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This study explores the mechanisms behind superplumes and their unique behavior with depth, including the implications for mineralogy and geochemistry. The findings shed light on the complex nature of mantle convection and provide insights into the Earth's interior processes.
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How to Stabilize Superplumes Eh Tan, Mike Gurnis Caltech Colorado Mantle Convection Workshop, 2005
Modes of Mantle Convection Tackley 2000
African superplume Ni et al. 2002 dVs = -3% dVp = -0.5% sharp, steep side 1000 km above CMB 1000 km wide in mid-mantle
Dynamic Interpretation 1 Davaille et al., 1999
Dynamic Interpretation 2 McNamara & Zhong, 2004
Superplumes Explained? Not actually… • Lower layer is a lot hotter, but also more viscous • Probably OK, the layer might be made of weird material • Constant thermal expansion coefficient • We know thermal expansion decreases ~5x with depth • Can we make a superplume with depth-dependent thermal expansion?
Dynamic Interpretation 3 Ni et al. 2002
Numerical Model • 2D Cartesian ConMan • Modified for Truncated Anelastic Liquid Approximation • Chemical field is modeled by marker chain method • Different materials can have different Ks and r
Implication on Mineralogy • Lee et al. (AGU Spring Meeting, 2005) showed that pyroxenite under high pressure is 2% denser and has 5% higher Ks than PREM value. • How to get pyroxenite in the lower mantle? • subducted metasomatized oceanic crust, according to some petrologist
Conclusions • Metastable superplumes are slightly denser and have higher bulk modulus • The physical and chemical properties of oceanic crust satisfy seismological, geodynamical, mineralogical and geochemical observations.