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 corona is a layer of hot plasma that surrounds the Sun, traces out its complex magnetic
field, and ultimately expands into interplanetary space as the supersonic solar wind …

The chromosphere is a thin layer of the solar atmosphere that bridges the relatively cool
photosphere and the intensely heated transition region and corona. Compressible and …

The solar chromosphere forms a crucial, yet complex and until recently poorly understood,
interface between the solar photosphere and the heliosphere.▪ Advances in high-resolution …

The Sunrise balloon-borne solar observatory consists of a 1 m aperture Gregory telescope,
a UV filter imager, an imaging vector polarimeter, an image stabilization system, and further …

The 1.5 m telescope GREGOR opens a new window to the understanding of solar small‐
scale magnetism. The first light instrumentation includes the Gregor Fabry Pérot …

The Sunrise balloon-borne solar observatory, consisting of a 1 m aperture telescope that
provides a stabilized image to a UV filter imager and an imaging vector polarimeter, carried …

Hinode is Japan's third solar mission following Hinotori (1981–1982) and Yohkoh (1991–
2001): it was launched on 2006 September 22 and is in operation currently. Hinode carries …

We present observational evidence of compressible MHD wave modes propagating from the
solar photosphere through to the base of the transition region in a solar magnetic pore. High …

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 …