Upload
others
View
3
Download
0
Embed Size (px)
Citation preview
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Dependency of Geodynamic
Parameters on the GNSS
Constellation
S. Scaramuzza,R. Dach, G. Beutler, D. Arnold, A. Jaggi
Astronomical Institute, University of Bern, Switzerland
Session: Plenary #06 — Reference FrameIGS Workshop, 08.–12. February 2016, Sydney, Australia
Slide 1 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Overview
Introduction and Motivation
Geocenter Parameters
Earth Rotation Parameters
Summary and Conclusion
Slide 2 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Levels of Multi-GNSS Analysis
satCLK
ORB
ERP
GCC
TRP
CRD
recCLK
GPS GLONASS
Slide 3 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Levels of Multi-GNSS Analysis
satCLK
ORB
ERP
GCC
TRP
CRD
recCLK+ISB
GPS GLONASS
Slide 3 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Levels of Multi-GNSS Analysis
satCLK
ORB
ERP
GCC
TRP
CRD
recCLK+ISB
GPS GLONASS
Slide 3 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Levels of Multi-GNSS Analysis
satCLK
ORB
ERP
GCC
TRP
CRD
recCLK+ISB
GPS GLONASS
Slide 3 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Levels of Multi-GNSS Analysis
satCLK
ORB
ERP
GCC
TRP
CRD
recCLK+ISB
GPS GLONASS
Slide 3 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Levels of Multi-GNSS Analysis
satCLK
ORB
ERP
GCC
TRP
CRD
recCLK+ISB
GPS GLONASS
Slide 3 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Update in the CODE Processing
• The daily NEQs may be setup with ERP and GCC parametersper satellite.
Slide 4 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Update in the CODE Processing
• The daily NEQs may be setup with ERP and GCC parametersper satellite.
• Since GPS week 1842 (May 2015) CODE constructs NEQ-fileswith
• plane-wise ERP (6 for GPS and 3 for GLONASS), and• satellite-wise GCC parameters.
Slide 4 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Update in the CODE Processing
• The daily NEQs may be setup with ERP and GCC parametersper satellite.
• Since GPS week 1842 (May 2015) CODE constructs NEQ-fileswith
• plane-wise ERP (6 for GPS and 3 for GLONASS), and• satellite-wise GCC parameters.
• By parameter stacking• the IGS solution with one set of ERP and GCC parameters,
may be constructed.
Slide 4 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Update in the CODE Processing
• The daily NEQs may be setup with ERP and GCC parametersper satellite.
• Since GPS week 1842 (May 2015) CODE constructs NEQ-fileswith
• plane-wise ERP (6 for GPS and 3 for GLONASS), and• satellite-wise GCC parameters.
• By parameter stacking• the IGS solution with one set of ERP and GCC parameters,• system-specific ERP and GCC solutions,
may be constructed.
Slide 4 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Update in the CODE Processing
• The daily NEQs may be setup with ERP and GCC parametersper satellite.
• Since GPS week 1842 (May 2015) CODE constructs NEQ-fileswith
• plane-wise ERP (6 for GPS and 3 for GLONASS), and• satellite-wise GCC parameters.
• By parameter stacking• the IGS solution with one set of ERP and GCC parameters,• system-specific ERP and GCC solutions,• . . .
may be constructed.
Slide 4 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Principle of Solution Generation
GPS GLONASS
Slide 5 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Principle of Solution Generation
ERP(GLONASS)ERP(GPS)
GPS GLONASS
Slide 5 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Principle of Solution Generation
ERP(GLONASS)ERP(GPS)
ERP(Combined)
GPS GLONASS
Slide 5 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Principle of Solution Generation
ERP(GLONASS)ERP(GPS)
ERP(Combined)
GPS GLONASS
Slide 5 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Principle of Solution Generation
GCC(GLONASS)GCC(GPS)
GCC(Combined)
GPS GLONASS
Slide 5 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Geocenter Parameters
Introduction and Motivation
Geocenter Parameters
Earth Rotation Parameters
Summary and Conclusion
Slide 6 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Geocenter Parameters
Time series for GCC estimates: Z component from GLONASS
Time2012 2013 2014 2015
GZ [c
m]
-20
-10
0
10
20
-90
-45
0
45
90
Slide 7 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Geocenter Parameters
Time series for GCC estimates: Z component from GPS
Time2012 2013 2014 2015
GZ [c
m]
-20
-10
0
10
20
-90
-45
0
45
90
Slide 7 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Geocenter Parameters
Time series for GCC estimates: Z component from GPS+GLO
Time2012 2013 2014 2015
GZ [c
m]
-20
-10
0
10
20
-90
-45
0
45
90
Slide 7 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Geocenter Parameters
Formal errors for GCC estimates: Z component
Time2012 2013 2014 2015
Err
or G
Z [m
m]
0
2
4
6
8
10
12GPSGLONASS
Slide 8 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Geocenter Parameters
Formal errors for GCC estimates: Z component
Time2012 2013 2014 2015
Err
or G
Z [m
m]
0
2
4
6
8
10
12CombinedGPSGLONASS
Slide 8 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Geocenter Parameters
Formal errors for GCC estimates: Z component
Time2012 2013 2014 2015
Err
or G
Z [m
m]
0
2
4
6
8
10
12CombinedGPSGLONASS
In full agreement to Meindl et al., 2013: DOI 10.1016/j.asr.2012.10.026.
