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On Precession and Nutation Values

Published online by Cambridge University Press:  12 April 2016

R.O. Vicente*
Affiliation:
Dept. of Applied Mathematics Faculty of Sciences 1294 LisbonPortugal

Abstract

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The results of research on the Earth’s theory of rotation are presented, comparing observed and theoretical values specially for the luni-solar precession and nutation. Investigations of geodynamics show the strong dependence of the nutation values on the adopted model for the structure of the Earth, while the values referring to the precession are not affected as much. The new observational techniques are able to determine some of these values with greater precision than the classical optical techniques, but it is essential that the observations should be done in a systematic and regular way for several decades.

Type
Part 2. Poster Papers
Copyright
Copyright © United States Naval Observatory 1991

References

Bullen, K.E.: 1963, Introductions to the Theory of Seismology, C.U.P. Google Scholar
Charlot, P., Sovers, O.J., Williams, J.G., Newhall, X.X.: 1991, This proceedingGoogle Scholar
Déhant, V.: 1988 in “Earth Rotation and Reference Frames for Geodesy and Geodynamics. eds. Babcock, A. and Wilkins, G. A., Reidel, 323.Google Scholar
Déhant, V.: 1990, Geophvs. J. Int. 100, 477.Google Scholar
DziewoNski, A. M., Anderson, D.L.: 1981 Phys. Earth Planet. Int. 25, 27.Google Scholar
Fedorov, E.P.: 1958 Nutation and the Forced Motion of the Earth’s Pole, Acad. Sci. Ukraine, Kiev (translated by Jeffreys, B., 1961, Pergamon Press).Google Scholar
Fricke, W.: 1967, Astron. J. 72, 1368.CrossRefGoogle Scholar
Fricke, W.: 1971, Astron, and Astrophys. 13, 298.Google Scholar
Fricke, W.: 1982, Astron, and Astrophvs. 107, 113.Google Scholar
Herring, T.A., Gwinn, C.R., Shapiro, I.I.: 1986 J. Geophys. Res 91, 4745.Google Scholar
Herring, T.A.: 1988 Annual Report B I H for 1987, p. D106.Google Scholar
Hill, G.W.: 1893, Astr. J. 13, 1.Google Scholar
Hough, S.S.: 1895, Phil. Trans. A, 186, 469.Google Scholar
Jackson, J.: 1930, Month. Not. R. A. S. 90, 733.Google Scholar
Jeffreys, H.: 1949, Month. Not. R. A. S. 109, 670.CrossRefGoogle Scholar
Jeffreys, H.: 1950, Month. Not. R. A. S. 110, 460.Google Scholar
Jeffreys, H., Vicente, R.O.: 1957, Month. Not. R. A. S. 117, 142.Google Scholar
Kinoshita, H.: 1977, Cel. Mech. 15, 277.Google Scholar
Kinoshita, H., Souchay, J.: 1990, Cel. Mech. (to be published).Google Scholar
Lieske, J.H., Lederle, T., Fricke, W., Morando, B.: 1977 Astron. Astrophys. 58, p. 1.Google Scholar
McCarthy, D. D., Luzum, B.J.: 1991 Astron. J. (to be published).Google Scholar
Morgan, H.R.: 1943, Astr. J. 50, 125.CrossRefGoogle Scholar
Newcomb, S.: 1892, Month. Not. R. A. S., 52, 336.Google Scholar
Newcomb, S.: 1895, Astronomical Constants, Washington, Gov. Printing Office.Google Scholar
Poincaré, H.: 1910, Bull. Astronomique. 27, 321.Google Scholar
Seidelmann, P.K.: 1982, Cel. Mech., 27, 79.Google Scholar
Spencer Jones, H.: 1939, Month. Not. R. A. S., 99, 211.Google Scholar
Vicente, R.O.: 1964, Vistas in Astronomy, 5, p. 1.Google Scholar
Wahr, J.M.: 1981, Geophys. J., 64, 705.Google Scholar
Wahr, J.M., Bergen, Z.: 1986, Geophys. J., 87, 633.Google Scholar
Walter, H.G.: 1991, This proceeding.Google Scholar
Woolard, E.W.: 1953, Astr. Pap. Amer. Ephem. Wash., 15, Part 1.Google Scholar
Zhu, S.Y., Groten, E., Reigber, Ch.: 1990, Astron. J., 99, 1024.Google Scholar