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1
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0343332099
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note
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The mantle is solid except for some shallow (<100 km depth) regions where small percentages of partial melting may take place.
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-
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2
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0342896957
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note
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21 Pa·s by the movement of vacancies or dislocations through the crystal lattice.
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3
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0003887839
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4
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0343768018
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note
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2 and the cooling rate is ∼100 K per million years.
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0343768014
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note
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-1 for hydrated olivine, the major mantle mineral.
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19
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0000870861
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S. W. Bougher, D. M. Hunten, R. J. Phillips, Eds. Univ. of Arizona Press, Tucson, AZ
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0342896927
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note
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Oceanic plates are made at oceanic spreading centers (mid-ocean ridges) and reenter the mantle at subduction zones less than 200 million years later. Subducted oceanic plates ("slabs") sink through the mantle.
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24
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M. A. Richards, R. Gordon, R. van der Hilst, Eds. (American Geophysical Union, Washington, DC, in press)
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0343332072
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note
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Any 3D solenoidal velocity field can be divided into a poloidal component, associated with divergence in a horizontal plane, and a toroidal component, associated with vertical vorticity. The toroidal component is associated with the strike-slip (shear) component at plate boundaries.
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0342462859
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Incompatible trace elements are present in small concentrations and are not readily incorporated into silicate crystal lattices, and thus tend to enter any melt that forms.
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-
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54
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0343767989
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note
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This depletion is relative to a "primitive" composition, which is the presumed composition of Earth's mantle before the extraction of any continental crust.
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-
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55
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0342462857
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note
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A seismic discontinuity at 660 km depth, which is now understood to result from a phase transition, separates the upper and lower mantles.
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58
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0342462856
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Both a viscosity increase and a deflection of the phase boundary within upwellings and downwellings may temporarily deflect slabs.
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Possible regimes of mixing are chaotic (turbulent), in which stretching of heterogeneities increases exponentially with time, and laminar, in which stretching increases linearly with time. Steady-state flows without toroidal motion exhibit only laminar mixing.
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I thank J. Vidale for suggesting Fig. 2B, and two anonymous reviewers for helpful advice. Supported by NASA and the David and Lucile Packard Foundation.
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