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Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU [email protected] [email protected] ENVISAT Orbit & RA2 CCVT in Newcastle University

Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU [email protected]

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Page 1: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

Philip Moore

Jiasong Wang

School of Civil Engineering and Geosciences

University of Newcastle upon Tyne

Newcastle upon Tyne

NE1 7RU

[email protected]

[email protected]

ENVISAT Orbit & RA2 CCVT in Newcastle University

Page 2: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

ENVISAT Precise Orbit Determination

Force ModelGravity model

3-body perturbation

Earth tides

Ocean tides

Atmospheric density

SRP + Albedo + Infrared

Relativity

Param (Dynamic)

Param (Reduced Dyn)

GRIM5-C1(120×120)

DEC403 JPL Eph

IERS96

GOT99

MSIS86

Macro/ESA; SRP factor = 1

Schwarzschild

6-hour drag+daily 1cpr along/cross track

6-hour drag+hourly 1cpr along/cross track

Sigma=5.E-9m/s/s

Correl. Time = 3 hours

Page 3: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

Altimeter Range model adopted

Model Source ENVISAT / ERS2

Total geocentric

ocean tide (1) + pole tide

Solid earth tide

Dry troposphere

Wet troposphere

Ionosphere

Inverse Barometer

Sea state bias

Orbit

GOT99: ENVISAT from GDR; model for ERS2

Model (from GDR): both satellites

Model (from GDR): both satellites

Model (from GDR): both satellites

GIM + scale from IRI95: both satellites

ENVISAT from GDR; inferred for ERS2

Model (from GDR): both satellites

From GDR or NCL POD

Page 4: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

0

1

2

3

4

5

6

7

c10-1

c10-2

c10-3A

c10-3B

c10-4

c10-5

c11-1A

c11-1B

c11-2

c11-3

c11-4A

c11-4B

c11-5

SLR(redu) DORI S(redu) SLR(dyn) DORI S(dyn)

RMS of SLR (cm) and DORIS RMS (0.1mm/s)

residuals in NCL POD

Page 5: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

0

0. 5

1

1. 5

2

2. 5

3

3. 5

c10-1

c10-2

c10-3A

c10-3B

c10-4

c10-5

c11-1A

c11-1B

c11-2

c11-3

c11-4A

c11-4B

c11-5

NCL-DEOS CNES-DEOS NCL-DEOS

RMS radial orbit difference (cm) for

ENVISAT cycles 10 and 11

Page 6: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

0

1

2

3

4

5

6

7

8

c10-1

c10-2

c10-3A

c10-3B

c10-4

c10-5

c11-1A

c11-1B

c11-2

c11-3

c11-4A

c11-4B

c11-5

NCL-DEOS CNES-DEOS NCL-CNES

RMS cross-track orbit difference (cm) for ENVISAT cycles 10 and 11

Page 7: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

Radial orbit difference between reduced dynamic and dynamic POD: RMS values over 4º long. by 2º lat. bins

Page 8: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

Radial orbit difference between DEOS and NCL (cyc10)

RMS values 4º long. by 2º lat. bins

Page 9: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

Radial orbit difference between DEOS and NCL (cyc11):

RMS values over 4º long. by 2º lat. bins

Page 10: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

Altimeter statistics

Flag Rejected

Cyc 10

Rejected

Cyc 11

1. Land 673042 667684

2. Shallow water

(reject if > -1000m)

311764 260787

3. SWH = 0 90339 78204

4. Tide (reject if > 20m) 936 1016

5. Peakiness (reject if

<1.5 or > 1.8)

75382 69038

Total rejected 1151463 1076729

Accepted 933856 945734

Page 11: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

RMS of crossover residuals cycles 10-11:

CNES v NCL reduced SLR+DORIS orbit

6

6. 5

7

7. 5

8

8. 5

c10-1

c10-2

c10-3A

c10-3B

c10-4

c10-5

c11-1A

c11-1B

c11-2

c11-3

c11-4A

c11-4B

c11-5

CNESReduDyn

Page 12: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

Sea State bias and altimeter time tag estimation from single crossovers

orbit 1 = CNES; orbit 2 = NCL (Reduced dynamic);

