Hostname: page-component-5c6d5d7d68-lvtdw Total loading time: 0 Render date: 2024-08-18T17:01:32.722Z Has data issue: false hasContentIssue false

Is the Chandler Period Stable?

Published online by Cambridge University Press:  07 August 2017

Gao Buxi*
Affiliation:
Institute of Geodesy and Geophysics Chinese Academia Sinica Wuhan, 430077, P. R. China

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 problem on Chandler period is an unsolved one. Several authors suggested a hypothesis that the Chandler wobble is only one free period which slightly changes in time and is amplitude-dependent. In this paper we shall make the hypothesis more rigorous than that has been carried yet. A new deconvolution method for Fourier transform is suggested. Using this method the polar motion data are analysed. The analysis results are shown; the Chandler period is not stable and is indeed amplitude-dependent. The probable explanation for the amplitude-dependent of Chandler period is that, which might be caused by non-equilibrium response of the ocean.

Type
Impact on Geodynamics
Copyright
Copyright © Kluwer 

References

1. Carter, W.E. (1981) ‘Frequency modulation of the Chandlerian componentof polar motion’, Geophys. Res. 86, B3, 1653.CrossRefGoogle Scholar
2. Chao, B.F. (1983) ‘Autoregressive harmonic analysis of the Earth's polar motion using homogeneous International Latitude Service data’, J.G.R., Vol. 88, 1029910307.Google Scholar
3. Colombo, G. & Shapiro, I.I. (1968) ‘Theoretical model for the Chandler wobble’, Nature, 217, 156.CrossRefGoogle Scholar
4. Dickman, S.R. (1979) ‘Consequences of an enhanced pole tide’, Geophys. Res. 84, B10, 54415456.CrossRefGoogle Scholar
5. Gao, B. (1990) ‘Variations of the Chandler wobble and the annual polar motion from 1965.0 to 1985.0’, ACTA Astrnomica Sinica, Vol. 31, No. 3.Google Scholar
6. Lambeck, K. (1980) The Earth's Variable Rotation, Geophysical causes and consequences, Combridge University Press.CrossRefGoogle Scholar
7. Melchior, P. (1957) in Ahrens, L.H. et al(eds), Latitude Variation, Pergamon, New Youk, 212.Google Scholar
8. Munk, W.H. & MacDonald, G. (1960) The Rotation of the Earth, Cambridge University Press.Google Scholar
9. Naito, I. (1977) ‘Secular variation of pole tide’, J. Phys. Earth, 25, 221231.CrossRefGoogle Scholar
10. Okobo, S. (1982) ‘Is the Chandler period variable?’, Geophys. J.R. astr. Soc. 71, 629646.Google Scholar
11. Smith, M.L. & Dahlen, F.A. (1981) ‘The period and Q of the Chandler wobble’, Geophys. J.R. astr. Soc. 64, 223281.Google Scholar
12. Vandrak, J. (1989) Report No.402, Department of Geodetic Science and Sorveying, The Ohio State University, Columbus.Google Scholar
13. Wilson, C.R. & Vincente, R.O. (1981) ‘Estimates of Chandler's component of polar motion as derived from various data sets’, Astron. Nachr. 302, 227.CrossRefGoogle Scholar