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Kimura's Z-Term and the Liquid Core Theory

Published online by Cambridge University Press:  27 June 2016

Yasujiro Wako*
Affiliation:
International Latitude Observatory of Mizusawa, Iwate, Japan

Abstract

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Kimura (1902) pointed out that there might be an unknown cause other than polar motion which would produce an apparent latitude variation, and introduced the Z-term as, Δϕ = Xcos λ + + Ysin λ + Z.

The theoretical results by Jeffreys-Vicente (1957) and Molodensky (1961) have shown that the effect of a liquid core of the Earth may increase the coefficients of the semi-annual solar nutation term (2 ⊙) which is involved in the diurnal nutation (the so-called Oppolzer term) by 0″.02. It is reasonable to accept this correction which will appear in the Z-term with an argument of (2 ⊙ −α).

From comparison of the observed amplitudes and the phase angles of the annual Z-terms derived from the ILS data, it is concluded that the argument of the principal annual term in Z is (2 ⊙ −α) and not ⊙. The following results were obtained for the annual Z-term for 1955-1966 from the analysis of data by two independent methods (Wako, 1970): 0″.0137 sin (2 ⊙ −α + 2°.2), 0″.0203 sin (2 ⊙ −α + 4°.3).

Melchior (1970) proposed another effect of the Earth's liquid core for the annual nutation in obliquity, thus a term such as a sin (⊙ +α + A) would appear in the Z-term and it might cause a part of semi-annual Z-term. For the determination of these corrections, analysis of Kimura's Z-term is the most effective method.

Type
Research Article
Copyright
Copyright © Reidel 1972 

References

Fedorov, E. P.: 1963, in Nutation and Forced Motion of the Earth's Pole (Pergamon, New York, transl. by Jeffreys, B. S.).Google Scholar
Jeffreys, H. and Vicente, R. O.: 1957a, Monthly Notices Roy. Astron. Soc. 117, 142.Google Scholar
Jeffreys, H. and Vicente, R. O.: 1957b, Monthly Notices Roy. Astron. Soc. 177, 162.CrossRefGoogle Scholar
Kimura, H.: 1902a, Astron. J. 27, 107.CrossRefGoogle Scholar
Kimura, H.: 1902b, Astron. Nachr. 158, 234.Google Scholar
Melchior, P.: 1970, ‘Precession-Nutations and Tidal Potential’, in IAU Colloquium No. 9 (System of Astronomical Constants), Heidelberg.Google Scholar
Melchior, P. and Dejaiffe, R.: 1969, Ann. Obs. Roy. Belgique, 3e Serie, 10, Fasc. 3.Google Scholar
Molodensky, M. S.: 1961, Comm. Obs. Roy. Belgique 188, S., G., 58, 25.Google Scholar
Oppolzer, T. von: 1882, Lehrbuch zur Bahnbestimmung 1, 126.Google Scholar
Thomas, D. V.: 1964, Nature 201, 481.Google Scholar
Vicente, R. O. and Jeffreys, H.: 1964, Nature 204, 120.CrossRefGoogle Scholar
Wako, Y.: 1969a, Acad. Roy. Belg. Bull. Cl. Sci. 5e Serie, 55, 357.Google Scholar
Wako, Y.: 1969b, Publ. Int. Lat. Obs. Mizusawa 7, No. 1, 51.Google Scholar
Wako, Y.: 1970, Publ. Astron. Soc. Japan 22, 525.Google Scholar