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Bernese GPS Software Version 5.0 - Bernese GNSS Software

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5. Preparation of Earth Orientation, <strong>GNSS</strong> Orbit, and Satellite Clock Information<br />

5.5 Preparation of Satellite Clock Corrections<br />

Satellite clock corrections are necessary for the synchronization of the receiver clocks. The<br />

synchronization is performed in the data preprocessing step using program CODSPP, see<br />

Section 6.3. The satellite clock corrections with respect to <strong>GPS</strong> time may be extracted from<br />

three sources, namely from broadcast messages, from IGS precise orbit files, or from IGS<br />

clock RINEX files (see Chapter 4).<br />

You will in general produce a satellite clock file in PRETAB when converting precise orbit<br />

information into tabular format (see Section 5.4.1). You will fit the satellite clock information<br />

from the precise files within intervals of several hours (12 hours is recommended in panel<br />

“PRETAB 3: Options for Clocks”) by low degree polynomials (the recommended degree is q = 2)<br />

and thus create a satellite clock file which may be used to compute satellite clock corrections<br />

for each observation epoch. This way of handling the clocks in the precise files is the normal<br />

case.<br />

You also have the possibility to extract the unaltered satellite clock corrections from the<br />

precise orbit files (usually given at 15 minute intervals) by asking for a polynomial degree<br />

and an interval length of “zero”. This way, for observations made exactly at the time of<br />

the tabular epochs in the precise orbit file, you may access the very precise IGS satellite<br />

clock information (e.g., in case that Selective Availability SA is enabled). Program CODSPP<br />

may take profit out of this special case for handling precise clock information, if you are<br />

asking for the correct option in this program. The option may also be used to perform a<br />

precise point positioning with program <strong>GPS</strong>EST (see Section 10.5). In general this option is,<br />

however, rather harmful due to the significant data reduction (one epoch every 15 minutes<br />

instead of, e.g., every 30 seconds). Therefore, use this special option with care!<br />

Program SATCLK (”Menu>Orbits/EOP>Broadcast orbits>Extract satellite clocks”) extracts satellite clock<br />

information from broadcast files generated by program RXNBV3 and writes it into a satellite<br />

clock file in the <strong>Bernese</strong> format (see Section 22.7.10). You may also generate a satellite<br />

clock file for use in CODSPP or <strong>GPS</strong>EST from Clock RINEX files using program CCRNXC<br />

(see Section 14.3). Clock RINEX files available from the IGS contain clock values for every<br />

5 minutes instead of every 15 minutes as for the IGS precise orbit files. From CODE, precise<br />

clock information at a rate of 30 seconds is available since March 2004 (see Section 4.12.1).<br />

5.6 Concatenation of Orbit Information and Orbit Comparison<br />

5.6.1 Concatenation of Precise Orbit Information<br />

Let us briefly discuss the program CCPREORB (”Menu>Orbits/EOP>Cut/concatenate precise orbit<br />

files”). This program allows to merge two orbit files in SP3 format: all satellites found in<br />

the first file are written into the new orbit file. If the second file contains further satellites<br />

(e.g., GLONASS satellites), they are added to the new orbit file. In this way it is possible to<br />

use, e.g., the <strong>GPS</strong> orbit information from one SP3 file and the GLONASS orbit information<br />

from another SP3 file or to merge precise <strong>GPS</strong> orbits in the SP3 format with GLONASS<br />

broadcast orbits in the SP3 format.<br />

Several options are available to control the merging of two precise files. Priority of individual<br />

satellites from the two files may be adapted based on the prediction flags in SP3c<br />

Page 98 AIUB

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