Context. The solar atmosphere is highly dynamic, and observing the small-scale features is
valuable for interpretations of the underlying physical processes. The contrasts and …

Abstract Space-weather HMI Active Region Patches (SHARPs) data from the Helioseismic
and Magnetic Imager (HMI) on board the Solar Dynamics Observatory (SDO) provides high …

Context. Interferometric observations of the Sun with the Atacama Large Millimeter/sub-
millimeter Array (ALMA) provide valuable diagnostic tools for studying the small-scale …

Broad-band imaging and even imaging with a moderate bandpass (about 1 nm) provides a
photon-rich environment, where frame selection (lucky imaging) becomes a helpful tool in …

Understanding the complex dynamics and structure of the upper solar atmosphere strongly
benefits from the use of a combination of several diagnostics. Frequently, such diverse …

The wealth of observational data available has been instrumental in investigating physical
features relevant to solar granulation, supergranulation and Active Regions. Meanwhile …

Context. The intensity of radiation from the solar atmosphere at millimetre wavelengths is
closely related to the plasma temperature, and the formation height of the radiation is …

Context. Activity on the far side of the Sun is routinely studied through the analysis of the
seismic oscillations detected on the near side using helioseismic techniques such as phase …

In recent years, the new physics of the Sun has been revealed using advanced data with
high spatial and temporal resolutions. The Helioseismic and Magnetic Imager (HMI) on …

The volume of data being collected in solar physics has exponentially increased over the
past decade and with the introduction of the Daniel K. Inouye Solar Telescope (DKIST) we …