Three regimes of mantle convection with non‐Newtonian viscosity and stagnant lid convection on the terrestrial planets
- 1 August 1997
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 24 (15) , 1907-1910
- https://doi.org/10.1029/97gl01682
Abstract
No abstract availableThis publication has 28 references indexed in Scilit:
- Steady tetrahedral and cubic patterns of spherical shell convection with temperature‐dependent viscosityJournal of Geophysical Research, 1996
- Interaction of weak faults and non-newtonian rheology produces plate tectonics in a 3D model of mantle flowNature, 1996
- Stagnant lid convection on VenusJournal of Geophysical Research, 1996
- Magellan and comparative planetologyJournal of Geophysical Research, 1996
- On the thermal evolution of VenusJournal of Geophysical Research, 1994
- High Rayleigh number regime of temperature‐dependent viscosity convection and the Earth's early thermal historyGeophysical Research Letters, 1993
- Effects of strongly temperature‐dependent viscosity on time‐dependent, three‐dimensional models of mantle convectionGeophysical Research Letters, 1993
- Rheology of the Upper Mantle: A SynthesisScience, 1993
- Mantle ConvectionThe Journal of Geology, 1992
- The relationship between plate velocity and trench viscosity in Newtonian and power‐law subduction calculationsGeophysical Research Letters, 1990