Coronal jets represent important manifestations of ubiquitous solar transients, which may be
the source of significant mass and energy input to the upper solar atmosphere and the solar …

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 and stellar flares are the most intense emitters of X-rays and extreme ultraviolet
radiation in planetary systems,. On the Sun, strong flares are usually found in newly …

Abstract Coronal Mass Ejections (CMEs) are the key drivers of strong to extreme space
weather storms at the Earth that can have drastic consequences for technological systems in …

Solar filament eruptions, flares, and coronal mass ejections (CMEs) are manifestations of
drastic releases of energy in the magnetic field, which are related to many eruptive …

Hinode is Japan's third solar mission following Hinotori (1981–1982) and Yohkoh (1991–
2001): it was launched on 2006 September 22 and is in operation currently. Hinode carries …

Context. Jets are dynamic, impulsive, well-collimated plasma events that develop at many
different scales and in different layers of the solar atmosphere. Aims. Jets are believed to be …

In this work, we present results of a time-dependent data-driven numerical simulation
developed to study the dynamics of coronal active region magnetic fields. The evolving …

Observations of coronal jets increasingly suggest that local fragmentation and intermittency
play an important role in the dynamics of these events. In this work, we investigate this …

The solar atmosphere is full of complicated transients manifesting the reconfiguration of the
solar magnetic field and plasma. Solar jets represent collimated, beam-like plasma …