Coronal mass ejections (CMEs) and solar flares are the large-scale and most energetic
eruptive phenomena in our solar system and able to release a large quantity of plasma and …

Coronal mass ejections (CMEs) are large-scale expulsions of coronal plasma and magnetic
field propagating through the heliosphere. Because CMEs are observed by white-light …

Magnetic flux ropes are characterized by coherently twisted magnetic field lines, which are
ubiquitous in magnetized plasmas. As the core structure of various eruptive phenomena in …

We study the physical mechanism of a major X-class solar flare that occurred in the super
NOAA active region (AR) 12192 using data-driven numerical magnetohydrodynamic (MHD) …

The topology and dynamics of the three-dimensional magnetic field in the solar atmosphere
govern various solar eruptive phenomena and activities, such as flares, coronal mass …

Solar flares are powerful radiations occurring in the Sun's atmosphere. They are powered by
magnetic reconnection, a phenomenon that can convert magnetic energy into other forms of …

Impulsive solar energetic particle events are widely believed to be due to the prompt escape
into the interplanetary medium of flare-accelerated particles produced by solar eruptive …

Magnetic reconnection, the central engine that powers explosive phenomena throughout the
universe, is also perceived to be one of the principal mechanisms for accelerating particles …

The magnetohydrodynamics of active region NOAA 11283 is simulated using an initial non-
force-free magnetic field extrapolated from its photospheric vector magnetogram. We focus …

Context. Bridging the gap between heliospheric and solar observations of eruptions requires
the mapping of interplanetary coronal mass ejection (CME) footpoints down to the Sun's …