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Solution of Earth orientation parameters in 20th century based on optical astrometry and new catalog EOC-3

Published online by Cambridge University Press:  01 October 2007

J. Vondrák
Affiliation:
Astronomical Institute, Boční II, CZ-14131, Prague, Czech Republic email: vondrak@ig.cas.cz
C. Ron
Affiliation:
Astronomical Institute, Boční II, CZ-14131, Prague, Czech Republic email: vondrak@ig.cas.cz
V. Štefka
Affiliation:
Astronomical Institute, Boční II, CZ-14131, Prague, Czech Republic email: vondrak@ig.cas.cz
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Abstract

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A new star catalog has been derived recently, which is based on combination of Hipparcos/Tycho Catalogues with long lasting ground-based astrometric observations. In addition to ‘classical’ mean positions and proper motions of the stars, it contains also information on periodic motions of many stars that are due to double or multiple stellar systems. The catalog, called EOC-3, contains 4418 different objects, out of which 585 have significant periodic motions. This improved catalog is used as a reference frame in optical wavelength to derive a new series of Earth Orientation Parameters. To this end, almost five million observations of latitude/universal time variations made at 33 observatories are used. The new EOP series covers almost the entire 20th century (namely the interval 1899.7-1992.0).

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2008

References

Capitaine, N., Wallace, P. T., & Chapront, J. 2003, A&A, 412, 567Google Scholar
Høg, E., Fabricius, C., Makarov, V. V. et al. 2000, A&A, 355, L27Google Scholar
Mathews, P. M., Herring, T. A., & Buffet, B. A. 2002, J. Geophys. Res., 107 (B4), doi: 10.1029/2001JB000390.CrossRefGoogle Scholar
Ron, C., Capitaine, N., & Vondrák, J. 2005, in: Capitaine, N. (ed.) Journées 2004 Systèmes de référence spatio-temporels, (Observatoire de Paris), p. 110Google Scholar
Vondrák, J. 2004, Serb. Astron. J. 168, 1CrossRefGoogle Scholar
Vondrák, J. & Štefka, V. 2007, A&A, 463, 783Google Scholar
Vondrák, J., Pešek, I., Ron, C., & Čepek, A. 1998, Publ. Astron. Inst. Acad. Sci. Czech R. 87Google Scholar
Vondrák, J., Ron, C., & Pešek, I. 2000, in: Dick, S., McCarthy, D. D., & Luzum, B. (eds.), Polar motion: Historical and Scientific Problems, Proc. IAU Coll. 178, ASP Conf. Series 208, p. 206CrossRefGoogle Scholar
Wielen, R., Schwan, H., Dettbarn, C. et al. 2001, Veröff. Astron. Rechen-Inst. Heidelberg, 40, Kommissions-Verlag G. Braun, Karlsruhe.Google Scholar
Yoder, C. F., Williams, J. G., & Parke, M. E. 1981, J. Geophys. Res. 86, 881CrossRefGoogle Scholar