• Max time diff=5day, rejection criterion 20cm

Orbit Used/rejected RMS change t(ms) SSB: %SWH

1/Cyc 10

2/Cyc 10

6003/319

6030/292

9.46—7.25cm

9.23—6.94cm

0.01 ±0. 36

-0.01 ±0. 36

4.85 ± 1.03

4.83 ± 1.02

1/Cyc 11

2/Cyc 11

4791/582

5132/241

9.26—7.29cm

8.81—6.80cm

-0.17 ± 0.40

-0.20 ± 0.39

4.29 ± 1.08

4.16 ± 1.03

Note: SSB given as % of SWHConclusion: Results independent of orbit

Page 13: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

Sea State bias and altimeter time tag estimation from single crossover

Max time diff = 5day, NCL orbit applied, for Cyc 10 +11

Reject

level

Used/rejected RMS change t(ms) SSB: %SWH

60cm 11347/348 9.81—7.71cm -0.10 ± 0.26 4.62 ± 0.71

20cm 11154/540 9.03—6.87cm -0.09 ± 0.26 4.53 ± 0.73

Conclusion: Rejection level unimportant

Page 14: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

ENVISAT - ERS2 SSH: Ascending passes

Corrections applied: sea state bias and USO drift (ERS2) only

Page 15: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

ENVISAT - ERS2 SSH: Descending passesCorrections applied: sea state bias and USO drift (ERS2) only

Page 16: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

ENVISAT - ERS2 SSH: All passesAll Corrections applied:

Page 17: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

Note: All corrections applied:

descending pass mean = 118.1cm ;

ascending pass mean = 115.0cm

Page 18: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

Differences between ENVISAT (cyc 10) and ERS2 (cyc 78) solid Earth tide corrections: Note mean = -1.1cm

Page 19: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

Differences between ENVISAT (cyc 11) and ERS2 (cyc 79) solid Earth tide corrections: Note mean = -0.8cm

Page 20: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

Differences between ENVISAT (cyc 10) and ERS2 (cyc 78) total tidal corrections. Note mean = 1.4cm. Noise from total geocentric ocean tides, see next slide

Page 21: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk
Page 22: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

Differences between ENVISAT (cyc 10) and ERS2 (cyc 78) inverse barometer corrections: Note mean = -3.0cm

Page 23: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

Differences between ENVISAT (cyc 11) and ERS2 (cyc 79) inverse barometer corrections: Note mean = -2.8cm

Page 24: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

Differences between ENVISAT (cyc 10) and ERS2 (cyc 78)iono+wet+dry+inverse bar. corrections: Note mean = -3.1cm

Page 25: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

Differences between ENVISAT (cyc 10) and ERS2 (cyc 78) wet trop. Correction: Note mean = -0.4cm

Page 26: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

Differences between ENVISAT (cyc 10) and ERS2 (cyc 78)iono (GIM) corrections: Note mean = 0.14cm

Page 27: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

ENVISAT (cyc 10): mean = 1.237m

Page 28: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

ENVISAT (cyc 11): mean = 1.237m again!!

Page 29: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

Conclusions

• Orbits – agree to near 2cm RMS radially between analysis

centres– Reduced dynamic is better than dynamic OD

• Sea-state bias– Zero values (for very low wave heights??)– Assuming wave heights correct first look SSB

4.6% SWH – Non-parametric approximation not yet applied

Page 30: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

Conclusions

• Altimetry correction (Cyc10, 11)– inverse barometer correction has a bias of -3.0cm with

ERS2

– tide effect is different from ERS2 with mean=-1.4cm

• Crossover residuals – RMS about 7cm; shows benefit of DORIS tracking and

to a lesser extent dual frequency altimeter.

Great results c.f. 6.0cm for TOPEX/Poseidon

Page 31: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk

•Sea surface height (SSH) difference with ERS2 (Cyc10, 11)

–With only SSB correction applied, bias=112cm

–With all corrections for both satellite , bias=117cm

–For Ascending pass and descending pass , 3cm difference for this relative bias calculation. Within error bars?

•SSH compared with mean sea surface (CLS01) (Cyc10)

– Bias=123.7cm (ENVISAT Cyc 10)

– Bias=5.4cm (ERS2 Cyc 078)

– relative bias = 118.3cm between two satellites

Conclusions

Page 32: Philip Moore Jiasong Wang School of Civil Engineering and Geosciences University of Newcastle upon Tyne Newcastle upon Tyne NE1 7RU philip.moore@ncl.ac.uk