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 …

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 …

Using data obtained by the EUV Imaging Spectrometer on board Hinode, we have
performed a survey of obvious and persistent (without significant damping) Doppler shift …

The solar wind is known to be highly structured in space and time. Observations from Parker
Solar Probe have revealed an abundance of so-called magnetic switchbacks within the near …

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 …

We present a comprehensive radiative magnetohydrodynamic simulation of the quiet Sun
and large solar active regions. The 197 Mm wide simulation domain spans from 18 (10) Mm …

Coronal bright points (CBPs) are ubiquitous structures in the solar atmosphere composed of
hot small-scale loops observed in extreme-ultraviolet (EUV) or X-rays in the quiet Sun and …

Here we detail the dynamic evolution of localized reconnection regions about 3D magnetic
null points using numerical simulation. We demonstrate for the first time that reconnection …

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 …

Coronal bright points (CBPs) are a fundamental class of solar activity. They represent a set
of low-corona small-scale loops with enhanced emission in the extreme-ultraviolet and X-ray …