Grete, Philipp; Vlaykov, Dimitar G; Schmidt, Wolfram; Schleicher, Dominik R G; Federrath, Christoph
Turbulence in compressible plasma plays a key role in many areas of astrophysics and engineering.
The extreme plasma parameters in these environments, e.g. high Reynolds numbers, supersonic and
super-Alfvenic flows, however, make direct numerical simulations computationally intractable even
for the simplest treatment—magnetohydrodynamics (MHD). To overcome this problem one can use
subgrid-scale (SGS) closures—models for the influence of unresolved, subgrid-scales on the resolved
ones. In...[Show more]
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