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Bernese GPS Software Version 5.0 - Bernese GNSS Software

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6. Data Preprocessing<br />

Preprocessing for a<br />

double-difference analysis<br />

code phase<br />

RNXSMT<br />

<strong>GPS</strong>EST<br />

RESRMS<br />

RESCHK<br />

SATMRK<br />

RXOBV3<br />

CODSPP<br />

SNGDIF<br />

if a bad station<br />

detected<br />

MAUPRP<br />

<strong>GPS</strong>EST<br />

RESRMS<br />

RESCHK<br />

SATMRK<br />

RINEX observations<br />

Alternative way for<br />

preprocessing<br />

code phase<br />

SNGDIF<br />

RNXSMT<br />

RXOBV3<br />

CODSPP<br />

MAUPRP<br />

Preprocessing for a<br />

zero-difference analysis<br />

code phase<br />

Double-difference processing Zero-difference processing<br />

if a bad station<br />

detected<br />

RNXSMT<br />

RXOBV3<br />

CODSPP<br />

<strong>GPS</strong>EST<br />

RESRMS<br />

RESCHK<br />

SATMRK<br />

Figure 6.1: Functional flow diagram for the preprocessing part in the <strong>Bernese</strong> <strong>GPS</strong> <strong>Software</strong>.<br />

Gray boxes indicate programs, applied to code and phase in a single run<br />

or in separate runs.<br />

in Section 6.4), and clean the single-difference phase observation files (program MAUPRP,<br />

description in Section 6.5). If you are going to use the Melbourne-Wübbena linear combination<br />

for ambiguity resolution (see Section 8.4) you should use RNXSMT to smooth the<br />

code observations (description in Section 6.2).<br />

For zero-difference solutions, e.g., to estimate receiver or satellite clock corrections, usually<br />

the program RNXSMT is used to screen code and phase observations and to smooth the<br />

code data. The receiver clock synchronization (program CODSPP) is used to prepare a priori<br />

station clock corrections which are stored in the observation files. The disadvantage of<br />

cleaning phase observations using RNXSMT is that the phase data can only be cleaned with<br />

code measurement accuracy. If you have excellent high rate satellite clocks available you<br />

may use program MAUPRP instead of (or in addition to) program RNXSMT to clean the<br />

phase observation files.<br />

The program SNGDIF removes marked observations and keeps the phase ambiguities from<br />

the zero-difference observation files while generating baseline files. If you form baselines<br />

after a zero-difference preprocessing you can, therefore, perform a double difference solution<br />

with the same observations as for a zero-difference analysis. In some cases (e.g., LEO data)<br />

this preprocessing procedure may be preferable also for a double-difference analysis.<br />

Independent from the chosen preprocessing strategy an additional post-fit residual screening<br />

(see Section 6.6) is highly recommended (double difference case) or even mandatory (zerodifference<br />

case). The procedure involves the following steps (that may be iterated):<br />

Page 102 AIUB<br />

iterations

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