03/000 vlbi network design australian government geoscience australia ngrs workshop, 1-2 february,...

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03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

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ICRF catalogue (1998) Geoscience Australia 17 August defining sources with position accuracy ~0.4 mas candidate sources other sources 608 sources separated into 3 groups

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Page 1: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

03/000

VLBI network design

Australian Government

Geoscience Australia

NGRS Workshop, 1-2 February, Canberra

Page 2: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

Geoscience

Australia17 August 2005

Page 3: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

ICRF catalogue (1998)

Geoscience Australia

17 August 2005

1.212 defining sources with position accuracy ~0.4 mas

2.294 candidate sources

3.102 other sources

608 sources separated into 3 groups

Page 4: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

Radiotelescopes in Australia

Geoscience Australia

28 June 2004

Page 5: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

ICRF defining sources

Geoscience Australia

17 August 2005

Page 6: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

ICRF source instability(quasar 2145+067)

Geoscience Australia

17 August 2005

Year

1994 1996 1998 2000 2002 2004

mse

c

-0.10

-0.08

-0.06

-0.04

-0.02

0.00

0.02

0.04

0.06

0.08

Daily estimatesApproximation

Instability~0.2 mas( 6 mm )

Page 7: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

ICRF source instability

Geoscience Australia

17 August 2005

It is important to monitor all radiosources to mitigate the effect of instability

About 60 defining sources from the ICRF catalogue are appeared to be unstable!

New ICRF realization wanted now

Page 8: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

Geoscience

Australia17 August 2005

Page 9: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

Radiotelescopes in Australia

Geoscience Australia

17 August 2005

Page 10: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

Geoscience

Australia17 August 2005

Hobart,26-meterantenna

Too far from all other telescopes;Limited amount of defining sources in southern hemisphere – problems with scheduling;Slow slew rate (1 deg/sec) – little data

Page 11: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

Problem

Geoscience Australia

17 August 2005

- set of radiosources to be fixed (212 defining sources);

- if unstable radiosources are fixed the geodetic results will be corrupted;

- effect of the instability of the fixed radiosources on the TRF solution has never been studied!

Page 12: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

Procedure

Geoscience Australia

17 August 2005

- two global VLBI solutions have been obtained by identical way;

- Solution 1: 207 ICRF defining sources;

- Solution 2: 199 ‘stable’ sources (Feissel-Vernier);

- daily TRF solutions have been obtained for Sol #1 and #2 providing two sets of time series of VLBI site geodetic positions;

- differences of the daily geodetic positions were calculated;

- measure of discrepancy between two solution

Page 13: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

TRF daily difference time series

Geoscience Australia

17 August 2005

Height differencesWestford

Year

1980 1985 1990 1995 2000 2005

met

er

-0.15

-0.10

-0.05

0.00

0.05

0.10

0.15

Height componentOnsala60

Year

1976 1980 1984 1988 1992 1996 2000 2004m

eter

-0.15

-0.10

-0.05

0.00

0.05

0.10

0.15

Page 14: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

Geoscience

Australia17 August 2005

Heght differencesNy-Alesund

Year

1994 1996 1998 2000 2002 2004 2006m

eter

-0.15

-0.10

-0.05

0.00

0.05

0.10

0.15

TRF daily difference time series

Height componentKokee

Year

1992 1994 1996 1998 2000 2002 2004 2006

met

er

-0.15

-0.10

-0.05

0.00

0.05

0.10

0.15

Page 15: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

Geoscience

Australia17 August 2005

TRF daily difference time series

Height componentTigoconc

Year

2002 2003 2004 2005 2006

met

er

-0.15

-0.10

-0.05

0.00

0.05

0.10

0.15

Height positionSvetloe

Year

2003.0 2003.5 2004.0 2004.5 2005.0 2005.5

met

er-0.15

-0.10

-0.05

0.00

0.05

0.10

0.15

Page 16: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

Geoscience

Australia17 August 2005

TRF daily difference time series

Height component,Hobart

Year

1988 1992 1996 2000 2004

met

er

-0.15

-0.10

-0.05

0.00

0.05

0.10

0.15

Height componentHartrao

Year

1984 1988 1992 1996 2000 2004

met

er

-0.15

-0.10

-0.05

0.00

0.05

0.10

0.15

Page 17: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

wrms and offset of the TRF solution

Geoscience Australia

17 August 2005

Station Latitude(º)

wrms (mm)

