Rony Keppens (PI)
Rony is very proud to lead the team, and is actively researching MHD, developing codes, and applying them to Solar and Prominence-related physics.Postdocs
Niels Claes
Involvement period: 2020/01/01 - 2023/08/31Main developer of the Legolas code.
Largely focused on MHD spectral theory applied to solar atmospheric configurations, with particular interest in thermal instabilities and prominence fine structure.
Malcolm Druett
Involvement period: 2024/01/01 - presentMulti-dimensional solar flare simulations, and the lower solar atmosphere.
Jack Jenkins
Involvement period: 2020/04/01 - 2023/11/302.5 & 3D formation, structure, and evolution of solar prominence condensations.
Valeriia Liakh
Involvement period: 2022/01/17 - present2.5 & 3D simulation of prominence oscillations triggered by external activity.
Beatrice Popescu Braileanu
Involvement period: 2020/05/01 - 2020/09/30Partial ionization effects and implementation in MPI-AMRVAC
Wenzhi Ruan
Involvement period: 2020/02/01 - 2022/01/31Involvement period: 2022/10/01 - 2023/09/30
Impulsive phase of solar flares and coronal rains in gradual phase.
Alex Pietrow
Involvement period: 2024/03/01 - presentsynthetic views on 2.5 & 3D simulations of rain and prominences.
Sadeghi Mohammad
Involvement period: 2024/03/01 - presentwaves and oscillations in rain and prominences.
Madhurjya Changmai
Involvement period: 2021/09/27 - presentRole of turbulence and magnetic reconnection due to instabilities in Solar Prominences
Joris Hermans
Involvement period: 2019/10/01 - 2023/12/31The influence of cooling curves and flow on thermal instability
Jordi De Jonghe
Involvement period: 2019/09/01 - 2023/10/13Waves and instabilities in (H)MHD and multi-fluid descriptions.
Co-developer of the Legolas code.
Veronika Jercic
Involvement period: 2020/01/01 - 2020/12/31Oscillations of solar prominences with multi-threaded structure.
PhDs
Dion Donne
Involvement period: 2024/01/01 - present3D simulations of solar prominences with fine-structure.