Comparison between theories of nutation for a rigid-Earth model

Details Comparison between theories of nutation for a rigid-Earth model Comparison between theories of nutation for a rigid-Earth model

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...276..266s&link_type=abstract

Astronomy and Astrophysics, Vol. 276, p. 266 (1993)

Astronomy and Astrophysics

Astrophysics

13

Celestial Mechanics, Earth

Scientific paper

The theory of nutation for a rigid-Earth model serves classically as a basis to the theory of nutation for a more elaborate one (including an elastic mantle. a fluid outer core and a solid inner core). In view of the present level of accuracy of the observations new tables of nutation for a rigid-Earth model including all the coefficients up to 0.01 milliarcsec have been determined by (Zhu & Groten 1989) and (Kinoshita & Souchay 1990). We show in detail the dramatic improvement of these two theories with respect to the theory of Kinoshita (1977) as well as a qualitative and quantitative relative comparison.

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