This thesis focuses on the long-term rotational stability of the Earth and terrestrial planets. One important class of perturbation is a reorientation of the solid planet with respect to a rotation pole that remains fixed in an inertial frame. These motions are driven by mass redistribution within or on the surface of the planet (e.g. glaciation, mantle convective flow). Long-term changes in the orientation of the rotation pole are called True Polar Wander (TPW). / Earth and Planetary Sciences
Identifer | oai:union.ndltd.org:harvard.edu/oai:dash.harvard.edu:1/12274557 |
Date | 04 June 2016 |
Creators | Chan, Ngai Ham |
Contributors | Mitrovica, Jerry X. |
Publisher | Harvard University |
Source Sets | Harvard University |
Language | en_US |
Detected Language | English |
Type | Thesis or Dissertation |
Rights | open |
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