strong>EST 1.2: Input Files 2”<br />

• Save the results in a “Kinematic coordinates” file<br />

• Set the “Type of computed residuals” in panel “<strong>GPS</strong>EST 3.1: General Options 1” to<br />

NORM APRIORI<br />

• Enable the kinematic positioning with checkbox “Kinematic coordinates” in Section<br />

“EPOCH PARAMETERS” of panel “<strong>GPS</strong>EST 5.1: Setup of Parameters and Pre-<br />

Elimination 1” and set the “Pre-Elimination” to EVERY EPOCH<br />

• Select the kinematic station in panel “<strong>GPS</strong>EST 6.5: Kinematic Coordinates”<br />

• Constrain the solution to the a priori positions from the kinematic coordinates file<br />

according to the already achieved accuracy (depends primarily on data quality<br />

- from our experience the data quality decreases with increasing rover speed).<br />

This value may be adapted during the iteration in this script (e.g., by using the<br />

$bpe->putKey(); mechanism)<br />

PID 303 <strong>GPS</strong>XTR: A filename for the “Kinematic summary” in panel “<strong>GPS</strong>XTR 2: Output Files”<br />

may be added<br />

PID 311 ...PID 522: These scripts are not necessary in kinematic mode and may be skipped<br />

PID 901 PPP SUM ...PID 903 BPE CLN: Adapt these scripts to your needs.<br />

The kinematic solutions from several stations may be merged by simply concatenating the<br />

positions from the single kinematic coordinate files. A header section (e.g., from the first<br />

file) must be included.<br />

The clock RINEX files provided by the IGS contain satellite clock information with a sampling<br />

of 300 seconds, only. Consequently, the resulting kinematic coordinate file from the<br />

PPP.PCF can only contain a coordinate set every 5 minutes. The following scripts must be<br />

modified to densify the solution up to 30 seconds:<br />

PID 001 PPP COP: Copy the precise orbit, Earth orientation information, and clock RINEX<br />

file from an IGS analysis center providing high rate satellite clock values (e.g., CODE)<br />

instead of using the IGS combined products. It is recommended to modify the value<br />

of the PCF-variable V B accordingly.<br />

PID 212 RNXSMT P:<br />

• Adapt option “Sampling interval for RINEX data” to generate a kinematic solution<br />

with a sampling higher than 30 seconds.<br />

• The parameter MAXREC=10000 in the main program ${FG}/RNXSMT.f limits<br />

the number of epochs that can be analyzed in one program run. You may either<br />

increase this number and compile the program or limit the processing to a shorter<br />

observation interval with option “Use observation window”. Alternatively you may<br />

cut the RINEX observation file using program CCRINEXO.<br />

Page 460 AIUB

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