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 …

Filaments are omnipresent features in the solar atmosphere. Their location, properties, and
time evolution can provide important information about changes in solar activity and assist in …

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 …

We discuss the chosen concepts, detailed design, implementation and calibration of the 85-
electrode adaptive optics (AO) system of the Swedish 1-meter Solar Telescope (SST), which …

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 …

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 …

Context. Solar jets are collimated plasma flows moving along magnetic field lines and are
accelerated at low altitude following magnetic reconnection. Several of them originate from …

Context. Investigating light bridges (LBs) helps us comprehend key aspects of sunspots.
However, few studies have analyzed the properties of LBs in terms of the geometric height …

Context. Magnetic reconnection in the deep solar atmosphere can give rise to enhanced
emission in the Balmer hydrogen lines, a phenomenon known as Ellerman bombs (EBs). It …