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 …

For a better understanding of the magnetic field in the solar corona and dynamic activities
such as flares and coronal mass ejections, it is crucial to measure the time-evolving coronal …

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 …

In this paper, we summarize current progress on using the observed magnetic fields for
magnetohydrodynamics (MHD) modeling of the coronal magnetic field and of solar …

It is well-known that magnetic fields dominate the dynamics in the solar corona, and new
generation of numerical modeling of the evolution of coronal magnetic fields, as featured …

Abstract The Coronal Global Evolutionary Model (CGEM) provides data-driven simulations
of the magnetic field in the solar corona to better understand the build-up of magnetic energy …

In recent years, global coronal models have experienced an ongoing increase in popularity
as tools for forecasting solar weather. Within the domain of up to 21.5 R⊙ …

Solar eruptions are well-recognized as major drivers of space weather but what causes
them remains an open question. Here we show how an eruption is initiated in a non …

This study aims to provide a reference for different magnetic field models and reconstruction
methods for interplanetary coronal mass ejections (ICMEs). To understand the differences in …

The solar eruption on 2007 May 19, from AR 10956 near solar disk center, consisted of a B9.
5 flare (12: 48 UT), a filament eruption, an EUV dimming, a coronal wave, and a multifront …