Stefaan Poedts
Uniwersytet Marii Curie-Skłodowskiej, KU Leuven Association, KU Leuven
About
Stefaan Poedts graduated in Applied Mathematics in 1984 at the KU Leuven. As 'research assistant' of the Belgian National Fund for Scientific Research he obtained a PhD in Sciences (Applied Mathematics) in 1988 at the same university. After one year as Postdoctoral researcher he left the KU Leuven to become a Postdoctoral researcher at the Max-Planck-Institut für Plasmaphysik in Garching bei München.
In October 1991 he moved to the Netherlands to work in the FOM-Instituut voor Plasmafysica 'Rijnhuizen', first as 'scientific collaborator' and from October 1995 on as 'Senior researcher'.
In October 1996 he returned to the KU Leuven as Research Associate of the FWO-Vlaanderen at the Centre for mathematical Plasma Astrophysics (CPA) in the Department of mathematics. Since October 1, 2000 he is Academic Staff at the KU Leuven, first as 'Hoogleraar' (= 'Reader' in UK and 'associate professor' in USA) and presently as 'Gewoon hoogleraar' (= 'Professor' in UK and 'Full Professor' in USA).
Research interests:
Solar Astrophysics: Theory and Observations
Coronal loop dynamics
Coronal heating mechanisms
Space Weather
Solar corona and solar wind modeling
Coronal Mass Ejections: initiation and IP evolution, incl. interaction with planetary magnetospheres
Controlled Thermonuclear Fusion Research (CTFR)
Tokamak dynamics and stability
MHD spectroscopy
Employment
-
Uniwersytet Marii Curie-Skłodowskiej Professor (part-time)2019 - Present
-
KU Leuven Association
-
KU Leuven full professor
Education
-
KU Leuven PhD1984 - 1988
-
KU Leuven Master of Science, Applied mathematics1982 - 1984
-
KU Leuven Bachelor in Science, Mathematics1980 - 1982
Projects & Funding
Projects & funding information is unavailable.
Publications (1346)
- MHD Modeling of Magnetic Flux Evolution Around Solar Maximum by the Coronal Model COCONUT Save
- Magnetosphere–ionosphere response to the 21 and 25 June 2015 coronal mass ejections Save
- Comprehensive Magnetohydrodynamic Modeling of 10 Successive Coronal Mass Ejections Driving a Historic Geomagnetic Storm—the 2024 Mother’s Day Event Save
- The space weather awareness training network SWATNet Save
- Dynamic spectra of type III radio emissions from particle-in-cell simulations Save
- Hybrid Simulations of the Proton Beam Instabilities in the Young Solar Wind: The Formation of Hammerhead-like Distributions Save
- EGU LUNEX 2026 Total Solar Eclipse Campaign in Spain: Early Career Scientist Multiwavelength Observations and Outreach Save
- Impact of heat flux and suprathermal electrons on steady-state solar wind modelling with Icarus Save
- Adaptive mesh refinement strategies for heliosphere and space weather modelling Save
- Advancing Heliophysics and Space Weather Modeling through Open Science Save