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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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6.6 Screening of Post-Fit Residuals<br />

“RMS threshold level for a bad solution” only the station with the biggest total RMS error will<br />

be marked as “bad”. The residual screening has to be repeated after removing the station.<br />

The “bad” stations may be listed in a file allowing to delete the corresponding observation<br />

files. If you have detected and removed bad stations you should recompute the residual files<br />

(program <strong>GPS</strong>EST) and generate a new edit information file (program RESRMS) before<br />

marking the observations with the program SATMRK. If you are processing a network<br />

of baselines you have to rebuild the entire network (program SNGDIF) after deleting the<br />

observation files of the bad station. The new baselines have, of course, to be preprocessed<br />

again (program MAUPRP) before the residuals may be recomputed.<br />

Bad Satellite Detection<br />

You can download the file indicating satellite problems from the anonymous ftp account<br />

of AIUB (http://www.aiub.unibe.ch/download/BSWUSER50/GEN/SAT_yyyy.CRX, where<br />

yyyy is the four digit year). This file is updated every time when a new satellite problem<br />

appears (satellite maneuvers, bad data,...) in the routine processing for the IGS at CODE.<br />

Observations of misbehaving satellites are rejected by the program RXOBV3 in your processing<br />

if you use this file. It is, therefore, not necessary for you to repeat the detection<br />

procedure for misbehaving satellites.<br />

Nevertheless, the description of the algorithm is given here:<br />

(1) The CODSPP extraction (program CODXTR, see Section 6.3.4) and the arc split summary<br />

(program DEFXTR, see Section 5.4.2) may contain hints for a repositioning of a<br />

satellite. If at least one of these files shows an indication of a repositioning a maneuver<br />

is postulated for the corresponding satellites.<br />

(2) Satellites for which a maneuver is postulated but which show no abnormal behavior<br />

with respect to the mean RMS in the bottom line of the RESRMS-residual summary<br />

(option “Maximum ratio of satellite RMS to overall RMS” in the section “OPTIONS FOR BAD<br />

SATELLITE DETECTION”) are dropped from the maneuver list.<br />

(3) Satellites without any observations in the RESRMS summary table are added to the<br />

list of bad satellites. This can happen, e.g., when all observations of the satellite in all<br />

contributing observation files are marked.<br />

(4) The number of observations from all stations or baselines to each satellite are compared<br />

in the first and in the second table of the RESRMS residual summary (before and<br />

after the screening of post-fit residuals). A satellite for which a big amount of data<br />

is removed is assumed to be “bad” (option “Maximal percentage of deleted data”). This<br />

part is skipped if a maneuver hypothesis holds for at least one satellite because a<br />

maneuvered satellite may affect the residuals of other satellites.<br />

Note that for GLONASS a four times higher value is applied than for <strong>GPS</strong> because<br />

of the lower total number of observations (see subroutine RCSATCHK.f90).<br />

(5) The ratio of the overall RMS for one satellite w.r.t. the mean total RMS for all satellites<br />

is computed. If this ratio exceeds the specified maximum ratio (option “Maximum ratio<br />

of satellite RMS to overall RMS”), the satellite is assumed to be “bad”. Two different<br />

threshold ratios are used depending on whether satellites with a maneuver hypothesis<br />

were identified or not.<br />

<strong>Bernese</strong> <strong>GPS</strong> <strong>Software</strong> <strong>Version</strong> <strong>5.0</strong> Page 135

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