WHY DOES THE IGS CARE ABOUT EOPs?

Slides:



Advertisements
Similar presentations
Dennis D. McCarthy Elements of Prediction. Why are we here? IERS Working Group on Predictions IERS Working Group on Predictions Definitive user requirements.
Advertisements

Where do precise orbits and clocks come from? Kristine M. Larson ASEN 6090 Spring 2010.
Processing of VLBI observation in St. Petersburg University Kudryashova Maria Astronomical Institute of Saint Petersburg University.
Reference Frames for GPS Applications and Research
On the alternative approaches to ITRF formulation. A theoretical comparison. Department of Geodesy and Surveying Aristotle University of Thessaloniki Athanasios.
Effect of Surface Loading on Regional Reference Frame Realization Hans-Peter Plag Nevada Bureau of Mines and Geology and Seismological Laboratory University.
Jim Ray & Jake Griffiths, NOAA/National Geodetic Survey Xavier Collilieux & Paul Rebischung, IGN/LAREG S UBSEASONAL GNSS P OSITIONING E RRORS Linear rate.
Jake Griffiths & Jim Ray NOAA/National Geodetic Survey Acknowledgement: Kevin Choi SUBDAILY ALIAS AND DRACONITIC ERRORS IN THE IGS ORBITS Harmonics of.
A quick GPS Primer (assumed knowledge on the course!) Observables Error sources Analysis approaches Ambiguities If only it were this easy…
2-3 November 2009NASA Sea Level Workshop1 The Terrestrial Reference Frame and its Impact on Sea Level Change Studies GPS VLBI John Ries Center for Space.
Institut for Geodesy Research Unit Earth Rotation and Global Dynamic Processes Earth Orientation Parameters from Lunar Laser Ranging Liliane Biskupek Jürgen.
Laser Ranging Contributions to Earth Rotation Studies Richard S. Gross Jet Propulsion Laboratory California Institute of Technology Pasadena, CA 91109–8099,
Know the Earth…Show the Way NATIONAL GEOSPATIAL-INTELLIGENCE AGENCY Approved for Public Release NGA Case # NGA’s Role in GPS Barbara Wiley.
Jim Ray & Jake Griffiths, NOAA/National Geodetic Survey Xavier Collilieux & Paul Rebischung, IGN/LAREG S UBSEASONAL GNSS P OSITIONING E RRORS Linear rate.
Jim Ray & Jake Griffiths NOAA/National Geodetic Survey STATUS OF IGS ORBIT MODELING & AREAS FOR IMPROVEMENT Earth radiation pressure (albedo) accelerations.
2013 AGU Fall Meeting – 9 December 2013 – San Francisco, CA – Poster #G13B-0933 Status of IGS Core Products J. Griffiths NOAA,
Geodetic Survey Division EARTH SCIENCES SECTOR Slide 1 Real-Time and Near Real-Time GPS Products and Services from Canada Y. Mireault, P. Tétreault, F.
GNSS Observations of Earth Orientation Jim Ray, NOAA/NGS 1. Polar motion observability using GNSS – concepts, complications, & error sources – subdaily.
GNSS Observations of Earth Orientation Jim Ray, NOAA/NGS 1. Polar motion observability using GNSS – concepts, complications, & error sources – subdaily.
Abstract The International Earth Rotation and Reference Systems Service (IERS) has established a Working Group on Prediction to investigate what IERS prediction.
Modern Navigation Thomas Herring MW 11:00-12:30 Room
Chapter 8: The future geodetic reference frames Thomas Herring, Hans-Peter Plag, Jim Ray, Zuheir Altamimi.
Regional and Global Measurements: The Reference Frame for Understanding Observations Geoff Blewitt University of Nevada, Reno, USA Zuheir Altamimi IGN,
Space Geodesy (1/3) Geodesy provides a foundation for all Earth observations Space geodesy is the use of precise measurements between space objects (e.g.,
IGS Analysis Center Workshop, 2-6 June 2008, Florida, USA GPS in the ITRF Combination D. Angermann, H. Drewes, M. Krügel, B. Meisel Deutsches Geodätisches.
The IGS contribution to ITRF2013 – Preliminary results from the IGS repro2 SINEX combinations Paul Rebischung, Bruno Garayt, Xavier Collilieux, Zuheir.
TERRESTRIAL REFERENCE SYSTEMS FOR GLOBAL NAVIGATION SATELLITE SYSTEMS
