Splinter Meeting Computation

Computational Astrophysics

Time: Tuesday September 19, 14:00-16:30 and Wednesday September 20, 14:00-16:30

Room: HS3

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 *)

PresentationTitleType PDF
BhasariNon-equilibrium energy balance in the solar chromosphereTalk PDF
BrauerLine and continuum radiative transfer simulations: From magnetic fields to polarizationTalk PDF
DolagMagneticum: The largest cosmological hydrodynamical simulationsTalk PDF
PuchweinForming (more) realistic galaxy clusters in simulationsTalk PDF
SchmidtSimulations of merging cool-core clustersTalk PDF
WichtSimulating the Jupiter's interior dynamicsTalk PDF

*) submitted abstracts, acceptance pending.

Further information provided by the organizers