Splinter Meeting Computation
Time: Tuesday September 19, 14:00-16:30 and Wednesday September 20, 14:00-16:30
Convenors: Rolf Kuiper (Tübingen), Hubert Klahr (MPIA), Wilhelm Kley (Tübingen)
Numerical simulations play an ever more important role in astrophysical research. The goal of the splinter meeting is to bring together the national and international community in the field to present and discuss new computational methods, algorithms and applications. The topics will include magneto-hydrodynamics, radiative transport, N-body dynamics, and others.
Related contributions *)
|Bhasari||Non-equilibrium energy balance in the solar chromosphere||Talk|
|Brauer||Line and continuum radiative transfer simulations: From magnetic fields to polarization||Talk|
|Dolag||Magneticum: The largest cosmological hydrodynamical simulations||Talk|
|Puchwein||Forming (more) realistic galaxy clusters in simulations||Talk|
|Schmidt||Simulations of merging cool-core clusters||Talk|
|Wicht||Simulating the Jupiter's interior dynamics||Talk|
*) submitted abstracts, acceptance pending.