Journal
EARTH AND PLANETARY SCIENCE LETTERS
Volume 278, Issue 1-2, Pages 50-54Publisher
ELSEVIER
DOI: 10.1016/j.epsl.2008.11.027
Keywords
hot-spots; mantle plumes; plate tectonics; paleomagnetism; multigrid-refinement; multi-resolution
Categories
Funding
- Natural Environmental Research Council (NERC)
- Engineering and Physical Sciences Research Council (EPSRC), through the Environmental Mathematics and Statistics (EMS) [NER/S/E/2004/12725]
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Hot-spots are anomalous regions of magmatism that cannot be directly associated with plate tectonic processes. They are widely-regarded as the surface expression of upwelling mantle plumes. Hot-spots exhibit variable life-spans, magmatic productivity and fixity. This suggests that a wide-range of upwelling structures coexist within Earth's mantle, a view supported by geochemical and seismic evidence, but, thus far, not fully-reproduced by numerical models. Here, results from a new, global, 3-D spherical, mantle convection model are presented, which better reconcile hot-spot observations, the key modification from previous models being increased convective vigor. Model upwellings show broad-ranging dynamics; some drift slowly, while others are more mobile, displaying variable life-spans. intensities and migration velocities. Such behavior is consistent with hot-spot observations, indicating that the mantle must be simulated at the correct vigor and in the appropriate geometry to reproduce Earth-like dynamics. Thermally-driven mantle plumes can explain the principal features of hot-spot volcanism on Earth. (c) 2008 Elsevier B.V. All rights reserved.
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