Context. Computational astrophysics nowadays routinely combines grid-adaptive
capabilities with modern shock-capturing, high resolution spatio-temporal integration …

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 …

Spicules are rapidly evolving fine-scale jets of magnetized plasma in the solar
chromosphere. It remains unclear how these prevalent jets originate from the solar surface …

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 …

The thermal structure of the chromosphere is regulated through a complex interaction of
various heating processes, radiative cooling, and the ionization degree of the plasma. Here …

Nearly all energy generated by fusion in the solar core is ultimately radiated away into space
in the solar atmosphere, while the remaining energy is carried away in the form of neutrinos …

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 Mg ii h and k lines are among the best diagnostic tools of the upper solar
chromosphere. This region of the atmosphere is of particular interest, as it is the lowest …

To study acoustic wave propagation and the corresponding energy deposition in partially
ionized plasmas, we use a two-fluid computational model that treats neutrals and charged …

Our understanding of magnetic reconnection (MR) under chromospheric conditions remains
limited. Recent observations have demonstrated the important role of ion–neutral …