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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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22. Data Structure<br />

Used by: ORBGEN (”Menu>Orbits/EOP>Create standard orbits”) in the UPDATE mode and<br />

STDPRE (”Menu>Orbits/EOP>Convert standard to precise orbits”) to derive approximated<br />

rms values of the orbit quality for each satellite.<br />

Example: Figure 22.22: In the example file each arc is characterized by 18 orbital<br />

elements (6 Keplerian elements, 9 radiation pressure coefficient parameters,<br />

and 3 pseudo-stochastic parameters at the middle of the arc).<br />

${X}/DOC/EXAMPLE.ELE is also available.<br />

Information concerning the orbit parameterization is given in Chapter 15.<br />

The first column contains the a priori orbital parameters, column 2 and 3 the improved values<br />

and their rms. An asterisk “*” indicates that a parameter was not estimated, ORBSYS 2<br />

in the last column defines the orbital system (ORBSYS 1: B1950.0, ORBSYS 2: J2000.0), and<br />

the string T950101B characterizes, if present, the a priori model for radiation pressure and<br />

the orbit model used (orbit model flag “B”). Pseudo-stochastic orbit parameters are listed<br />

at the end of the file.<br />

22.7.7 Pole File in IGS/IERS Format<br />

Type: ASCII<br />

Directory: Campaign-specific directory ORB.<br />

Extension: IEP<br />

Content: Pole coordinates, UT1-UTC, and nutation offsets together with statistical<br />

information.<br />

Created by: Parameter estimation program <strong>GPS</strong>EST (”Menu>Processing>Parameter estimation”)<br />

or ADDNEQ2 (”Menu>Processing>Normal equation stacking”) or by other IGS analysis<br />

centers.<br />

Used by: Extraction programs POLUPD (”Menu>Orbits/EOP>Handle EOP files>Convert IERS to<br />

<strong>Bernese</strong> format”), POLXTR (”Menu>Orbits/EOP>Handle EOP files>Concatenate IERS pole<br />

files”), submission format of Earth rotation parameters for IERS and IGS.<br />

Example: Figure 22.23 shows Earth rotation estimates in theIEP format stemming from<br />

a 3-days arc. The right-most columns listing the correlations and nutation<br />

estimates are not reproduced. ${X}/DOC/EXAMPLE.IEP is also available.<br />

This file is only used to send pole, UT1-UTC, and nutation information from global Earth<br />

rotation parameter estimations to the IERS Bureau. ERP information is provided in this<br />

format by the IGS. Note that starting on <strong>GPS</strong> week 0966 a new version of the format (version<br />

2) was implemented for all official IGS products in order to get an increased resolution<br />

for the polar motion coordinates, their rates, UT/LOD, and their respective sigmas (see<br />

IGSMAIL #1943). The reading routines in the <strong>Bernese</strong> <strong>GPS</strong> <strong>Software</strong> read the old and the<br />

new format (together with about 13 different pole fileformats).<br />

Files from external sources have the extension ERP. In order to avoid confusion with <strong>Bernese</strong><br />

ERP files rename external files to names with extension IEP.<br />

Page 508 AIUB

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