Offset(mm)

height latitude longitude height latitude longitude

Algopark 46 5.5 3.0 2.1 0.9 +/- 0.3 0.2 +/- 0.2 0.1 +/- 0.1

DSS45 -35 13.5 9.7 4.6 3.0 +/- 1.7 -0.5 +/- 1.2 -0.7 +/- 0.6

Fortaleza -4 8.6 4.7 3.7 -1.2 +/- 0.4 -0.5 +/- 0.2 0.0 +/- 0.2

Hartrao -25 15.4 7.2 5.2 -1.6 +/- 0.9 -1.4 +/- 0.5 0.2 +/- 0.3

Hobart26 -43 20.4 10.2 9.3 10.6 +/- 1.4 -3.9 +/- 0.7 -0.8 +/- 0.6

Kokee 22 4.8 3.1 3.4 -0.2 +/- 0.2 0.6 +/- 0.1 0.1 +/- 0.1

Medicina 45 3.5 2.7 1.7 0.6 +/- 0.4 0.1 +/- 0.3 -0.3 +/- 0.2

Ny-Alesund 79 3.5 1.4 1.5 -0.3 +/- 0.3 0.0 +/- 0.1 -0.2 +/- 0.1

O’Higgins -63 11.8 6.2 5.9 1.9 +/- 1.8 1.9 +/- 0.9 -0.6 +/- 0.9

Onsala60 57 3.2 2.0 2.1 0.0 +/- 0.1 0.1 +/- 0.1 -0.1 +/- 0.1

Seshan25 31 7.2 2.7 3.3 -0.2 +/- 1.8 0.3 +/- 0.7 -0.2 +/- 0.8

Svetloe 60 4.4 3.9 1.6 -6.9 +/- 7.6 -6.9 +/- 7.5 -3.1 +/- 3.0

Tigoconc -37 16.3 9.4 4.9 24.3 +/- 8.5 -17.8 +/- 4.4 2.7 +/- 2.9

Westford 43 5.4 2.9 2.6 1.0 +/- 0.1 0.5 +/- 0.1 0.0 +/- 0.1

Wettzell 49 4.7 3.0 2.4 0.0 +/- 0.1 0.6 +/- 0.1 -0.4 +/- 0.1

Page 18: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

Geoscience

Australia17 August 2005

Effect on the TRF quality (wrms vs latitude)

height component wrms vs latitude

latitude

-90 -60 -30 0 30 60 90

mm

0

5

10

15

20

25

Page 19: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

Geoscience

Australia17 August 2005

Hobart daily difference time series

Height component,Hobart

Year

1988 1992 1996 2000 2004

met

er

-0.15

-0.10

-0.05

0.00

0.05

0.10

0.15

The number of observations per session

0 100 200 300 400 500 600

Met

er

-0.15

-0.10

-0.05

0.00

0.05

0.10

0.15

Page 20: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

Hobart’s problem

Geoscience Australia

17 August 2005

- poor reference sources due to geographical location

- insufficient amount of data due to low slew rate

Page 21: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

Hobart’s problem solution

Geoscience Australia

17 August 2005

- ICRF (0.1 mas)

ITRF (1 mm)

high slew rate dish

IVS

Australian

more data

more sources

Australian geodetic datum

better reference sourcepositions

GPS

SLR

Page 22: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

Conclusion

Geoscience Australia

17 August 2005

- ICRF deficiency causes uncertainties in geodetic positions as much as 10-20 mm for VLBI sites in Southern hemisphere;

- more good radiosources for schedule

- more radiosources

- more VLBI stations with high slew rate 5 deg/sec

- potentially we can reach ~ 1 mm or better by 2010

Page 23: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

criteria

Geoscience Australia

17 August 2005

Page 24: 03/000 VLBI network design Australian Government Geoscience Australia NGRS Workshop, 1-2 February, Canberra

Geoscience

Australia17 August 2005

ICRF instability(wrms vs declination)

Weighted RMS on vs declination

Declination

-90 -60 -30 0 30 60 90

mas

0.0

0.5

1.0

1.5

2.0

Weighted RMS on cos vs declination

Declination

-90 -60 -30 0 30 60 90

mas

0.0

0.2

0.4

0.6

0.8

1.0