Modelling planetary dynamics by using the temperature at the core–mantle boundary as a control variable: effects of rheological layering on mantle heat transport
- 13 July 1998
- journal article
- Published by Elsevier in Physics of the Earth and Planetary Interiors
- Vol. 108 (3) , 219-234
- https://doi.org/10.1016/s0031-9201(98)00101-0
Abstract
No abstract availableThis publication has 69 references indexed in Scilit:
- A sensitivity study of three‐dimensional spherical mantle convection at 108 Rayleigh number: Effects of depth‐dependent viscosity, heating mode, and an endothermic phase changeJournal of Geophysical Research, 1997
- Phase transitions in the Martian mantle: Implications for partially layered convectionEarth and Planetary Science Letters, 1997
- Thermal expansivity of lower mantle phases MgO and MgSiO3 perovskite at high pressure derived from vibrational spectroscopyPhysics of the Earth and Planetary Interiors, 1996
- High rayleigh number convection at infinite prandtl number with weakly temperature-dependent viscosityGeophysical & Astrophysical Fluid Dynamics, 1996
- Effect of depth-dependent viscosity on the planform of mantle convectionNature, 1996
- Cooling of the Earth, Urey ratios, and the problem of potassium in the coreGeophysical Research Letters, 1993
- Time‐dependent three dimensional compressible convection with depth‐dependent propertiesGeophysical Research Letters, 1992
- Thermal expansivity in the lower mantleGeophysical Research Letters, 1992
- A seismic equation of state II. Shear properties and thermodynamics of the lower mantlePhysics of the Earth and Planetary Interiors, 1987
- Convection with pressure- and temperature-dependent non-Newtonian rheologyGeophysical Journal International, 1984