precise science orbits for the goce satellite – …...goce workshop at esa lp symposium, bergen,...

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GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010 Precise Science Orbits for the GOCE Satellite – Aiming at the cm-level H. Bock 1 , A. Jäggi 1 , U. Meyer 1 , G. Beutler 1 , M. Heinze 2 1 Astronomical Institute, University of Bern, Switzerland 2 Institute of Astronomical and Physical Geodesy (IAPG), TU München, Germany

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Page 1: Precise Science Orbits for the GOCE Satellite – …...GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010 Precise Science Orbits for the GOCE Satellite – Aiming at the

GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010

Precise Science Orbits for the GOCE Satellite –

Aiming at the cm-level

H. Bock1, A. Jäggi1, U. Meyer1, G. Beutler1, M. Heinze2

1Astronomical Institute, University of Bern, Switzerland2Institute of Astronomical and Physical Geodesy (IAPG),

TU München, Germany

Page 2: Precise Science Orbits for the GOCE Satellite – …...GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010 Precise Science Orbits for the GOCE Satellite – Aiming at the

GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010

GOCE-HPF: Orbit groupsGOCE-HPF: Orbit groups

Responsibilities:

• DEOS => RSO(Rapid Science Orbit)

• AIUB => PSO (Precise Science Orbit)

• IAPG => Validation

Page 3: Precise Science Orbits for the GOCE Satellite – …...GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010 Precise Science Orbits for the GOCE Satellite – Aiming at the

GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010

GOCE Precise Science OrbitsGOCE Precise Science Orbits

GOCE instruments data used:• 1 Hz GPS data of highest

quality• Star tracker measurements

Precise Science Orbit product

PSO is a Level 2 product consistingof two different orbit solutions:

• Kinematic• Reduced-dynamic

Page 4: Precise Science Orbits for the GOCE Satellite – …...GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010 Precise Science Orbits for the GOCE Satellite – Aiming at the

GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010

• A kinematic orbit is an ephemeris at discrete measurement epochs

• Kinematic positions are fully independent of the force models used for LEO orbit determination

• Kinematic orbits are well suited for gravity field recovery of the long- wavelength part

Kinematic orbit representationKinematic orbit representation

Page 5: Precise Science Orbits for the GOCE Satellite – …...GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010 Precise Science Orbits for the GOCE Satellite – Aiming at the

GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010

• Satellite trajectory is a particular solution of the equation of motion defined by the force models used. The strength of the force models is reduced, to some extent, by additional empirical parameters.

• Reduced-dynamic orbits heavily depend on the force models used, e.g., on the gravity field model (solving the equation of motion)

• Reduced-dynamic orbits are well suited to compute LEO orbits of highest quality

Reduced-dynamic orbit representationReduced-dynamic orbit representation

Page 6: Precise Science Orbits for the GOCE Satellite – …...GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010 Precise Science Orbits for the GOCE Satellite – Aiming at the

GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010

Special GOCE characteristic: Drag-free flightSpecial GOCE characteristic: Drag-free flight

Transition to first drag-free flight on 7 May 2009

Empirical accelerations from reduced-dynamic orbit determination

Page 7: Precise Science Orbits for the GOCE Satellite – …...GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010 Precise Science Orbits for the GOCE Satellite – Aiming at the

GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010

Special GOCE characteristic: Drag-free flightSpecial GOCE characteristic: Drag-free flight

• Non-gravitational forces in along-track direction are compensated by the IPA (Ion Propulsion Assembly)

• Empirical accelerations from reduced-dynamic orbit determination illustrate the effect

Page 8: Precise Science Orbits for the GOCE Satellite – …...GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010 Precise Science Orbits for the GOCE Satellite – Aiming at the

GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010

Special GOCE characteristics: Observation epochsSpecial GOCE characteristics: Observation epochs

• Internal clock is not steered to integer seconds

• This is no problem for the GPS data processing but

=> resulting kinematic positions are not truly equidistant

Fractional offsets of observation epochs at midnight (from RINEX)

