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A comparison of R1 and R4 IVS networks S.B. Lambert, Royal Observatory of Belgium, formerly at NVI, Inc./US Naval Observatory A.-M. Gontier, Paris Observatory

A comparison of R1 and R4 IVS networks S.B. Lambert, Royal Observatory of Belgium, formerly at NVI, Inc./US Naval Observatory A.-M. Gontier, Paris Observatory

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Page 1: A comparison of R1 and R4 IVS networks S.B. Lambert, Royal Observatory of Belgium, formerly at NVI, Inc./US Naval Observatory A.-M. Gontier, Paris Observatory

A comparison of R1 and R4 IVS networks

S.B. Lambert,Royal Observatory of Belgium, formerly at NVI, Inc./US Naval Observatory

A.-M. Gontier,Paris Observatory

Page 2: A comparison of R1 and R4 IVS networks S.B. Lambert, Royal Observatory of Belgium, formerly at NVI, Inc./US Naval Observatory A.-M. Gontier, Paris Observatory

Two parallel networks running since 2002

Overview of the networks

R1 (Mondays), 13 sites R4 (Thursdays), 10 sites

Page 3: A comparison of R1 and R4 IVS networks S.B. Lambert, Royal Observatory of Belgium, formerly at NVI, Inc./US Naval Observatory A.-M. Gontier, Paris Observatory

Overview of the networks

R1 (Mondays), 13 sites R4 (Thursdays), 10 sites

Question: are the networks consistent?Question: are the networks consistent?

Can they realize identically EOP and reference systems?Can they realize identically EOP and reference systems?

Page 4: A comparison of R1 and R4 IVS networks S.B. Lambert, Royal Observatory of Belgium, formerly at NVI, Inc./US Naval Observatory A.-M. Gontier, Paris Observatory

Overview of the networks

R1 (Mondays), 13 sites R4 (Thursdays), 10 sites

2002 2003 2004 2005

> 10,000 GILCGILC

HARTHART

MATEMATE

NYALNYAL

ONSAONSA

TSUKTSUK

WESTWEST

WETTWETT

GILCGILC

KOKEKOKE

MATEMATE

TSUKTSUK

WESTWEST

WETTWETT

GILCGILC

NYALNYAL

TSUKTSUK

WESTWEST

WETTWETT

GILCGILC

TSUKTSUK

WESTWEST

WETTWETT

5,000-10,000

ALGOALGO

KOKEKOKE

HARTHART

SESHSESH

TIGOTIGO

HARTHART

KOKEKOKE

MEDIMEDI

SESHSESH

TIGOTIGO

HARTHART

HOBAHOBA

KOKEKOKE

MEDIMEDI

ONSAONSA

TIGOTIGO

< 5,000 MEDI

TIGO

HOBA

MEDI

NYAL

HOBA

ONSA

NYAL

SESH

SVET

2002 2003 2004 2005

> 10,000 ALGOALGO

GILCGILC

KOKEKOKE

NYALNYAL

WETTWETT

ALGOALGO

FORTFORT

GILCGILC

KOKEKOKE

MATEMATE

NYALNYAL

WETTWETT

ALGOALGO

GILCGILC

KOKEKOKE

NYALNYAL

SVETSVET

WETTWETT

ALGOALGO

FORTFORT

GILCGILC

KOKEKOKE

NYALNYAL

SVETSVET

WETTWETT

5,000-10,000

FORTFORT FORTFORT

< 5,000 HOBA

MATE

SESH

ONSA

SVET

TIGO

TSUK

MEDI

ONSA

TIGO

HART

MEDI

TIGO

Page 5: A comparison of R1 and R4 IVS networks S.B. Lambert, Royal Observatory of Belgium, formerly at NVI, Inc./US Naval Observatory A.-M. Gontier, Paris Observatory

Sensitivity of a baseline to Earth orientation, where X, Y and Z are the station coordinates:

“permanent” network all sites

EOP and baseline geometry

xX 2 Z 2

yY 2 Z 2

UT1UTC

X 2 Y 2

x

y

UT1

Page 6: A comparison of R1 and R4 IVS networks S.B. Lambert, Royal Observatory of Belgium, formerly at NVI, Inc./US Naval Observatory A.-M. Gontier, Paris Observatory

Description of the solution

Solution run with R1 sessions only, then with R4 sessions only

Global: site positions and velocities, antenna axes, source positions

Arc: polar motion and rate, UT1-UTC and rate, nutation offsets

NNR and NNT on all sites except MEDICINA and GILCREEK (known episodic motions)

NNR on 212 ICRF defining sources

Made with CALC/SOLVE software

Compared against IERS Bulletin A (USNO combined solution)

Page 7: A comparison of R1 and R4 IVS networks S.B. Lambert, Royal Observatory of Belgium, formerly at NVI, Inc./US Naval Observatory A.-M. Gontier, Paris Observatory

Comparison of EOP solutions

Difference to IERS Bulletin A, mean standard error about 300 as

Page 8: A comparison of R1 and R4 IVS networks S.B. Lambert, Royal Observatory of Belgium, formerly at NVI, Inc./US Naval Observatory A.-M. Gontier, Paris Observatory

Comparison of TRF

7-parameter Helmert transformation to compare individual TRF against ITRF

Number of sites

R1 R4

Page 9: A comparison of R1 and R4 IVS networks S.B. Lambert, Royal Observatory of Belgium, formerly at NVI, Inc./US Naval Observatory A.-M. Gontier, Paris Observatory

What shows up in operational series?

Difference to IERS Bulletin A, standard error about 300 as

Page 10: A comparison of R1 and R4 IVS networks S.B. Lambert, Royal Observatory of Belgium, formerly at NVI, Inc./US Naval Observatory A.-M. Gontier, Paris Observatory

Conclusion

• Compares the 2 parallel 24-hour R1 and R4 networks run by the IVS

• Looks at the possible influence of geometry, EOP and TRF realizations

• Evolution of R1 between 2002 and 2005 greatly improved the R1 series : sites in the southern hemisphere after 2003

• Current R1 and R4 residuals against IERS Bulletin A have same standard deviationCurrent R1 and R4 residuals against IERS Bulletin A have same standard deviation

• R1 network more extended than R4 but with a reduced East-West “permanent” network

• R4 smaller but “permanent”

• R1-derived TRF closer to ITRF than R4-derived TRF but with larger uncertaintiesR1-derived TRF closer to ITRF than R4-derived TRF but with larger uncertainties

• Inconsistencies show up in operational series (drift of 30 Inconsistencies show up in operational series (drift of 30 as per year)as per year)