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Algorithms: finite-volume discretization.
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Astrophysical Fluid Dynamics - James Stone
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- 1 Intro
- 2 Example: The Sun
- 3 Jupiter's atmosphere
- 4 HST image of region in Carina nebula
- 5 Crab nebula (supernovae remnant)
- 6 Mathematical Model
- 7 Ideal magnetohydrodynamics (MHD)
- 8 MHD waves.
- 9 Phase velocities of MHD waves: Friedrichs diagrams.
- 10 Circularly polarized Alfven waves.
- 11 Numerical Methods
- 12 World's fastest (open) computer
- 13 Algorithms: finite-volume discretization.
- 14 Godunov's orginal (first-order) method
- 15 Higher-order methods
- 16 Adaptive Mesh Refinement (AMR)
- 17 Validating physics modules
- 18 Relativistic ray-tracing important
- 19 Future Work
