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 cutoff effect is a significant determinant of solar magnetohydrodynamic wave
propagation and hence pivotal in energy transfer studies, such as solar plasma heating and …

Alfvénic motions are ubiquitous in the solar atmosphere and their observed properties are
closely linked to those of photospheric p-modes. However, it is still unclear how a …

Context. While it is conjectured that a chromospheric canopy plays a role in penumbra
formation, it has been difficult to find observational evidence of the connectivity between the …

The X-ray and extreme-ultraviolet (EUV) emissions from low-mass stars significantly affect
the evolution of the planetary atmosphere. However, it is observationally difficult to constrain …

Acoustic wave heating is believed to contribute significantly to the missing energy input
required to maintain the solar chromosphere in its observed state. We studied the …

Context. Transverse oscillations are ubiquitously observed in the solar corona, both in
coronal loops and in open magnetic flux tubes. Numerical simulations suggest that their …

Solar pores are efficient magnetic conduits for propagating magnetohydrodynamic wave
energy into the outer regions of the solar atmosphere. Pore observations often contain …

The importance of the chromosphere in the mass and energy transport within the solar
atmosphere is now widely recognized. This review discusses the physics of …

Context. Sunspot umbrae show a change in the dominant period of their oscillations from
five minutes (3.3 mHz) in the photosphere to three minutes (5.5 mHz) in the chromosphere …