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Strong PZ dependence on P in simulations
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Classroom Contents
Convective Penetration - Context, Theory, and Simulations - Evan Anders
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- 1 Stellar convective penetration: Context, theory, and simulations
- 2 A simple model of a radiative-convective boundary
- 3 Convective overshoot causes entrainment.
- 4 Three linked processes in convective boundary mixing A fluid dynamical perspective
- 5 Entrainment builds a penetration zone
- 6 A toy model of fluxes in stellar convection
- 7 What sets the size of a convective penetration region?
- 8 A toy model of fluxes in convective penetration
- 9 Strong PZ dependence on P in simulations
- 10 From 3D to MESA
- 11 Wrap up We think we understand convective penetration, generally We think it's parameterizeable. We need to expand the model & nail down parameter values. Questions?
- 12 Dynamics of convective penetration
- 13 Measured output profiles of a simulation of penetration
