The quiet Sun is the region of the solar surface outside of sunspots, pores, and plages. In
continuum intensity it appears dominated by granular convection. However, in polarized …

Abstract The Atacama Large Millimeter/submillimeter Array (ALMA) is a new powerful tool for
observing the Sun at high spatial, temporal, and spectral resolution. These capabilities can …

Abstract The Daniel K. Inouye Solar Telescope (DKIST) Visible Spectro-Polarimeter (ViSP)
is a traditional slit-scanning spectrograph with the ability to observe solar regions up to a …

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 The Diffraction-Limited Near-Infrared Spectropolarimeter (DL-NIRSP) is one of the
first-light instruments for the National Science Foundation's Daniel K. Inouye Solar …

Since the first discovery of a broad-lined type Ic supernova (SN) with a long-duration gamma-
ray burst (GRB) in 1998, fewer than fifty GRB-supernovae (SNe) have been discovered. The …

Given its unchallenged capabilities in terms of sensitivity and spatial resolution, the
combination of imaging spectropolarimetry and numeric Stokes inversion represents the …

The European Solar Telescope (EST) is a project aimed at studying the magnetic
connectivity of the solar atmosphere, from the deep photosphere to the upper …

Context. While it is conjectured that a chromospheric canopy plays a role in penumbra
formation, it has been difficult to find observational evidence of the connectivity between the …

Context. When spectropolarimetric data are recorded at high spatial, spectral, and temporal
resolution, the quality of the data is generally limited by the signal-to-noise ratio. Aims. We …