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 …

The heating of the solar chromosphere and corona to the observed high temperatures, imply
the presence of ongoing heating that balances the strong radiative and thermal conduction …

Using high-cadence observations from the Hydrogen-alpha Rapid Dynamics camera
imaging system on the Dunn Solar Telescope, we present an investigation of the statistical …

Solar pores are intense concentrations of magnetic flux that emerge through the solar
photosphere. When compared to sunspots, they are much smaller in diameter and can …

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 …

Abstract The Daniel K. Inouye Solar Telescope (DKIST) is a ground-based observatory for
observations of the solar atmosphere featuring an unprecedented entrance aperture of four …

Sunspots host various oscillations and wave phenomena like umbral flashes, umbral
oscillations, running penumbral waves, and coronal waves. All fan loops rooted in sunspot …

We present a study of wave processes in sunspots from active regions NOAA 11131 on
2010 December 10 and NOAA 12565 on 2016 July 14 observed by SDO/AIA in the 1600 …

Solar pores are efficient magnetic conduits for propagating magnetohydrodynamic wave
energy into the outer regions of the solar atmosphere. Pore observations often contain …

The importance of the chromosphere in the mass and energy transport within the solar
atmosphere is now widely recognized. This review discusses the physics of …