Hostname: page-component-78c5997874-s2hrs Total loading time: 0 Render date: 2024-11-18T08:45:04.820Z Has data issue: false hasContentIssue false
  • English
  • Français

On the Establishment of Terrestrial Coordinate System by Classical Techniques

Published online by Cambridge University Press:  12 April 2016

Ya. S. Yatskiv
Ya. S. Yatskiv*
Affiliation:
Main Astronomical Observatory, Ukrainian Academy of Sciences, Kiev, U.S.S.R.

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.

The definition and practical realization of the astronomical system of terrestrial coordinates are discussed. In particular, the separation of secular polar motion and nonpolar drift of observatories are touched upon as far as those phenomena are crucially intertwined with the realization of a terrestrial coordinate system.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 56: Reference Coordinate Systems for Earth Dynamics , August 1980 , pp. 155 - 164
Copyright
Copyright © Reidel 1981

References

Belotserkovskij, D.Yu. and Kaufman, M.B.,: 1979, in McCarthy, D.D. and Pilkington, J.D.H. (eds.) “IAU Symposium No. 82, Time and the Earth’s Rotation”, D. Reidel, Dordrecht, pp. 23–27 Google Scholar
Fedorov, E.P., Korsuń, A.A., Major, S.P., Panchenko, N.I., Taradij, W.K., Yatskiv, Ya.S.: 1972, “Motion of the Earth’s Pole for the Years 1890.0–1969.0, Naukova Dumka, Kiev.Google Scholar
Fedorov, E.P.: 1975a, Astrometrija i Astrofizika, Kiev, No. 27, pp. 3–13.Google Scholar
Fedorov, E.P.: 1975b, in Kolaczek, B. and Weiffenbach, G. (eds.), “IAU Colloquium No. 26, On Reference Coordinate Systems for Earth Dynamics”, Warsaw, pp. 63–77.Google Scholar
Fedorov, E.P.: 1979, in McCarthy, D.D. and Pilkington, J.D.H. (eds.) “IAU Symposium No. 82, Time and the Earth’s Rotation”, Reidel, D., Dordrecht, pp. 89–101.Google Scholar
Gubanov, V.S. and Yaguidin, L.I.: 1979, in McCarthy, D.D. and Pilkington, J.D.H. (eds.), “IAU Symposium No. 82, Time and the Earth’s Rotation”, D. Reidel, Dordrecht, pp. 47–51.Google Scholar
Guinot, B.: 1979, in McCarthy, D.D. and Pilkington, J.D.H. (eds.), “IAU Symposium No. 82, Time and the Earth’s Rotation”, D. Reidel, Dordrecht, pp. 7–18.Google Scholar
Kolaczek, B.: 1979, in McCarthy, D.D. and Pilkington, J.D.H. (eds.), “IAU Symposium No. 82, Time and the Earth’s Rotation”, D. Reidel, Dordrecht, pp. 125–128.Google Scholar
Korsuń, A.A. and Emetz, A.I.: 1980, in Proceedings of the 4th International Symposium, “Geodesy and Physics of the Earth”, Karl-Marx-Stadt (in press).Google Scholar
Mandelbrot, B.B. and McCamy, K.: 1970, “On the Secular Polar Motion and the Chandler Wobble”, Geophys. J. R. Astr. Soc., 21, pp. 217–2 32.CrossRefGoogle Scholar
Markovitz, N.: 1970, in Mansihna, L., Smylie, D.E., Beck, A.E. (eds.), “Earthquake Displacement Fields and the Rotation of the Earth”, Springer-Verlag, New York, pp. 69–81.Google Scholar
Mironov, N.T.: 1973, Astron. Circular, No. 769, pp. 7–8.Google Scholar
Orlov, A.Ya.: 1941, Bull. Sternberg Institut, Moskva, No. 8.Google Scholar
Seidelmann, P.K. et al.: 1979, Final Report of the IAU Working Group on Nutation, 17th General Assembly of the IAU, Montreal.Google Scholar
Yatskiv, Ya.S., Korsuń, A.A., Mironov, N.T.: 1979, in McCarthy, D.D. and Pilkington, J.D.H. (eds.), “IAU Symposium No. 82, Time and the Earth’s Rotation”, D. Reidel, Dordrecht, pp. 29–39.Google Scholar