Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Centre for Plasma Astrophysics, K.U.Leuven, Belgium
Center for Plasma Astrophysics, K.U.Leuven, Belgium; Leuven Mathematical Modeling and Computational Science Centre, Leuven, Belgium; Astronomical Institute, Utrecht University, the Netherlands; FOM Institute for Plasma Physics Rijnhuizen, Nieuwegein, the Netherlands
CPA / K.U.Leuven, Celestijnenlaan 200 B, 3001 Leuven, Belgium
National Center for Atmospheric Research, Boulder, CO, US
FOM-Institute for Plasma Physics `Rijnhuizen', P.O. Box 1207, 3430 BE Nieuwegein, The Netherlands
Centre for Plasma Astrophysics, K.U.LEUVEN, Belgium
Centre for Plasma Astrophysics, Katholieke Universiteit Leuven, Celestijnenlaan 200B, B-3001 Leuven, Belgium Institute for Plasma Physics `Rijnhuizen' - Institute for Plasma Physics
Belgian National Fund of Scientific Research, Kiepenheuer-Institut für Sonnenphysik
FOM-Institute for Plasma Physics Rijnhuizen, P.O. Box 1207, 3430 BE Nieuwegein, The Netherlands
FOM-Institute for Plasma Physics `Rijnhuizen', Nieuwegein, the Netherlands
Astronomical Institute, Utrecht University, Utrecht, the Netherlands
FOM-Institute for Plasma Physics Rijnhuizen, PO Box 1207, 3430 BE Nieuwegein, The Netherlands
FOM-Institute for Plasma-Physics Rijnhuizen, P.O. Box 1207, 3430 BE Nieuwegein, The Netherlands
FOM-Institute for Plasma Astrophysics 'Rijnhuizen', P.O. Box 1207, 3430 BE Nieuwegein, The Netherlands
Centre for Plasma-Astrophysics, KU Leuven, Celestijnenlaan 200B, 3001 Leuven, Belgium; FOM - Institute for Plasma Physics Rijnhuizen, PO Box 1207, 3430 BE Nieuwegein, The Netherlands
FOM-Institute for Plasma Physics Rijnhuizen
Centre for Plasma Astrophysics, K.U.Leuven, Celestijnenlaan 200B, 3001 Heverlee, Belgium
A multidimensional grid-adaptive relativistic magnetofluid code
A new radiative cooling curve based on an up to date plasma emission code
Accretion funnels onto weakly magnetized young stars
Adaptive mesh refinement for conservative systems: multi-dimensional efficiency evaluation
AMRVAC and Relativistic Hydrodynamic simulations for GRB afterglow phases
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