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. 

Coming soon.

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At a glance
Research in Teams
Sept. 1, 2014 — Oct. 8, 2014