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 …

We present an overview of the National Science Foundation's Daniel K. Inouye Solar
Telescope (DKIST), its instruments, and support facilities. The 4 m aperture DKIST provides …

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 …

The Sun's outer atmosphere is heated to temperatures of millions of degrees, and solar
plasma flows out into interplanetary space at supersonic speeds. This paper reviews our …

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 …

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 …

Magnetoseismology, a technique of magnetic field diagnostics based on observations of
magnetohydrodynamic (MHD) waves, has been widely used to estimate the field strengths …

Total solar eclipses (TSEs) provide a unique opportunity to quantify the properties of the K-
corona (electrons), F-corona (dust), and E-corona (ions) continuously from the solar surface …

The article discusses characteristics, fundamental and applied tasks of the Siberian
Radioheliograph that is developed at the ISTP SB RAS Radio Astrophysical Observatory …