Accuracy of the Determination or Prediction of Earth Orientation Parameters

  • Martine Feissel
Conference paper
Part of the International Association of Geodesy Symposia book series (IAG SYMPOSIA, volume 105)


The Earth orientation can be described as a function of time by a series of five parameters which link coordinates in a terrestrial reference frame to a celestial reference frame. The accuracy of this link is reviewed in the cases of Very Long Baseline radio Interferometry, Lunar Laser Ranging and Satellite Laser Ranging. Examples of the influence of the models used in the definition of the reference frames are given. Possible ways to use the International Earth Rotation Service (IERS) results for tying reference frames are evaluated. The predictability of the Earth Orientation Parameters is studied.


Satellite Laser Range Polar Motion Earth Orientation Parameter Terrestrial Reference Frame Lunar Laser Range 
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  1. Altamimi, Z., Arias, E.F., Boucher, C., Feissel, M. 1989: Earth Orientation Determination: Some tests of consistency. This volume.Google Scholar
  2. Dickey, J.O. 1989: Atmospheric excitation of the Earth’s rotation. This volume.Google Scholar
  3. Feissel, M. 1984: Stability of polar motion time series. Proc. Internat. Symp. on Space Techniques for Geodynamics, Somogyi and Reigber J, Res. Inst, of the Hugarian Acad, of Sci. (Sopron, Hungary), Vol. 1, p. 255.Google Scholar
  4. Galas, R. and Sigl, R. 1989: Prediction of polar motion. This volume.Google Scholar
  5. Gambis, D. 1989: Short and long term universal time prediction from both astronomical and atmospheric angular momentum data. This volume.Google Scholar
  6. Herring, T. 1988: Correction to the IAU Nutation series BIH Annual Report for 1987. p. D-105, Attach. 1..Google Scholar
  7. IERS 1989a: Earth orientation and reference frame determinations, atmospheric excitation functions, up to 1988. IERS Technical Note 2. Observatoire de Paris.Google Scholar
  8. IERS 1989b: Annual Report for 1988. Observatoire de Paris.Google Scholar
  9. Korth, W. and Dietrich, R. 1988: Investigations on the stability of the terrestrial reference frame for the determination of ERP using SLR data. Proc. 6th Symp. “Geodesy and Physics of the Earth”, 21–26 Aug. 1988, Potsdam (DDR).Google Scholar
  10. Lieske, J.H., Lederle, T., Fricke, W, and Morando, B. 1977: Expressions for the Precession Quantities Based upon the IAU (1976) System of Astronomical constants. Astron. Astrophys. 58, 1.Google Scholar
  11. McCarthy D.D. (ed.) 1989: IERS Standards. IERS Technical Note 3. Observatoire de Paris.Google Scholar
  12. Melbourne W.(ed.). 1985: Project MERIT Standards, USNO Circular no 167.Google Scholar
  13. Minster J.B. and Jordan T.H. 1978: Present-day Plate Motion, J. Geophys. Res. 83, 5331.CrossRefGoogle Scholar
  14. NEOS (U.S. National Earth Orientation Service), 1989: Annual Report for 1988.Google Scholar
  15. Rutman, J. 1978: Characterization of Phase and Frequency Instabilities in Precision Frequency Sources: Fifteen Years of Progress. Proceedings of the IEEE, 66,. 1048.Google Scholar
  16. Seidelmann P.K. 1982: IAU Theory of Nutation: The Final Report of the IAU Working Group on Nutation. Celest. Mech. 27, 79.CrossRefGoogle Scholar
  17. Yoder, C.F., Williams, J.G. and Parke, M.E. 1981: Tidal Variations of Earth Rotation, J.Geophys. Res. 86, 881.CrossRefGoogle Scholar

Copyright information

© Springer-Verlag New York Inc. 1990

Authors and Affiliations

  • Martine Feissel
    • 1
  1. 1.Observatoire de ParisCentral Bureau of International Earth Rotation ServiceParisFrance

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