GG S Global Geodetic Observing System (GGOS): Status and Future. Markus Rothacher, Ruth Neilan, Hans-Peter Plag

Transcription

1 2020 Global Geodetic Observing System (GGOS): Status and Future Markus Rothacher, Ruth Neilan, Hans-Peter Plag GeoForschungsZentrum Potsdam (GFZ) Jet Propulsion Laboratory (JPL) University of Nevada, Reno (UNR) AOGS 5th Annual Meeting 2008 June 16-20, 2008 Busan, Korea

2 Contents Motivation Monitoring and Modeling the Earth System Structure of GGOS GGOS Instrumentation / Infrastructure GGOS Data Flow and Portal Processing, Analysis, Combination Modeling and Interpretation Conclusions

3 Motivation: Missing Understanding of Key Processes

4 GGOS: Monitoring and Modelling the Earth s System Reference frames: highest accuracy and long-term stability Global Monitoring Space Techniques VLBI C SLR/LLR O GNSS M DORIS B Altimetry I InSAR N Gravity/Magnet. Missions A T Terrestrial I Techniques O Levelling N S Gravimetry Tide Gauges Information about Earth System Geometry Earth System Station Position/Motion, Sea Level Change, Deformation Sun/Moon I N (Planets) T Atmosphere E Ocean R Hydrosphere A C Cryosphere T I Crust O Mantle N Core S Earth Rotation Precession/Nutation, Polar Motion, UT1, LOD Gravity Geocenter Gravity Field, Temporal Variations Innovative Technologies Interpretation

5 GGOS Chronology July 2003: Decision of the International Association of Geodesy (IAG) to establish a Global Geodetic Observing System (GGOS) April 2004: IAG/GGOS becomes participating organization of GEO (Group on Earth Observation) for the realization of GEOSS (Global Earth Observing System of Systems) May 2006: GGOS becomes official member of IGOS-P (Integrated Global Observation Strategy Partnership) July 2007: GGOS becomes an official component of the IAG, the observing system of the IAG GGOS2020 reference document is almost complete, is in the review process (~ 200 pages)

6 Std Ocean Gravimetry Geometry IAG Services: Backbone of GGOS IERS: International Earth Rotation and Reference Systems Service IGS: International GNSS Service IVS: International VLBI Service ILRS: International Laser Ranging Service IDS: International DORIS Service IGFS: International Gravity Field Service BGI: Bureau Gravimetrique International IGeS: International Geoid Service ICET: International Center for Earth Tides ICGEM: International Center for Global Earth Models IDEMS: International Digital Elevation Models Service PSMSL: Permanent Service for Mean Sea Level IAS: International Altimetry Service (in preparation) BIPM: Bureau International des Poids et Mesures IBS: IAG Bibliographic Service

7 Structure of the Future GGOS Bureau for Networks and Communication Global Networks of Observing Stations Regional and Global Data and Product Centers Data Analysis Centers Bureau for Conventions and Standards Coordination Office Archiving and Dissemination Earth Observation Satellites / Planetary Missions GGOS Portal Combination Centers Missionspecific Data and Product Centers Archiving and Dissemination Bureau for Satellite and Space Missions Modeling Centers Access to all information, data, products Users, Science & Society Meta data; information Real data; information

8 GGOS Instrumentation: 5 Levels of Objects 5: Level 4: Moon,Planets Planets Moon

9 Level 1: Ground-Based Component GPS VLBI Sup.Grav. Abs.Grav. SLR/LLR DORIS Tide Gauges

10 Future Core Ground-Based Infrastructure Core Network (~ 40 Stations): 2-3 VLBI telescopes for continuous observations SLR/LLR telescope for tracking of all major satellites At least 3 GNSS antennas and receivers (controlled equipment changes) DORIS beacon of the most recent generation Ultra-stable oscillator for time and frequency keeping and transfer Terrestrial survey instruments for permanent/automated local tie monitoring Superconducting and absolute gravimeter (gravity missions, geocenter) Meteorological sensors (pressure, temperature, humidity) Seismometer for combination with deformation from space geodesy and GNSS seismology Additional sensors: water vapor radiometer, tilt-meters, gyroscopes, ground water sensors, General Characteristics: highly automated, 24-hour/365 days, latest technologies

11 Ground-Based Infrastructure: Innovation VLBI: High slew rates (> 5 deg/s) 1-3 small telescopes at a site Continuous frequency range (2-18 GHz) VLBI Twin Telescope (Wettzell) SLR: khz laser technology 2 frequency systems Higher quantum efficiency khz Laser: Lageos Spin (Graz) DORIS: 3rd generation DORIS systems Galileo Experimental Sensor Station (GESS) GNSS: GPS, Glonass, Galileo, Compass, Sampling > 10 Hz Real-time 3 antennas/receivers DORIS Beacon (Thule)

