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The Erwin Schroedinger Institute for Mathematical Physics

Multi-scale models of magnetohydrodynamic (MHD) turbulence in solar convection (part 2/2)

The main objective is to advance mathematical tools to understand solar convection with the use of the package ANTARES (A Numerical Tool for the Astrophysical RESearch), developed at the Institute of Mathematics at the University of Vienna for simulations of solar granulation and other astrophysical flows. 

At a glance

Type: Research in Teams
When: Sep 01, 2014 to
Oct 08, 2014
Organizers: Friedrich Kupka and Herbert Muthsam (U Vienna), Arakel Petroysan (Russian Academy of Sciences), Oleh Pomazan (Nat. Research Nuclear U, MEPhI, Moscow)
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