Heat transport efficiency for stagnant lid convection with dislocation viscosity: Application to Mars and Venus

Keyphrases

• Boundary-layer Analysis 33%
• Critical Heat Flux 33%
• Dislocation 100%
• Finite Element Simulation 33%
• Heat Transfer Rate 33%
• Heat Transport 100%
• Lithospheric Mantle 33%
• Magmatism 33%
• Mantle Convection 33%
• Mantle Temperature 66%
• Mars 100%
• Newtonian Viscosity 33%
• Non-Newtonian Viscosity 33%
• Planetary Evolution 33%
• Plate Tectonics 100%
• Radiogenic Isotopes 33%
• Solidus 66%
• Stagnant Lid 33%
• Stagnant-lid Convection 100%
• Surface Heat Flux 33%
• Terrestrial Planets 33%
• Thermal Boundary Layer 33%
• Transport Efficiency 100%
• Upper Mantle 33%
• Venus 100%
• Viscosity 100%

Earth and Planetary Sciences

• Heat Flux 66%
• Lithosphere 33%
• Magmatism 33%
• Mantle Convection 33%
• Planetary Evolution 33%
• Plate (Tectonics) 100%
• Radiogenic Isotope 33%
• Terrestrial Planet 33%
• Thermal Boundary Layer 33%
• Upper Mantle 33%

Physics

• Finite Element Analysis 50%
• Lithosphere 50%
• Mantle Convection 50%
• Melting Point 100%
• Planetary Evolution 50%
• Terrestrial Planet 50%
• Thermal Boundary Layer 50%