Developing a first 2.5D numerical model to reproduce the rotational flows in the prominence cavities.
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...
Studying the induced prominence oscillation by the nearby eruption and energetic coronal wave from the distant source.
Testing a multitude of scaled heating laws for the solar corona on the prevalence of prominence condensations within flux rope topologies
Rendering the successful simulation of a fully 3D solar filament/prominence, down to scales of ~20 km, using MPI-AMRVAC.
Using MPI-AMRVAC, we performed a 2.5D MHD simulation to investigate the formation and evolution of the coronal rain phenomenon.
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.
We show that condensation can happen inside post-flare loop without background heating with a test.
MPI-AMRVAC is successfully deployed to study the formation and evolution of a prominence in a 2.5D translationally-invariant setup.