Physics
Scientist
Astronomisch Instituut, Katholieke Universiteit Leuven, Celestijnenlaan 200 B, 3030 Heverlee, Belgium
Department of Solar Physics, Royal Observatory of Belgium, Ringlaan 3, B-1180, Brussel, Belgium
Department of Mathematical and Computational Sciences, University of St. Andrews
Center for Plasma Astrophysics, Katholieke Universiteit Leuven, Celestijnenlaan 200B, B-3001 Leuven, Belgium
SIDC, Royal Observatory of Belgium, Ringlaan 3, 1180 Brussels, Belgium
St. Andrews Univ., United Kingdom
Leuven, Katholieke Universiteit, Heverlee, Belgium
Centre for Plasma Astrophysics, Katholieke Universiteit Leuven, Celestijnenlaan 200B, B-3001 Leuven, Belgium of St. Andrews, UK
University of St. Andrews, St. Andrews, Scotland, UK
Koninklijke Sterrenwacht van Belgie, Ringlaan 3, 1180 Ukkel, Belgium
SIDC-Royal Observatory of Belgium
Royal Observatory of Belgium, Ringlaan -3- Avenue Circulaire, 1180 Brussels, Belgium
Royal Observatory of Belgium, Ringlaan 3, 1180 Brussels, Belgium / SIDC, Royal Observatory of Belgium, Ringlaan-3, Brussels 1180, Belgium
Royal Observatory of Belgium, Belgium
A combined finite element/Fourier series method for the numerical study of the stability of line-tied magnetic plasmas
A complete coronal loop stability analysis in ideal magnetohydrodynamics. II. Force-free cylindrical equilibria
A complete solar coronal loop stability analysis in ideal magnetohydrodynamics. I. Non-force-free cylindrical equilibria
A solar coronal heating model: multi-energy relaxation events
Coronal heating by magnetic reconnection in loops with zero net current
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