By Jones C.A.
ISBN-10: 0203207610
ISBN-13: 9780203207611
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Extra resources for Earth's Core and Lower Mantle
Example text
Int. 142, 631–642, figures 1 and 9. ) The relationship between magnetic field, fluid velocity, and boundary heating patterns from a steady state numerical dynamo model by Sarson et al. (1997) is shown in Figure 7. 5-dimensional numerical dynamo model. Here, the fluid upwelling and boundary heat flow are nearly anticorrelated. There is a slight westward phase shift of the downwellings relative to the high boundary Thermal interaction of the core and mantle 19 Figure 6 Steady state numerical solution of thermal convection in a rotating spherical shell including heterogeneous heat flow at the outer boundary, at buoyancy number B=RaE=1, Ekman number E=10−3.
Buffett) pp. 167–182, AGU (1997). Gubbins, D. , “Morphology of the geomagnetic field and implications for the geodynamo,” Nature 325, 509–511 (1987). Gubbins, D. ” Geophys. Res. Lett. 13, 1521–1524 (1986). , Fichtl, G. , “Laboratory experiments on planetary and stellar convection performed on Spacelab 3,” Science 234, 61–64 (1986). Hide, R. “On the earth’s core-mantle interface,” Q. J. R. Met. Soc. 96, 579–590 (1970). , “The nature of Earth’s core,” Annu. Rev. Earth Planet. Sci. 18, 357–386 (1990).
Instituto Nazionale de Geofisica, Rome (1996). Zhang, K. , “On convection in the earth’s core driven by lateral temperature variations in the lower mantle,” Geophys. J. Int. 108, 247–255 (1992). Zhang, K. , “Convection in a rotating spherical fluid shell with an inhomogeneous temperature boundary condition at infinite Prandtl number,” J. Fluid Mech. 250, 209–232 (1993). Zhang, K. , “Convection in a rotating spherical shell with an inhomogeneous temperature boundary condition at finite Prandtl number,” Phys.
Earth's Core and Lower Mantle by Jones C.A.
by Joseph
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