64
S. Scaramuzza et al.: Dependency of Geodynamic Parameters on the GNSS Constellation IGS Workshop, 08.–12. February 2016, Sydney, Australia Dependency of Geodynamic Parameters on the GNSS Constellation S. Scaramuzza, R. Dach, G. Beutler, D. Arnold, A. J¨ aggi Astronomical Institute, University of Bern, Switzerland Session: Plenary #06 — Reference Frame IGS Workshop, 08.–12. February 2016, Sydney, Australia Slide 1 of 20 Astronomical Institute, University of Bern AIUB

Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

  • Upload
    others

  • View
    3

  • Download
    0

Embed Size (px)

Citation preview

Page 1: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 2: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 3: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 4: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 5: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 6: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 7: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 8: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 9: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 10: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 11: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 12: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 13: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 14: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 15: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 16: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 17: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 18: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 19: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 20: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 21: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 22: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 23: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 24: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 25: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 26: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 27: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 28: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 29: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 30: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 31: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 32: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 33: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 34: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 35: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 36: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 37: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 38: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 39: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 40: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 41: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 42: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 43: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 44: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 45: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 46: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 47: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 48: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 49: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 50: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 51: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 52: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 53: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 54: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 55: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 56: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 57: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 58: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 59: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 60: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 61: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 62: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 63: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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

Page 64: Dependency of Geodynamic Parameters on the GNSS Constellationacc.igs.org/workshop2016/presentations/Plenary_06_02.pdf · 2016. 2. 22. · GNSS Constellation IGS Workshop, 08.–12

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