Slide 8 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Earth Rotation Parameters
Introduction and Motivation
Geocenter Parameters
Earth Rotation Parameters
Summary and Conclusion
Slide 9 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Earth Rotation Parameters
Amplitude spectra from ERP estimates: X component
Period [days] 10 100
Pol
e X
[µas
]
0
5
10
15
20
25
30CombinedGPSGLONASS
Differences w.r.t. IERS C04 series (related to ITRF2008) have been analysed.
Slide 10 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Earth Rotation Parameters
Amplitude spectra from ERP estimates: Y component
Period [days] 10 100
Pol
e Y
[µas
]
0
5
10
15
20
25
30CombinedGPSGLONASS
Differences w.r.t. IERS C04 series (related to ITRF2008) have been analysed.
Slide 10 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Earth Rotation Parameters
Formal errors for ERP estimates: X component
Time2012 2013 2014 2015
Err
or P
ole
X [µ
as]
0
5
10
15
20
25
30
35
CombinedGPSGLONASS
Slide 11 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Earth Rotation Parameters
Formal errors for ERP estimates: Y component
Time2012 2013 2014 2015
Err
or P
ole
Y [µ
as]
0
5
10
15
20
25
30
35
CombinedGPSGLONASS
Slide 11 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Principle of Solution Generation
ERP(GLONASS)ERP(GPS)
ERP(Combined)
GPS GLONASS
Slide 12 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Principle of Solution Generation
ERP(GLONASS)ERP(GPS)
ERP(Combined)
ERP(GLONASS)
ERP(GPSo) ERP(GPSe)
GPS GLONASS
Slide 12 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Formal errors for ERP estimates: X component
Time2012 2013 2014 2015
Err
or P
ole
X [µ
as]
0
5
10
15
20
25
30
35
GPSGPSoGPSe
Slide 13 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Formal errors for ERP estimates: Y component
Time2012 2013 2014 2015
Err
or P
ole
Y [µ
as]
0
5
10
15
20
25
30
35
GPSGPSoGPSe
Slide 13 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Amplitude spectra from ERP estimates: X component
Period [days] 10 100
Pol
e X
[µas
]
0
5
10
15
20
25
30GPSGPSoGPSe
Differences w.r.t. IERS C04 series (related to ITRF2008) have been analysed.
Slide 14 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Amplitude spectra from ERP estimates: Y component
Period [days] 10 100
Pol
e Y
[µas
]
0
5
10
15
20
25
30GPSGPSoGPSe
Differences w.r.t. IERS C04 series (related to ITRF2008) have been analysed.
