Figures and Statistics for Precise Point Positioning (PPP)
PPP Strategy:
A Precise Point Positioning (PPP) is performed using the ERPs, SP3 orbits,
and satellite clocks from the IGS Final/Rapid combination as well as from
the individual contributing Analysis Centers. Clocks and RINEX observations
are decimated to 5-min intervals.
The PPP is done on a daily basis for each of the available stations defining
the IGS Reference Frame ( 274 stations for IGS14). For each set of AC orbits,
ERPs, and satellite clocks, a PPP solution is done in three steps. Step 1 involves
fitting the satellite positions from the SP3 orbit files to the extended
CODE (6+9) orbit model using the associated ERPs in the ECF->Inertial transformation.
Step 2 involves preprocessing of the clocks and RINEX observations to detect and eliminate
clock jumps and cycle slips. Step 3 is the data reduction with iterative
post-fit cleaning; outliers in the phase residuals are taken to be greater
than 25 mm and outliers in the code residuals are taken to be greater than
2.5 m. A-priori modeling of the tropospheric delay is done using the Global Mapping
Function (GMF) and Global Pressure and Temperature (GPT) model. Prior to 11 April 2013,
The Niell Mapping Function (NMF) and standard meteorological data were used.
The products from each AC are processed seperately; this way the cleaning
for one AC has no effect on the results for the other ACs.
Helmert transformations are performed between the global network compiled
from the PPP results and both the IGS Reference Frame and the IGS combined
SINEX solution. The Helmert transformation parameters and station residual
statistics are given over the past 7 days. North, east, up residuals (after
the Helmert transformation) for each of the stations are presented including
its mean and standard deviation over the past 7 days.
The PPP results give a measure of the internal consistency for each set of
AC clocks, orbits, and ERPs. Over time, the PPP analysis also reveals information
about the stability of station coordinates and the realization of a given
reference frame.
Starting on 19-Aug-2012 (GPS Week 1702; mjd=56158), the IGS Finals products
switched from being based on weekly SINEX integrations to being based on
daily ones. Associated with this switch is a change to comparing with daily
SINEX files, instead of a weekly one. The switch began impacting the Rapid
PPP starting on 05-Sep-2012 (GPS Week 1704, day 3; mjd=56175).
Software:
Bernese GNSS Software v. 5.2, Developed by the Astronomical Institute of the
University of Bern, Switzerland
(Bernese v. 5.0 was replaced on 11 April 2013)
PPP using Rapid Orbits and Clocks
PPP Rapid Transformations |
recent weeks |
GIF |
PS |
history |
GIF |
PS |
PPP Rapid Rotations and Scales |
recent weeks |
GIF |
PS |
history |
GIF |
PS |
PPP Rapid Station RMS (IGS RF) |
recent weeks |
GIF |
PS |
history |
GIF |
PS |
PPP Rapid Station RMS (SINEX irf) |
recent weeks |
GIF |
PS |
history |
GIF |
PS |
PPP using Final Orbits and Clocks
All AC and IGR/IGS results in one plot for each component.
PPP Final Station RMS (IGS RF) |
recent weeks |
GIF |
PS |
history |
GIF |
PS |
PPP Final Station RMS (SINEX irf) |
recent weeks |
GIF |
PS |
history |
GIF |
PS |
Figures for the individual ACs (and IGR/IGS).
Transformation parameters from the SINEX combinations are
included for comparison.
Translations and Scale from:
Rotations from:
12 April 2013, originator IGS ACC