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Resolving turbulence
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Classroom Contents
Stellar Transport and the Climate of Stars - Blackboard Lunch
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- 1 Intro
- 2 How to study stars
- 3 Chemical abundances
- 4 Global oscillation modes
- 5 Types of modes
- 6 Star properties
- 7 Nuclear time scale
- 8 Stellar structure
- 9 Thermal equilibrium
- 10 Transport
- 11 Why Care
- 12 Observations
- 13 Matching Conditions
- 14 Numerical Challenges
- 15 Resolving turbulence
- 16 Rotation magnetic fields