Slide 14 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Formal errors for ERP estimates: Y component
Time2012 2013 2014 2015
Err
or P
ole
Y [µ
as]
0
5
10
15
20
25
30
35
0
45
90
Slide 15 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Formal errors for ERP estimates: Y component
Time2012 2013 2014 2015
Err
or P
ole
Y [µ
as]
0
5
10
15
20
25
30
35
0
45
90
Slide 15 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Formal errors for ERP estimates: Y component
Time2012 2013 2014 2015
Err
or P
ole
Y [µ
as]
0
5
10
15
20
25
30
35
0
45
90
Slide 15 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Formal errors for ERP estimates: Y component
0 5 10 15 20 25 30 35 40 45
Err
or P
ole
Y [µ
as]
10
15
20
25GPSe
Slide 16 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Formal errors for ERP estimates: Y component
0 5 10 15 20 25 30 35 40 45
Err
or P
ole
Y [µ
as]
10
15
20
25GPSe
0 5 10 15 20 25 30 35 40 45
Err
or P
ole
Y [µ
as]
10
15
20
25GPSo
Slide 16 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Formal errors for ERP estimates: Y component
0 5 10 15 20 25 30 35 40 45
Err
or P
ole
Y [µ
as]
10
15
20
25GPSe
0 5 10 15 20 25 30 35 40 45
Err
or P
ole
Y [µ
as]
10
15
20
25GPSo
0 5 10 15 20 25 30 35 40 45
Err
or P
ole
Y [µ
as]
15
20
25
30
35GLO
Slide 16 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Formal errors for ERP estimates: X component
0 5 10 15 20 25 30 35 40 45
Err
or P
ole
X [µ
as]
10
15
20
25GPSo
0 5 10 15 20 25 30 35 40 45
Err
or P
ole
X [µ
as]
10
15
20
25GPSe
Slide 17 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Formal errors for ERP estimates: X component
0 5 10 15 20 25 30 35 40 45
Err
or P
ole
X [µ
as]
10
15
20
25GPSo
0 5 10 15 20 25 30 35 40 45
Err
or P
ole
X [µ
as]
10
15
20
25GPSe
0 5 10 15 20 25 30 35 40 45
Err
or P
ole
X [µ
as]
15
20
25
30
35GLO
Slide 17 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Amplitude spectra from ERP estimates: Y component
Period [days] 10 100
Y [µ
asec
]
0
5
10
15
20
25
30
35
40
45
50 (26-Dec-2011 to 25-Dec-2014)
GPSGPSoGPSe
Differences w.r.t. IERS C04 series (related to ITRF2008) have been analysed.
Slide 18 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Amplitude spectra from ERP estimates: Y component
Period [days] 10 100
Y [µ
asec
]
0
5
10
15
20
25
30
35
40
45
50 (29-Jun-2011 to 28-Jun-2014)
GPSGPSoGPSe
Differences w.r.t. IERS C04 series (related to ITRF2008) have been analysed.
Slide 18 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Amplitude spectra from ERP estimates: Y component
Period [days] 10 100
Y [µ
asec
]
0
5
10
15
20
25
30
35
40
45
50 (31-Dec-2010 to 30-Dec-2013)
GPSGPSoGPSe
Differences w.r.t. IERS C04 series (related to ITRF2008) have been analysed.
Slide 18 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Amplitude spectra from ERP estimates: Y component
Period [days] 10 100
Y [µ
asec
]
0
5
10
15
20
25
30
35
40
45
50 (04-Jun-2010 to 03-Jun-2013)
GPSGPSoGPSe
Differences w.r.t. IERS C04 series (related to ITRF2008) have been analysed.
Slide 18 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Amplitude spectra from ERP estimates: Y component
Period [days] 10 100
Y [µ
asec
]
0
5
10
15
20
25
30
35
40
45
50 (06-Dec-2009 to 05-Dec-2012)
GPSGPSoGPSe
Differences w.r.t. IERS C04 series (related to ITRF2008) have been analysed.
Slide 18 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Amplitude spectra from ERP estimates: Y component
Period [days] 10 100
Y [µ
asec
]
0
5
10
15
20
25
30
35
40
45
50 (09-Jun-2009 to 08-Jun-2012)
GPSGPSoGPSe
Differences w.r.t. IERS C04 series (related to ITRF2008) have been analysed.
Slide 18 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Amplitude spectra from ERP estimates: Y component
Period [days] 10 100
Y [µ
asec
]
0
5
10
15
20
25
30
35
40
45
50 (11-Dec-2008 to 11-Dec-2011)
GPSGPSoGPSe
Differences w.r.t. IERS C04 series (related to ITRF2008) have been analysed.
Slide 18 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Amplitude spectra from ERP estimates: Y component
Period [days] 10 100
Y [µ
asec
]
0
5
10
15
20
25
30
35
40
45
50 (14-Jun-2008 to 14-Jun-2011)
GPSGPSoGPSe
Differences w.r.t. IERS C04 series (related to ITRF2008) have been analysed.
Slide 18 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Amplitude spectra from ERP estimates: Y component
Period [days] 10 100
Y [µ
asec
]
0
5
10
15
20
25
30
35
40
45
50 (17-Dec-2007 to 16-Dec-2010)
GPSGPSoGPSe
Differences w.r.t. IERS C04 series (related to ITRF2008) have been analysed.