Page 9: Precise Science Orbits for the GOCE Satellite – …...GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010 Precise Science Orbits for the GOCE Satellite – Aiming at the

GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010

GOCE PSO procedureGOCE PSO procedure

CODE products

GOCE GPS data

GOCE attitude data

Auxiliary data

Preparation of GPS orbits, clocks

and ERPs (30 hours)

Pseudorange:first a priori orbit

Receiver clock synchronization

Phase:Iterative data

screening

Reduced-dynamic orbit

solution (iterative)

Kinematic orbit solution

Data pre-processing

Piece-wise constant accelerations (6 min)

a priori10 sec

1 sec

• Tailored version of Bernese GPS Software used

• Un-differenced processing• 30 h batches

=> overlaps• CODE final products• Consequent use of antenna

phase center variation (PCV) map

• Final kinematic positions are only accepted, if five or more simultaneous observations were available=> on average only 0.5% positions missing

Page 10: Precise Science Orbits for the GOCE Satellite – …...GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010 Precise Science Orbits for the GOCE Satellite – Aiming at the

GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010

GOCE PSO procedure: ImprovementsGOCE PSO procedure: Improvements

• GOCE SLR residuals as a function of the azimuth of the SLR stations

• Significant improvement of SLR residuals due to use of the PCV map

Page 11: Precise Science Orbits for the GOCE Satellite – …...GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010 Precise Science Orbits for the GOCE Satellite – Aiming at the

GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010

GOCE PSO procedure: PCV mapGOCE PSO procedure: PCV map

• Azimuth-elevation diagram of antenna PCVs [mm] – ionosphere-free linear combination

• Azimuth of 0o => flight direction

• 154 days of data used for the generation of the PCV map

Page 12: Precise Science Orbits for the GOCE Satellite – …...GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010 Precise Science Orbits for the GOCE Satellite – Aiming at the

GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010

PSO: Comparison reduced-dynamic kinematic orbitsPSO: Comparison reduced-dynamic kinematic orbits

• Orbit differences between reduced-dynamic and kinematic PSO solutions

• Orbit differences > 1 m removed (only 60 positions for the whole period)

• Consistency of reduced-dynamic and kinematic PSO is at 2 cm level=> mean 3D-RMS 1.82 cm

Page 13: Precise Science Orbits for the GOCE Satellite – …...GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010 Precise Science Orbits for the GOCE Satellite – Aiming at the

GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010

PSO: Comparison reduced-dynamic kinematic orbitsPSO: Comparison reduced-dynamic kinematic orbits

Typical example fororbit differences betweenreduced-dynamic andkinematic PSO

Page 14: Precise Science Orbits for the GOCE Satellite – …...GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010 Precise Science Orbits for the GOCE Satellite – Aiming at the

GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010

PSO: Overlaps reduced-dynamic orbitsPSO: Overlaps reduced-dynamic orbits

• 5 h overlaps (21:30 – 02:30)• Mean 3D-RMS: 0.55 cm

Page 15: Precise Science Orbits for the GOCE Satellite – …...GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010 Precise Science Orbits for the GOCE Satellite – Aiming at the

GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010

Reduced-dynamic orbit Mean: 0.88 cm, RMS: 2.05 cm

Orbit validation with SLROrbit validation with SLR

Page 16: Precise Science Orbits for the GOCE Satellite – …...GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010 Precise Science Orbits for the GOCE Satellite – Aiming at the

GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010

Orbit validation with SLROrbit validation with SLR

Kinematic orbit Mean: 0.88 cm, RMS: 2.23 cm

Page 17: Precise Science Orbits for the GOCE Satellite – …...GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010 Precise Science Orbits for the GOCE Satellite – Aiming at the

GOCE Workshop at ESA LP Symposium, Bergen, 29./30.June, 2010

SummarySummary

• GOCE PSO product consists of a kinematic and a reduced- dynamic orbit solution

• Both orbits are computed in one and the same processing chain

• Use of PCV map led to a significant improvement of the PSO product

• Validation with independent SLR measurements shows that precision requirements of 2 cm are amply met by the PSO