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Note on the Determination of the Neaely Diurnal Free Nutation (Core Nutation) and the Principal Term of Nutation Based on the Astrometric Data

Published online by Cambridge University Press:  12 April 2016

Ya.S. Yatskiv  and
L.D. Kovbasyuk
Ya.S. Yatskiv
Affiliation:
The Main Astronomical Observatory of the Ukrainian SSR Academy of Sciences Kiev, USSR
L.D. Kovbasyuk
Affiliation:
Department of the All-union Astronomy and Geodesy Society Niznij Novgorod, USSR

Extract

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Due to the highly accurate determination of the corrections to the nutation terms (the IAU-1980 nutation theory) by VLBI observations, the proposal for adoption of the new nutation theory or standard model of nutation is being discussed. At this point there are two unsolved problems:

  1. (a) VLBI observations can’t provide reliable estimates of the principal nutation term. The reason is that the correlation between this term and the precession constant is high due to the insufficient time span of these observations (about 10 years).

  2. (b) period of free core nutation (FCN) which depends on the ellipticity of the mantle-core boundary has not been, so far, reliably determined from direct observations.

In the present paper, we would like to draw attention to the results of the analysis of astrometric latitude and time observations which could be useful for resolving these problems.

Type
Part 2. Poster Papers
Information
International Astronomical Union Colloquium , Volume 127: Reference Systems , 1991 , pp. 385 - 391
Copyright
Copyright © United States Naval Observatory 1991

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