The potential role of non‐Newtonian rheology in the resurfacing of Venus
- 1 March 1996
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 23 (5) , 511-514
- https://doi.org/10.1029/96gl00387
Abstract
No abstract availableKeywords
This publication has 23 references indexed in Scilit:
- How does Venus lose heat?Journal of Geophysical Research: Planets, 1995
- Ejecta correlations with spatial crater density and Venus resurfacing historyGeophysical Research Letters, 1995
- A source‐sink model of the generation of plate tectonics from non‐Newtonian mantle flowJournal of Geophysical Research, 1995
- Phase boundary deflections at 660‐km depth and episodically layered isochemical convection in the mantleJournal of Geophysical Research, 1994
- Role of plates and temperature‐dependent viscosity in phase change dynamicsJournal of Geophysical Research, 1994
- Phase transition Clapeyron slopes and transition zone seismic discontinuity topographyJournal of Geophysical Research, 1994
- Effects of multiple phase transitions in a three‐dimensional spherical model of convection in Earth's mantleJournal of Geophysical Research, 1994
- The global resurfacing of VenusJournal of Geophysical Research, 1994
- Episodic large‐scale overturn of two‐layer mantles in terrestrial planetsJournal of Geophysical Research, 1994
- Temperature‐dependent Newtonian and non‐Newtonian convection: Implications for lithospheric processesGeophysical Research Letters, 1993