Keyphrases
Numerical Modeling
100%
Core Formation
100%
Planetary Accretion
100%
Planetary Bodies
75%
Planetary Surfaces
50%
Energy Dissipation
50%
Metal-rich
50%
Gravitational Energy
50%
Simplified Model
50%
Three-layer Structure
50%
Kuramoto
50%
Silicate
25%
Mercury
25%
Viscosity
25%
Mars
25%
Rheology
25%
Numerical Experiments
25%
Temperature Effect
25%
Pressure-temperature
25%
Free Surface
25%
Viscosity Contrast
25%
Formation Dynamics
25%
Long Wavelength
25%
Magma Ocean
25%
Pressure Stress
25%
Potential Energy
25%
Temperature Rise
25%
Thermomechanical
25%
Planetary Scale
25%
Viscosity Ratio
25%
Deformable
25%
Material Remains
25%
Low Viscosity
25%
Numerical Methodology
25%
Non-Newtonian
25%
High Viscosity
25%
Cartesian Grid
25%
Effective Viscosity
25%
Temperature Stress
25%
Stress Dependence
25%
Aspherical
25%
Quasi-spherical
25%
Metallic Core
25%
Silicate Layer
25%
Iron Core
25%
Yamamoto
25%
Molten Metal
25%
Planetary Shape
25%
Self-gravitation
25%
Rheological Effect
25%
Molten Silicates
25%
Protoplanet
25%
Self-gravitating
25%
Metal Silicate
25%
Metallic Layer
25%
Intermediate Metals
25%
Earth and Planetary Sciences
Numerical Modeling
100%
Destabilization
100%
Planetary Surface
100%
Energy Dissipation
100%
Magma
50%
Potential Energy
50%
Protoplanets
50%
Rheology
50%
Iron
50%