Slide 18 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Amplitude spectra from ERP estimates: Y component
Period [days] 10 100
Y [µ
asec
]
0
5
10
15
20
25
30
35
40
45
50 (20-Jun-2007 to 19-Jun-2010)
GPSGPSoGPSe
Differences w.r.t. IERS C04 series (related to ITRF2008) have been analysed.
Slide 18 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Amplitude spectra from ERP estimates: Y component
Period [days] 10 100
Y [µ
asec
]
0
5
10
15
20
25
30
35
40
45
50 (22-Dec-2006 to 21-Dec-2009)
GPSGPSoGPSe
Differences w.r.t. IERS C04 series (related to ITRF2008) have been analysed.
Slide 18 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Amplitude spectra from ERP estimates: Y component
Period [days] 10 100
Y [µ
asec
]
0
5
10
15
20
25
30
35
40
45
50 (25-Jun-2006 to 24-Jun-2009)
GPSGPSoGPSe
Differences w.r.t. IERS C04 series (related to ITRF2008) have been analysed.
Slide 18 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Amplitude spectra from ERP estimates: Y component
Period [days] 10 100
Y [µ
asec
]
0
5
10
15
20
25
30
35
40
45
50 (27-Dec-2005 to 26-Dec-2008)
GPSGPSoGPSe
Differences w.r.t. IERS C04 series (related to ITRF2008) have been analysed.
Slide 18 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Amplitude spectra from ERP estimates: Y component
Period [days] 10 100
Y [µ
asec
]
0
5
10
15
20
25
30
35
40
45
50 (30-Jun-2005 to 29-Jun-2008)
GPSGPSoGPSe
Differences w.r.t. IERS C04 series (related to ITRF2008) have been analysed.
Slide 18 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
GPS: Two Three-Plane Constellations
Amplitude spectra from ERP estimates: Y component
Period [days] 10 100
Y [µ
asec
]
0
5
10
15
20
25
30
35
40
45
50 (01-Jan-2005 to 01-Jan-2008)
GPSGPSoGPSe
Differences w.r.t. IERS C04 series (related to ITRF2008) have been analysed.
Slide 18 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Summary and Conclusion
• The setup of satellite-, plane-, or GNSS-specific ERP- and/orGCC-parameters was implemented.
• It is enabled for internal purposes in the operational solution sinceMay 2015 and the most recent reprocessing (see Poster by Susniket al.).
• The results from a GNSS-specific setup on the NEQ-level areequivalent to independent GNSS-specific solutions.
Slide 19 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Summary and Conclusion
• The setup of satellite-, plane-, or GNSS-specific ERP- and/orGCC-parameters was implemented.
• There is almost no contribution from GLONASS to a combinedGPS+GLONASS GCC series (Z-component).
• Meindl et al (2013): due to the inclination of GLONASS satellites(64◦) the Sun may be almost perpendicular above the orbitalplane, which results in a direct correlation with dynamic orbitparameters.
Slide 19 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Summary and Conclusion
• The setup of satellite-, plane-, or GNSS-specific ERP- and/orGCC-parameters was implemented.
• There is almost no contribution from GLONASS to a combinedGPS+GLONASS GCC series (Z-component).
• The GLONASS contribution to the ERPs is mainly limited by thethree-plane constellation.
• The ERP results from the GLONASS constellation are comparableto solutions with a synthetic three-plane GPS constellation.
• The geometric effect changes in time due to the regression of thenodes of the satellite’s orbital planes.
Slide 19 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
Summary and Conclusion
• The setup of satellite-, plane-, or GNSS-specific ERP- and/orGCC-parameters was implemented.
• There is almost no contribution from GLONASS to a combinedGPS+GLONASS GCC series (Z-component).
• The GLONASS contribution to the ERPs is mainly limited by thethree-plane constellation.
• Similar limitations may be expected for Galileo and theMEO-constellation of BeiDou.
• With a full multi-GNSS analysis the constellation effect shouldbeheavily reduced, ideally eliminated.
Slide 19 of 20 Astronomical Institute, University of Bern AIUB
S.Scaramuzzaet
al.:Dep
enden
cyofGeo
dyn
amic
ParametersontheGNSSConstellation
IGSWorkshop,08.–12.February2016,Syd
ney,Australia
THANK YOUfor your attention
Publications of the satellite geodesy research group:
http://www.bernese.unibe.ch/publist
Slide 20 of 20 Astronomical Institute, University of Bern AIUB