An introduction to numerical methods used in astrophysics and especially in modeling of systems described by the MHD equations.
Completion of the course provides expertise in the following:
- discretization of simple hyperbolic PDE's such as the advection equation
- examination of the stability of difference equations using von Neummann stabilty analysis
- implicit and explicit numerical schemes and solution techniques for these
- multi-grid methods
- characteristic equations and boundary conditions based on these
http://www.uio.no/studier/emner/matnat/astro/AST5110/h14/index.html
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[Set 3: Multigrid modelling exercise]("Multigrid modelling exercise")
Different grid sizes have results converging at different scales to different structures
Residuals
Relative error, compared to analytic solution