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 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 Sun supports a rich spectrum of internal waves that are continuously excited by
turbulent convection. The Global Oscillation Network Group (GONG) network and the …

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 …

A magnetic field modifies the properties of waves in a complex way. Significant advances
have been made recently in our understanding of the physics of sunspot waves with the help …

We derive self-consistent formalism for the description of multi-component partially ionized
solar plasma, by means of the coupled equations for the charged and neutral components …

Fully compressible magnetohydrodynamic (MHD) simulations are a fundamental tool for
investigating the role of dynamo amplification in the generation of magnetic fields in deep …

Waves observed in the photosphere and chromosphere of sunspots show complex
dynamics and spatial patterns. The interpretation of high-resolution sunspot wave …

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 …

We review our current understanding of sunspots from the scales of their fine structure to
their large scale (global) structure including the processes of their formation and decay …