01/0000 HEO and Daylight Ranging “Reality and Wishes” Ramesh Govind ILRS Fall Workshop, 4 th October 2005.
SNARF: Theory and Practice, and Implications Thomas Herring Department of Earth Atmospheric and Planetary Sciences, MIT
IGS Analysis Center Workshop, 4 June 2008 Recommendations from “RT/NRT user requirements” 1.E-GVAP recommends IGS to support PPP strategy with high quality.
International Workshop on Laser Ranging, October 2008, Poznań (Poland) Quality assessment of the ILRS EOP „Daily” Product G. Bianco Agenzia Spaziale.
PENDING & PROPOSED MODEL CHANGES: SESSION RECOMMENDATIONS IGS core products AC modeling documentation Troposphere modeling Higher-order ionospheric corrections.
Principles of the Global Positioning System Lecture 18 Prof. Thomas Herring Room A;
LLR Analysis – Relativistic Model and Tests of Gravitational Physics James G. Williams Dale H. Boggs Slava G. Turyshev Jet Propulsion Laboratory California.
View on GPS and Galileo ‘From across the Atlantic…’ Ruth E. Neilan International GNSS Service (IGS) Central Bureau Jet Propulsion Laboratory/California.
SHA: the GNSS Analysis Center at SHAO Junping Chen, Bin Wu, Xiaogong Hu Haojun Li, Xiao Pei, Yize Zhang Shanghai Astronomical Observatory (SHAO)
A proposal for a consistent model of air pressure loading as part of the International Terrestrial Reference System (ITRS) Conventions Plag, H.-P. (1),
Kenneth Johnston US Naval Observatory Presented by Jules McNeff International Committee on GNSS Provider’s Forum Bangalore, India 4 September 2007 GPS.
Workshop, Miami, June 2008 IGS Contribution to ITRF Zuheir Altamimi & Xavier Collilieux IGN, France.
Rotational Errors in IGS Orbit & ERP Products Jim Ray, Jake Griffiths NOAA/NGS P. Rebischung IGN/LAREG J. Kouba NRCanada W. Chen Shanghai Astronomical.
NAPEOS: The ESA/ESOC Tool for Space Geodesy
Importance of SLR in the Determination of the ITRF Zuheir Altamimi IGN, France Geoscience Australia, Canberra, August 29, 2005 SLR Strength: its contribution.
IERS Combination WG and CPP Meeting, April 27, 2005, TU of Vienna, Austria Status and Future of the IERS Combination Efforts Markus Rothacher GeoForschungsZentrum.
IERS Combination WG and CPP Meeting, April 27, 2005, TU of Vienna, Austria Strategies for Weekly Routine Generation of Combined IERS Products Markus Rothacher.
IERS Directing Board Meeting No.39, BIPM Paris, September 23, 2004 IERS2005: Plan “Integrated Earth orientation parameters, Radio sources, and Site coordinates.
Recent GNSS activities in Germany for COST
Aurore Sibois and Shailen Desai
Thomas Herring, IERS ACC, MIT
Site survey and co-location
Consistency of Crustal Loading Signals Derived from Models & GPS: Inferences for GPS Positioning Errors Quantify error budget for weekly dNEU GPS positions.
Sub-Daily ERP Investigations
Reference Frame Representations: The ITRF from the user perspective
Unified Analysis Workshop, July 2017, Paris
Space Geodesy Branch Highlights, August 2002 CONT02 VLBI Campaign
Real-Time Working Group
Jet Propulsion Laboratory
Appliance of IceCORS network 2017 by Dalia Prizginiene
Presentation of Public ESA Multi-GNSS Products
IVS contribution to the ITRF2014
Kamil Teke and Johannes Böhm
ESOC IGS Reprocessing T. Springer, F. Dilssner, E. Schoenemann,
X SERBIAN-BULGARIAN ASTRONOMICAL CONFERENCE 30 MAY - 3 JUNE, 2016, BELGRADE, SERBIA EARTH ORIENTATION PARAMETERS AND GRAVITY VARIATIONS DETERMINED FROM.
Proposal for long station names in SINEX format Paul Rebischung Unified Analysis Workshop, Paris, July 2017 Good morning. So I’m going to.
ESOC Combined GNSS Processing
ESOC Combined GNSS Processing
Agenda Background and Motivation
Suggested Guidance for OPUS Projects Processing
Reference Frame Working Group Report
CNES-CLS Dynamical modelling of GPS orbits
Combination of reprocessed orbit, clock and ERP products
Presentation transcript:

