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 …

Magnetohydrodynamic Alfvén waves have been a focus of laboratory plasma physics and
astrophysics for over half a century. Their unique nature makes them ideal energy …

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 use images of high spatial and temporal resolution, obtained using both ground-and
space-based instrumentation, to investigate the role magnetic field inclination angles play in …

Waves and oscillations are important solar phenomena, not only because they can
propagate and dissipate energy in the chromosphere, but also because they carry …

We seek to clarify the nature of running penumbral (RP) waves: are they chromospheric
trans-sunspot waves or a visual pattern of upward-propagating waves? Full Stokes …

Recent high-resolution observations of sunspot oscillations using simultaneously operated
ground-and space-based telescopes reveal the intrinsic connection between different layers …

Context. Sunspot oscillations are one of the most frequently studied wave phenomena in the
solar atmosphere. Understanding the basic physical processes responsible for sunspot …

We present simultaneous, high-resolution, multi-temperature observations of running waves
and umbral flashes in a sunspot with the Interface Region Imaging Spectrograph. We …