Journal
GEOPHYSICAL RESEARCH LETTERS
Volume 36, Issue -, Pages -Publisher
AMER GEOPHYSICAL UNION
DOI: 10.1029/2009GL037706
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Funding
- NSF [0711542]
- COMPRES
- Division of Geological and Planetary Sciences, California Institute of Technology [10017]
- Division Of Earth Sciences
- Directorate For Geosciences [855815, 0711542] Funding Source: National Science Foundation
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Using a numerical model we explore the consequences of the intrinsic density change (Delta rho/rho approximate to 2-4%) caused by the Fe2+ spin transition in ferropericlase on the style and vigor of mantle convection. The effective Clapeyron slope of the transition from high to low spin is strongly positive in pressure-temperature space and broadens with high temperature. This introduces a net spin-state driving density difference for both upwellings and downwellings. In 2-D cylindrical geometry spin-buoyancy dominantly enhances the positive thermal buoyancy of plumes. Although the additional buoyancy does not fundamentally alter large-scale dynamics, the Nusselt number increases by 5-10%, and vertical velocities by 10-40% in the lower mantle. Advective heat transport is more effective and temperatures in the core-mantle boundary region are reduced by up to 12%. Our findings are relevant to the stability of lowermost mantle structures. Citation: Bower, D. J., M. Gurnis, J. M. Jackson, and W. Sturhahn (2009), Enhanced convection and fast plumes in the lower mantle induced by the spin transition in ferropericlase, Geophys. Res. Lett., 36, L10306, doi: 10.1029/2009GL037706.
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