Waves and oscillations have been observed in the Sun's atmosphere for over half a century.
While such phenomena have readily been observed across the entire electromagnetic …

In this article we review small-scale dynamo processes that are responsible for magnetic
field generation on scales comparable to and smaller than the energy carrying scales of …

Context. Magnetic reconnection in the deep solar atmosphere can give rise to enhanced
emission in the Balmer hydrogen lines, a phenomenon referred to as Ellerman bombs. Aims …

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 …

Aims. Solar prominences contain a significant number of neutral species. The dynamics of
the ionised and neutral fluids composing the prominence plasma can be slightly different if …

We report on observations acquired by the Interferometric Bidimensional Spectropolarimeter
(IBIS) during SOL2014-10-22T14: 02, an X1. 6 flare that occurred in active region NOAA …

Partially ionized plasmas (PIP) constitute an essential ingredient of our plasma universe.
Historically, the physical effects associated with partial ionization were considered in …

Observations at (sub-) millimeter wavelengths offer a complementary perspective on our
Sun and other stars, offering significant insights into both the thermal and magnetic …

This review covers the techniques, observations, and inferences of solar flare spectroscopy.
It is not a spectroscopist's view of solar flares but rather a solar flare physicist's view of …

In this work, we study the accuracy that can be achieved when inferring the atmospheric
information from realistic numerical magneto-hydrodynamic simulations that reproduce the …