WHY DOES THE IGS CARE ABOUT EOPs? Summary of core products of the International GNSS Service (IGS) Ultra-Rapid (real-time), Rapid, & Final series outputs: orbits, polar motion/LOD, clocks, & station positions Ultra-Rapid products very widely used for many demanding real-time applications e.g., very rapid tropo water vapor soundings for meteo models & natural hazards monitoring Ultra-Rapid product quality depends on EOP prediction accuracy latest observed orbits projected into future with EOP predictions EOP prediction errors limit accuracy of IGS real-time orbits Jim Ray IGS Analysis Center Coordinator NOAA/National Geodetic Survey NGA Future EOP Prediction Workshop, Springfield, VA, 17 November 2011

IGS Core Product Series (2011) ID Latency Issue times (UTC) Data spans Remarks Ultra-Rapid (predicted half) IGU real-time @ 03:00, 09:00, 15:00, 21:00 +24 hr @ 00:00, 06:00, 12:00, 18:00 ● for real-time apps ● GPS & GLONASS ● issued with prior IGA (observed half) IGA 3 - 9 hr 03:00, 09:00, 15:00, 21:00 -24 hr @ ● for near real-time apps ● issued with following Rapid IGR 17 - 41 hr 17:00 daily ±12 hr @ 12:00 ● for near-definitive, rapid apps ● GPS only Final IGS 11 - 17 d weekly each Thursday 12:00 for 7 d ● for definitive apps

IGS Ultra-Rapid Update Cycle day 1 day 2 day 3 ● 00h 06h 12h 18h = 24 hr of observations = observed EOPs = 24 hr of predictions = predicted EOPs IGU updates every 6 hr are always 3 hr after the beginning of each prediction interval

IGS Core Product Accuracies (2011) Series ID Product Types Accuracies Output Intervals Ultra-Rapid (predicted half) IGU ● GPS orbits ~ 5 cm (1D) 15 min ● GLONASS orbits ~10 cm (1D) ● GPS SV clocks ~3 ns RMS / ~1.5 ns Sdev ● EOPs: PM + LOD ~250 µas / ~50 µs 6 hr (observed half) IGA ~ 3 cm (1D) ~5 cm (1D) ~150 ps RMS / ~50 ps Sdev <50 µas / ~10 µs Rapid IGR ~2.5 cm (1D) ● GPS SV & station clocks ~75 ps RMS / ~25 ps Sdev 5 min <40 µas / ~10 µs daily Final IGS <2.5 cm (1D) <5 cm (1D) ~75 ps RMS / ~20 ps SDev 30 s (SVs) + 5 min <30 µas / ~10 µs ● Terrestrial frames ~2 mm N&E / ~5 mm U weekly IGS aims for ~1 cm orbit & ~1 mm terrestrial accuracies to satisfy most demanding mm-level user application requirements

Errors in obs EOPs ~ cancel out in forward/reverse transforms Rotational Transform: Observed EOPs(t) Observed orbit: Crust-fixed frame Observed orbit: Inertial frame 1) + Projected orbit: Inertial frame Observed orbit: Inertial frame 2) Rotational Transform: Observed + Predicted EOPs(t) Observed + Projected orbit: Crust-fixed frame 3) Errors in obs EOPs ~ cancel out in forward/reverse transforms but EOP prediction errors fully embedded in crust-fixed orbit predictions typical prediction errors: ~0.4 mas/d for PM; 0.1 ms/d = 1.5 mas/d for UT1 0.1 ms = 1.5 mas = 4.6 cm @ Earth = 19.4 cm @ GPS

Ultra-Rapid AC Orbit Comparisons (over 48 hr) Performance among Analysis Centers has become bimodal SIO & USNO have been excluded for >2 year AC quality is more uniform over first 6 hr of orbit predictions biggest differences occur for 6 – 24 hr orbit predictions

Some IGU AC Orbits Have Large Rotations 0.5 mas = 64 mm error @ GPS hgt SIO & USNO have large Z rotational errors; also Y CODE sometimes also has moderately large Z rotations these AC rotations probably from poor orbit modeling, not EOP predictions

