Evolution of the mode of convection within terrestrial planets
- 25 July 2000
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 105 (E7), 17563-17578
- https://doi.org/10.1029/2000je001240
Abstract
No abstract availableKeywords
This publication has 44 references indexed in Scilit:
- Influence of early plate tectonics on the thermal evolution and magnetic field of MarsJournal of Geophysical Research, 2000
- Formation age of Earth from 129I/127I and 244Pu/238U systematics and the missing XeJournal of Geophysical Research: Solid Earth, 1999
- Heat transport efficiency for stagnant lid convection with dislocation viscosity: Application to Mars and VenusJournal of Geophysical Research, 1998
- The nature of oceanic lower crust and shallow mantle emplaced at low spreading ratesTectonophysics, 1997
- Three regimes of mantle convection with non‐Newtonian viscosity and stagnant lid convection on the terrestrial planetsGeophysical Research Letters, 1997
- Thermal and chemical evolution of the terrestrial magma oceanPhysics of the Earth and Planetary Interiors, 1997
- Mantle convection and stability of depleted and undepleted continental lithosphereJournal of Geophysical Research, 1997
- Onset of thermal convection in fluids with temperature‐dependent viscosity: Application to the oceanic mantleJournal of Geophysical Research, 1994
- Martian plate tectonicsJournal of Geophysical Research, 1994
- Thermal histories of the core and mantlePhysics of the Earth and Planetary Interiors, 1984