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 …

Aiming to assess the progress and current challenges on the formidable problem of the
prediction of solar energetic events since the COSPAR/International Living With a Star …

Context. Investigating the early-stage evolution of an erupting flux rope from the Sun is
important for understanding the mechanisms of how it loses its stability and its space …

Context. The solar magnetic field plays an essential role in the formation, evolution, and
dynamics of large-scale eruptive structures in the corona. The estimation of the coronal …

We develop a general description of how information propagates through a
magnetohydrodynamic (MHD) system based on the method of characteristics and use that to …

Context. A proper estimate of the chromospheric magnetic fields is thought to improve
modelling of both active region and coronal mass ejection evolution. However, because the …

Context. Constructing the relevant magnetic field lines from active region modelling data is
crucial to understanding the underlying instability mechanisms that trigger the …

We investigate here the magnetic properties of a large-scale magnetic flux rope related to a
coronal mass ejection (CME) that erupted from the Sun on September 12, 2014 and …

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 …

We present a newly developed data-driven magnetohydrodynamics (MHD) simulation code
under a zero-β approximation based on a method proposed by Hayashi et al. 2018 and …