Ultra-Rapid Orbit Diffs (mm) wrt IGR (2009) DX DY DZ RX RY RZ SCL RMS WRMS MEDI TOTAL ERR IGU 6-hr predictions: mean 3.5 -0.6 0.3 0.8 3.1 -0.7 28.9 21.3 15.6 41.7 std dev 4.7 4.9 3.4 13.8 16.3 27.2 2.6 19.7 8.0 IGU 24-hr predictions: 1.1 -0.1 -0.5 -0.9 -1.3 64.7 47.3 30.2 80.2 1.8 2.0 3.8 21.9 31.2 52.0 1.9 33.3 6.0 IGA observations: 1.2 0.1 -0.2 0.9 -1.2 9.0 7.2 1.3 12.7 1.5 1.6 Orbit errors double when prediction interval increases by x4 IGA total err only ~40% worse than IGRs (but 175% worse for RZ)

Ultra-Rapid Orbit Diffs (mm) wrt IGR (2009) DX DY DZ RX RY RZ SCL RMS WRMS MEDI TOTAL ERR IGU 6-hr predictions: mean 3.5 -0.6 0.3 0.8 3.1 -0.7 28.9 21.3 15.6 41.7 std dev 4.7 4.9 3.4 13.8 16.3 27.2 2.6 19.7 8.0 IGU 24-hr predictions: 1.1 -0.1 -0.5 -0.9 -1.3 64.7 47.3 30.2 80.2 1.8 2.0 3.8 21.9 31.2 52.0 1.9 33.3 6.0 IGA observations: 1.2 0.1 -0.2 0.9 -1.2 9.0 7.2 1.3 12.7 1.5 1.6 Z rotation errors are largest RT error – from UT1 prediction errors Largest RT orbit prediction error comes from UT1 predictions IGA accuracy also limited by RZ rotations

Ultra-Rapid Orbit Diffs (mm) wrt IGR (2009) DX DY DZ RX RY RZ SCL RMS WRMS MEDI TOTAL ERR IGU 6-hr predictions: mean 3.5 -0.6 0.3 0.8 3.1 -0.7 28.9 21.3 15.6 41.7 std dev 4.7 4.9 3.4 13.8 16.3 27.2 2.6 19.7 8.0 IGU 24-hr predictions: 1.1 -0.1 -0.5 -0.9 -1.3 64.7 47.3 30.2 80.2 1.8 2.0 3.8 21.9 31.2 52.0 1.9 33.3 6.0 IGA observations: 1.2 0.1 -0.2 0.9 -1.2 9.0 7.2 1.3 12.7 1.5 1.6 due to modelling of orbit dynamics large X, Y rotation errors – from PM prediction errors Next largest RT limits from orbit modelling (solar radiation pressure effects) & PM prediction errors

 Multi-technique EOP combinations mostly sub-optimal !  EOP Error Sources Station-related measurements: thermal noise instrumentation propagation delays multipath, etc σStation ≈ 1/√NStation Geophysical & parameter models: esp near S1, K1, K2 tidal periods AAM/OAM errors Source-related errors: orbit dynamics (GPS, SLR, DORIS) quasar structures (VLBI) σSource ≈ 1/√NSource σEOP = + + Possible improvements: new subdaily EOP tide model ? better handling of parameter constraints ? modern theory of Earth rotation ? more robust SLR, VLBI networks ? more stable site installations ? near asymptotic limit for GPS already new GNSS constellations better GNSS orbit models ? quasar structure models (VLBI) ?  Multi-technique EOP combinations mostly sub-optimal ! 

Conclusions Generally, IGA/IGU near- & real-time orbits & EOPs are of very high quality could use more & better input Analysis Center solutions Rotations are leading real-time orbit error due to UT1 & PM prediction errors used for IGU orbits models for orbit dynamics also add some rotational errors for some ACs EOP services could better use IGU products provide updates at least 4 times daily seek better input AAM + OAM predictions improve combination algorithms present IERS predictions generally not adequate for IGS requirements IGS ACs generate better 1-day PM predictions internally from their own latest measurements; we cannot do that for UT1 though Better model for subdaily tidal EOP variations also needed errors of IERS model alias into GPS orbit parameters