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Regional atmospheric influence on the Chandler wobble
International audienceFrom the maps of regional contribution to atmospheric angular momentum (AAM) over the period 1948-2011 (NCEP/NCAR reanalysis data) time domain excitation in Chandler frequency band was extracted by Panteleev's filtering method. This
Christian Bizouard
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Inversion of polar motion data: Chandler wobble, phase jumps, and geomagnetic jerks
International audienceWe reconsider the analysis of the polar motion with a method totally different from the wavelet analysis used in previous papers.
Dominique Gibert, Jean-Louis Le Mouël
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Sensitivity of the Chandler Wobble Period of Mars to the Parameters of the Rheological Model
Doklady Earth SciencesT V Gudkova, Gudkova T V
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On the period and quality factor of the Chandler wobble
Izvestiya, Physics of the Solid Earth, 2008The motion of the Earth’s geophysical pole is modeled by numerical integration of the Liouville equations. The dependence of variable parameters of these equations (the period of free nutation T and the quality factor of the shell Q) is examined as a function of time and initial data sets used for constructing geophysical perturbing functions.
E. A. Spiridonov, I. Ya. Tsurkis
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Selection of Models of the Internal Structure of Mars According to the Chandler Period
2024 17th International Conference on Management of Large-Scale System Development (MLSD)Tamara Gudkova
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Influence of Mantle Inelasticity on the Model Value of the Chandler Wobble Period of Mars
Solar System ResearchT V Gudkova, Gudkova T V
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Quasi‐periodic wind signal as a possible excitation of Chandler wobble
Journal of Geophysical Research: Solid Earth, 1996The atmospheric contribution to the excitation of the Chandler wobble (CW) is studied for a period of about 11 years period beginning in September 1983, using the wobble data set (SPACE93). Two atmospheric angular momentum (AAM) functions are employed; one is based on Japan Meteorological Agency (JMA) data, and the other is based on U.S.
Masato Furuya, Yozo Hamano, Isao Naito
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