12 Level 2: Satellite Mission Component v a r G GRACE CHAMP Oce Topex/Pos. d l e i F y t i ry t e m i t l A n a JASON-1 IceSat-1 COSMIC ry t e m i t l A e Ic Cryosat-2 th r a E e c a f Sur MetOp e n g a M CHAMP TanDEM-X TerraSAR-X JASON-2 e r e h p s o m t A CHAMP GRACE Follow-on? GOCE d l e i t ic F SWARM and new mission concepts IceSat-2

13 New Mission Concepts: Constellations and Formations Formation flying, swarms Satellite Constellations

14 New Mission Concepts: GNSS Reflectometry Future satellite constellation as a component of a Multi-Hazard Early Warning System? AOGS 5 Annual Meeting 2008, June 16-20, 2008, Busan, Korea th

15 New Mission Concepts: Co-location Micro-Satellite(s) RO Antenna POD Antenna Star Sensors SLR Retro-Reflector VLBI Sender MicroSatellite 3 GPS Receiver Board (Redundancy)

16 Level 3, 4, 5: GNSS + Extraterrestrial GNSS and SLR Satellites: More than 100 GNSS satellites in 2020: GPS (24/32), GLONASS (24/19), GALILEO (30/1), QZSS (3/0), COMPASS (30/4), Cheap LAGEOS-type satellites with laser retro-reflectors and with GNSS receivers forming a network in space with internally 1 mm accuracy (distances up to km) Geodetic Planetary Missions: Bepi Colombo, Mars missions, lunar exploration (GRAIL, LEO), Stars (observed with CCD cameras or in future with GAIA) Quasars

17 GGOS Data Flow and Portal Network Synergies: Common data communication and infrastructure for all techniques (archiving, ) Real-time data transfer New communication technologies for remote areas

18 Processing, Analysis, Combination Processing and Analysis: Fully automated processing in near real-time or even in real-time (early warning systems, GNSS seismology, atmosphere sounding, ) Full reprocessing capabilities for all data available, long consistent time series for long-term trends Combination of all data types on the observation level Combination with LEO data (co-location, gravity, geocenter, atmosphere, ) Combination with satellite altimetry data (and with InSAR?) Combination with terrestrial data (e.g. gravity field, ) Combination of different analysis centers (redundancy, reliability, accuracy, ) Improvements in modeling, parameterization, conventions Supercomputers, visualization

19 Combination: Tsunami Early Warning System GNSS receivers

20 Combination of GNSS / Seismology Height [m] East [m] North [m] Sumatra Earthquake of September 12, 2007 Earth`s motion during the earthquake combination with seismometers Deformation due to the earthquake (magnitude determination, rupture process)

21 Tsunami Buoy: GPS / OBPU / Seismometer

22 GPS Tsunami Buoy: Motion Horizontal Position (Days): Height: Waves:

23 Tsunami Buoy: Sea Level Height RMS: ~ 2-3 cm Tsunami: ~ 50 cm Filtered GPS Heights Ocean Bottom Pressure Ocean Tidal Model (GOTT)

24 Combination of Geometry and Gravity (IERS/IGFS) GEOMETRY IERS Ellipsoidal heights GPS, Altimetry, INSAR Remote Sensing Leveling Sea Level IGFS REFERENCE SYSTEMS VLBI, SLR, LLR, GPS, DORIS Physical heights, geoid EARTH ROTATION GRAVITY FIELD VLBI, SLR, LLR, GPS, DORIS Classical: Astronomy New: Ringlasers, Gyros Orbit Analysis Satellite Gradiometry Ship-& Airborne Gravimetry Absolute Gravimetry Gravity Field Determination

25 Earth System Modelling Tides of the solid Earth Lunisolar Gravitational acceleration Oceanic tides Atmospheric tides Angular torques Density variations in the atmosphere Atmospheric loading Angular momentum variation of the atmosphere Effects from Earth interior Ocean circulation Global ground water Snow Ocean loading Angular momentum variation of the oceans Deformation of the Earth Precession,Nutation Polar motion Length of day Postglacial land uplift Tectonic plate motion Volcanism Earthquakes Pole tides Orientation of the Earth Global vegetation Gravity Field of the Earth

26 Example: Sea-Level Change & Ice-Mass Balances Data processing Altimetry missions Envisat ICESat Gravimetry missions Jason-1 CryoSat II GRACE Geodynamic modeling Ocean modeling Terrestrial networks Sea-level change (mm/a) Tide gauge Glacial-isostatic adjustment GPS Geoid change (mm/a)

27 Conclusions Geodesy can contribute significantly to the monitoring and understanding of the Earth system Integration of a multitude of different and innovative sensors on the ground and in space into a GGOS Complete and consistent data processing chains ranging from the acquisition to the processing of vast amounts of observational data Combination and assimilation of the geodetic/geophyiscal parameters into complex numerical models of the Earth system This will finally allow the understanding and prediction of the processes in the Earth system for the benefit of human society.

28 Thank you for your attention!