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International Laser Ranging Service

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... Institute of Applied Astronomy, Russia JAXA, Japan Aerospace Exploration Agency JPL ... U. of Texas DUT, Delft University of Technology, The Netherlands ESA ... – PowerPoint PPT presentation

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Title: International Laser Ranging Service


1
International Laser Ranging Service
  • GGOS Meeting
  • GFZ
  • Potsdam Germany
  • March 1 and 2, 2005

2
ILRS Organization
3
(No Transcript)
4
Data Applications
  • Earth orientation parameters (polar motion and
    LOD)
  • 3-D coordinates and velocities of the ILRS
    tracking stations
  • Time-varying geocenter coordinates
  • Static and time-varying coefficients of the
    Earth's gravity field
  • Precision Orbit Determination
  • Fundamental physical constants
  • Lunar ephemerides and librations
  • Lunar orientation parameters

5
ILRS Analysis and Associate Analysis Centers
  • ILRS SLR Official Combination Centers
  • Prime ASI/CGS, Italian Space Agency/Space
    Geodesy Center, Italy
  • Alternate DGFI, Deutsches Geodaetisches
    ForschungsInstitut, Germany
  • Active Contributors to the SLR Combination
    Products
  • ASI/CGS, Italian Space Agency/Space Geodesy
    Center "G. Colombo", Italy
  • DGFI, Deutsches Geodaetisches ForschungsInstitut,
    Germany
  • BKG, Bundesamt fuer Kartographi und Geodaesie,
    Germany
  • GFZ, GeoForschungsZentrum, Germany
  • JCET, Joint Center for Earth Systems Technology,
    USA
  • NSGF, NERC Space Geodesy Facility, UK
  • Lunar Analysis Centers
  • FFI, Forsvarets ForskningsInstitut, Norway
  • JPL, Jet Propulsion Laboratory, USA (SLR and
    Lunar)
  • OCA, Observatoire de la Cote d'Azure, France
    (Lunar)
  • POLAC, Paris Observatory Lunar Analysis Center,
    France (Lunar)
  • University of Texas, Lunar Analysis Center
    (Lunar)

6
Other SLR Analysis and Associate Analysis
Centers
  • AIUB, Astronomical Institute of Berne,
    Switzerland
  • CSR, Center for Space Research, U. of Texas
  • DUT, Delft University of Technology, The
    Netherlands
  • ESA/ESOC, European Space Agency/ESA Space
    Operations Center, Germany
  • GAOUA, Main Astronomical Obser., National Academy
    of Sciences, Ukraine
  • Geoscience Australia
  • IAA, Institute of Applied Astronomy, Russia
  • JAXA, Japan Aerospace Exploration Agency
  • JPL, Jet Propulsion Laboratory, USA
  • MCC, Mission Control Center, Russia
  • Newcastle University, UK
  • NICT, National Institute of Information and
    Communications Technology, Japan

7
ILRS Customers
  • IERS
  • Supported Missions (POD)
  • ILRS Analysis Centers
  • Academic Research Centers
  • National Agencies and Laboratories
  • Commercial Organizations

8
Current ILRS Missions Support
Gravity Probe-B Relativity ICESat Global
Topography (Ice, Oceans, and Land) GRACE-A/B
Static and Time Varying Gravity Field CHAMP
Gravity and Magnetic Field GFO-1 Ocean
Topography Envisat Ocean Topography,
Atmosphere ERS-2 Ocean Topography,
Atmosphere Jason Ocean Topography TOPEX/Posei
don Ocean Topography Larets
Technology, Gravity Field Starlette, Stella
Static and Time Varying Gravity Field, Tides
Meteor-3M Technology, SAGE Ajisai
Gravity Field LAGEOS- 1, 2 Ref. Frame,
Positioning, Static and T/V Gravity Beacon-C
Static and Time Varying Gravity Field
Etalon-1, 2 Positioning, EOP GLONASS-84,
87, 89 Orbit calibration and validation
GPS-35, 36 Orbit calibration and validation
Lunar Reflectors Apollo15, Apollo 11, Apollo
14, Luna 21, Luna 17 Key Passive
Satellites Active satellites with SLR
tracking only
9
Upcoming Missions
Mission Application Launch CRYOSat Ice
budget July 2005 Galileo (2) Orbit
calibration and validation October
2005 ALOS Environmental remote sensing Late
2005 GOCE Gravity Field, Geoid, Ocean Surface
2006
10
ILRS Station Operations
  • Location of Stations
  • Most stations are located close to participating
    agencies
  • Some are located to enhance global distribution
    (South Africa, Tahiti, Arequipa)
  • Voids in global distribution
  • Satellite Priorities
  • Priorities decrease with increasing orbital
    altitude and then increasing orbital inclination
  • Priorities may be increased to intensify support
    for active missions (such as altimetry), special
    campaigns, and post-launch intensive tracking
  • Priorities are reviewed and approved by the
    Governing Board
  • See http//ilrs.gsfc.nasa.gov/satellite_missions/p
    riorities/index.html
  • Scheduling, Coordination and Delivery of
    Observations
  • Stations tracking schedules range from 1 to 4
    shifts per week
  • Stations track according to priorities,
    predictions and their local capabilities
  • The Governing Board approves special campaigns
  • Special procedures (e.g. for vulnerable
    satellites) are approved by the Governing Board
    and managed by the Central Bureau
  • Data is delivered in 1 -2 hours from acquisition

11
Laser Ranging Data and Data Products
  • Satellite Laser Ranging
  • Data series spanning 3 decades at
    ftp//cddis.gsfc.nasa.gov/pub/slr/data)
  • Operational Satellite Ephemerides/predictions at
    ftp//cddis.gsfc.nasa.gov/pub/slr/predicts)
  • ILRS Station and EOP Combination Product (SINEX
    format)
  • Station Coordinates 3 mm 2 mm/year
  • EOP 0.2 milliarcsec LOD 60 microsec.
  • Analysis Center contributions
  • Station Coordinates
  • Earth Origin
  • Temporal and static gravity field (long
    wavelength)
  • LAGEOS Orbits (10 mm/weekly)
  • Position and EOP contributions available at
    ftp//cddis.gsfc.nasa.gov/pub/slr/products
  • Lunar Laser Ranging
  • Lunar Ephemerides 5 - 10 cm
  • Lunar Libration .01 arcsec.
  • Products available at http//ssd.jpl.nasa.gov/hori
    zons.html
  • Measurement and product standards?
  • Station Qualification Criteria ( data quantity,
    data quality, operational compliance)
  • See http//ilrs.gsfc.nasa.gov/stations/site_info/
    global_report_cards/

12
ILRS Future Activities
  • Upgrades for improved performance (short term,
    long term)
  • kilohertz ranging
  • autonomous operation (24/7)
  • improved event timers
  • two-color ranging (refraction)
  • better control systems for more efficient
    satellite pass interleaving
  • more compact retroreflector arrays
  • continuous data flow
  • transponder operations (LLR and planetary
    ranging)
  • broader applications (communications)
  • Improved modeling (S/C center of mass,
    propagation, etc.)
  • New Missions that will improve measurement
    quality
  • Additional passive, high mass density satellites
    in new orbits
  • Key Issues
  • Deterioration of the network
  • Non-performing stations
  • Global distribution
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