Hostname: page-component-cc8bf7c57-5wl6q Total loading time: 0 Render date: 2024-12-12T02:00:41.507Z Has data issue: false hasContentIssue false

Earth Rotation in the Hipparcos Reference Frame

Published online by Cambridge University Press:  12 April 2016

J. Vondrák
Affiliation:
Astronomical Institute, Czech Academy of Sciences Praha, Czech Republic
C. Ron
Affiliation:
Astronomical Institute, Czech Academy of Sciences Praha, Czech Republic
I. Pešek
Affiliation:
Astronomical Observatory, Czech Technical University Praha, Czech Republic

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

New determination of the Earth orientation parameters (EOP), based on optical astrometry observations since the beginning of the century, is now under preparation by the Working group established by Commission 19 of the IAU. The Hipparcos catalog is to define the celestial reference frame in which the new series of EOP are to be described. The novelties of the prepared solution are the higher resolution (5 days) and more parameters estimated from the solution (celestial pole offsets, rheological parameters of the Earth, certain instrumental constants). The mathematical model of the solution is described, and the results based on the observations made with 46 instruments at 29 observatories and a preliminary Hipparcos catalog are presented.

Type
Dynamics and Astrometry: Present and Future
Copyright
Copyright © Kluwer 1997

References

Argus, D.F. and Gordon, R.G.: 1991, “No-net-rotation model of current plate velocities incorporating plate motion model NUVEL-1”, Geophys. Res. Lett. 18, 20392042.CrossRefGoogle Scholar
Bizouard, Ch., Capitaine, N., Ron, C., and Vondrák, J.: 1996, “Principal term of nutation from the combination of VLBI observations and optical astrometry”, this volume.Google Scholar
Čepek, A.: 1994, “On solving normal equations of Earth orientation parameters”, Acta Polytechnica 34, 59.Google Scholar
Feissel, M.: 1986, private communication.Google Scholar
Kovalevsky, J.: 1996, private communication.Google Scholar
Lindegren, L. and Kovalevsky, J.: 1995, “Linking the Hipparcos Catalogue to the extra-galactic reference system”, Astron. Astrophys. 304, 189201.Google Scholar
Ma, C.: 1995, private communication.Google Scholar
McCarthy, D.D.: 1970, “Reduction method and star positions for Washington and Richmond Photographic Zenith Tube”, Master thesis, University of Virginia.Google Scholar
McCarthy, D.D.: 1992, “IERS Standards (1992)”, IERS Tech. Note 13, Obs. de Paris.Google Scholar
Pešek, I.: 1995, “Systematic deformations of the apparent almucantar in homogeniza-tion astrolabe data for new solution of Earth orientation parameters from optical astrometry”, Acta Polytechnica 35, 517.Google Scholar
Pešek, I., Vondrák, J., Chollet, F., and Noël, F.: 1993, “Systematic deformations of the apparent almucantar as derived from Danjon astrolabes in Paris and Santiago de Chile”, Astron. Astrophys. 274, 621626.Google Scholar
Scherneck, H.-G.: 1995, private communication.Google Scholar
Turon, C. and Morin, D.: 1995, private communication.Google Scholar
Turon, C. and Morin, D.: 1996, private communication.Google Scholar
Vondrák, J.: 1991, “Calculation of the new series of the Earth orientation parameters in the Hipparcos reference frame”, Bull. Astron. Inst. Czechosl. 42, 283294.Google Scholar
Vondrák, J. and Ron, C.: 1994, “Polar motion and nutation from astrometrie observations after 1900”, in: Dynamics and Astrometry of Natural and Artificial Celestial Bodies (K.Kurzyńska, F.Barlier, ,Seidelmann, P.K., Wytrzyszczak, I., eds), Astronomical Observatory, Poznań, 3944.Google Scholar
Vondrák, J., Feissel, M., and Essaïfi, N.: 1992, “Expected accuracy of the 1900-1990 Earth orientation parameters in the Hipparcos reference frame”, Astron. Astrophys. 262, 329340.Google Scholar
Vondrák, J., Ron, C., and Čepek, A.: 1993, “New solution of polar motion and celestial pole offsets 1900-1978 from ILS observations”, Wiss. Z. TU Dresden 42, 7477.Google Scholar
Vondrák, J., Ron, C., and Čepek, A.: 1994, “Determination of polar motion, celestial pole offsets and universal time by optical astrometry since the beginning of the century”, in: Systèmes de Référence Spatio-temporels, Journées 1994 (Capitaine, N., ed.), Paris, 128133.Google Scholar
Vondrák, J., Ron, C., Pešek, I., and Čepek, A.: 1995, “New global solution of Earth orientation parameters from optical astrometry in 1900-1990”, Astron. Astrophys. 297, 899906.Google Scholar
Vondrák, J., Ron, C., and Pešek, I.: 1996, “Using the Earth orientation parameters to link the Hipparcos and VLBI reference frames”, Astron. Astrophys., in press.Google Scholar
Yoder, F., Williams, J.G., and Parke, M.E.: 1981, “Tidal variations of Earth rotation”, J. Geophys. Res. 86, 881891.Google Scholar