The heating of the solar chromosphere and corona to the observed high temperatures, imply
the presence of ongoing heating that balances the strong radiative and thermal conduction …

Solar coronal loops are the building blocks of the solar corona. These dynamic structures
are shaped by the magnetic field that expands into the solar atmosphere. They can be …

Modern observatories have revealed the ubiquitous presence of magnetohydrodynamic
waves in the solar corona. The propagating waves (in contrast to the standing waves) are …

Recent observations have revealed two types of decayless transverse oscillations in short
coronal loops: one with short periods scaling with loop lengths, and the other with longer …

Understanding many physical processes in the solar atmosphere requires determination of
the magnetic field in each atmospheric layer. However, direct measurements of the magnetic …

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

High-frequency wave phenomena present a great deal of interest as one of the possible
candidates to contribute to the energy input required to heat the corona as a part of the …

Alfvén wave turbulence models lie at the heart of many investigations into the winds and
extreme-ultraviolet and X-ray emission from cool, solar-like stars. The models provide …

Transverse oscillations that do not show significant damping in solar coronal loops are
found to be ubiquitous. Recently, the discovery of high-frequency transverse oscillations in …

We review novel data analysis techniques developed or adapted for the field of coronal
seismology. We focus on methods from the last ten years that were developed for extreme …