Vortex flows, related to solar convective turbulent dynamics at granular scales and their
interplay with magnetic fields within intergranular lanes, occur abundantly on the solar …

Abstract Space plasmas can be described as conducting flows in a turbulent state, where
fluid motion is determined by a host of kinetic and magnetic coherent structures of different …

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 …

Context. Current models of the solar wind must approximate (or ignore) the small-scale
dynamics within the solar atmosphere; however, these are likely important in shaping the …

Context. Vortex flows exist across a broad range of spatial and temporal scales in the solar
atmosphere. Small-scale vortices are thought to play an important role in energy transport in …

Abstract The National Science Foundation's Daniel K. Inouye Solar Telescope (DKIST) will
revolutionize our ability to measure, understand, and model the basic physical processes …

The solar atmosphere is known to be replete with magneto-hydrodynamic wave modes, and
there has been significant investment in understanding how these waves propagate through …

Context. Chromospheric swirls are related to convectively driven vortex flows and
considered to play a significant role in the dynamics and heating of the upper solar …

In this work, a state-of-the-art vortex detection method, Instantaneous Vorticity Deviation, is
applied to locate three-dimensional vortex tube boundaries in numerical simulations of solar …

In the following short review we will outline some of the possible interaction processes of
lower solar atmospheric plasma with the embedded small-scale solar magnetic fields. After …