Magnetic fields play a fundamental role in the structure and dynamics of the solar corona. As
they are driven by their footpoint motions on the solar surface, which transport energy from …

Magnetic flux ropes are a bundle of twisted magnetic field lines produced by internal electric
currents, which are responsible for solar eruptions and are the major drivers of geomagnetic …

We present a method of conducting data-driven simulations of solar active regions and flux
emergence with the MURaM radiative magnetohydrodynamics (MHD) code. The horizontal …

The solar active region NOAA 12887 produced a strong X1. 0 flare on 2021 October 28,
which exhibits X-shaped flare ribbons and a circle-shaped erupting filament. To understand …

We review the current literature on the formation of coherent structures (CoSs) in strongly
turbulent 3D magnetized plasmas. CoSs [Current Sheets (CS), magnetic filaments, large …

We performed two data-based magnetohydrodynamic (MHD) simulations for solar active
region 12371, which produced an M6. 5 flare. The first simulation is a full data-driven …

Solar flares and plasma eruptions are sudden releases of magnetic energy stored in the
plasma atmosphere. To understand the physical mechanisms governing their occurrences …

We investigate the transverse coronal-loop oscillations induced by the eruption of a
prominence-carrying flux rope on 7 December 2012. The flux rope, originating from NOAA …

A data-driven active region evolution (DARE) model has been developed to study the
complex structures and dynamics of solar coronal magnetic fields. The model is configured …

Data-driven simulation proves to be a powerful tool in revealing the dynamic process of the
solar corona, but it remains challenging to implement the driving boundary conditions in a …