This review article summarizes the advancement in the studies of Earth-affecting solar
transients in the last decade that encompasses most of solar cycle 24. It is a part of the effort …

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 …

Context. Recent observations by the Extreme Ultraviolet Imager (EUI) on board Solar Orbiter
have characterized prevalent small-scale transient brightenings in the corona above the …

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 …

The violent disruption of the coronal magnetic field is often observed to be restricted to the
low corona, appearing as a confined eruption. The possible causes of the confinement …

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 …

Solar filaments are an intriguing phenomenon, like cool clouds suspended in the hot corona.
Similar structures exist in the intergalactic medium as well. Despite being a long-studied …

This review paper summarizes the research of Mercury's magnetosphere in the Post-
MESSENGER era and compares its dynamics to those in other planetary magnetospheres …

Especially in cold and high-density regions, the assumptions of ideal
magnetohydrodynamics (MHD) can break down, making first order non-ideal terms such as …

Coronal mass ejections (CMEs) play an important role in space weather. The propagation
characteristics of CMEs in the Corona and interplanetary space determine whether, when …