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 details of the mechanism (s) responsible for the observed heating and dynamics of the
solar atmosphere still remain a mystery. Magnetohydrodynamic waves are thought to have a …

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 …

Transverse magnetohydrodynamic waves have been shown to be ubiquitous in the solar
atmosphere and can, in principle, carry sufficient energy to generate and maintain the Sun's …

We present high-cadence observations and simulations of the solar photosphere, obtained
using the Rapid Oscillations in the Solar Atmosphere imaging system and the MuRAM …

Coronal holes are the coolest and darkest regions of the upper solar atmosphere, as
observed both on the solar disk and above the solar limb. Coronal holes are associated with …

We have modeled numerically the propagation of waves through magnetic structures in a
stratified atmosphere. We first simulate the propagation of waves through a number of …

Large-scale, globally propagating wave-like disturbances have been observed in the solar
chromosphere and by inference in the corona since the 1960s. However, detailed analysis …

Can the ubiquitously magnetic solar atmosphere have any effect on solar global
oscillations? Traditionally, solar atmospheric magnetic fields are considered to be somewhat …

A major, albeit serendipitous, discovery of the SOlar and Heliospheric Observatory mission
was the observation by the Extreme Ultraviolet Telescope (EIT) of large-scale extreme …