The Chandler Wobble is a geophysical phenomenon constituting a free oscillation of Earth's axis of rotation relative to the solid Earth, characterized by a quasi-periodic motion with a period of approximately 435 days resulting from the planet's non-rigidity and mass distribution asymmetries.
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134
The period and Q of the Chandler wobble
Melvyn Smith, F. A. Dahlen · Geophysical Journal International · 1981 · 308 citations
the excitation of the Chandler wobble
R. S. Gross · Geophysical Research Letters · 2000 · 200 citations
1–5 of 134
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Centre National de la Recherche Scientifique
Paris, France
9 h-index
19 publications
656 citations
Institut de physique du globe de Paris
Paris, France
8 h-index
21 publications
716 citations
Goddard Space Flight Center
Greenbelt, United States
7 h-index
7 publications
366 citations
California Institute of Technology
Pasadena, United States
6 h-index
8 publications
1.1K citations
Binghamton University
Binghamton, United States
6 h-index
7 publications
231 citations
Royal Observatory of Belgium
Brussels, Belgium
6 h-index
15 publications
880 citations
Jet Propulsion Laboratory
Pasadena, United States
6 h-index
9 publications
758 citations
Institute of Geodesy and Geophysics
Wuhan, China
6 h-index
14 publications
424 citations
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GJI · 42 publications · 2.6K citations
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- Journal of Geophysical Research Atmospheres
JGR · 22 publications · 1.5K citations
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- Geophysical Research Letters
9 publications · 423 citations
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- Nature
6 publications · 237 citations
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- Physics of The Earth and Planetary Interiors
4 publications · 173 citations
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