Strong solar flares and coronal mass ejections, here defined not only as the bursts of
electromagnetic radiation but as the entire process in which magnetic energy is released …

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 …

Solar eruptions are spectacular magnetic explosions in the Sun's corona, and how they are
initiated remains unclear. Prevailing theories often rely on special magnetic topologies that …

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 …

Solar eruptions are explosive disruption of coronal magnetic fields, and often launch coronal
mass ejections into the interplanetary space. Intriguingly, many solar eruptions fail to escape …

Solar flares are spectacular coronal events that release large amounts of energy. They are
classified as either eruptive or confined,, depending on whether they are associated with a …

We review and summarize the applications of the Grad-Shafranov (GS) reconstruction
technique to space plasma structures in the Earth's magnetosphere and in the interplanetary …

The magnetic flux rope is among the most fundamental magnetic configurations in plasma.
Although its presence after solar eruptions has been verified by spacecraft measurements …

A clear understanding of the nature of the pre-eruptive magnetic field configurations of
Coronal Mass Ejections (CMEs) is required for understanding and eventually predicting …

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 …