Rotational Flows in Solar Coronal Flux Rope Cavities
Developing a first 2.5D numerical model to reproduce the rotational flows in the prominence cavities.
Multithermal Jet Formation Triggered by Flux Emergence
Combining observation and simulations, we investigate the influence of flux emergence at one footpoint of an arcade on coronal rain as well as induced erupti...
Prominence oscillations triggered by external perturbations
Studying the induced prominence oscillation by the nearby eruption and energetic coronal wave from the distant source.
Prominence heating models
Testing a multitude of scaled heating laws for the solar corona on the prevalence of prominence condensations within flux rope topologies
3D Prominence formation
Rendering the successful simulation of a fully 3D solar filament/prominence, down to scales of ~20 km, using MPI-AMRVAC.
Coronal rain in randomly heated arcades
Using MPI-AMRVAC, we performed a 2.5D MHD simulation to investigate the formation and evolution of the coronal rain phenomenon.
When hot meets cold: post-flare coronal rain
We performed a 2.5D flare simulation from pre-flare phase all the way into the gradual phase to study the formation of coronal rain in post-fflare loop.
Postflare loop condensation without background heating.
We show that condensation can happen inside post-flare loop without background heating with a test.
2.5D Prominence formation
MPI-AMRVAC is successfully deployed to study the formation and evolution of a prominence in a 2.5D translationally-invariant setup.