Characterized by cyclic axisymmetric perturbations to both the magnetic and fluid
parameters, magnetohydrodynamic fast sausage modes (FSMs) have proven useful for …

Studies on small-scale jets' formation, propagation, evolution, and role, such as type I and II
spicules, mottles, and fibrils in the lower solar atmosphere's energetic balance, have …

The existence of the Sun's hot atmosphere and the solar wind acceleration continues to be
an outstanding problem in solar-astrophysics. Although magnetohydrodynamic (MHD) …

Both observations and numerical simulations suggest that Alfvénic waves may carry
sufficient energy to sustain the hot temperatures of the solar atmospheric plasma. However …

It has been shown recently that magnetic twist and axisymmetric MHD modes are ubiquitous
in the solar atmosphere, and therefore the study of resonant absorption for these modes has …

Ubiquitous transverse oscillations observed in spicular waveguides, identified as the kink
wave-mode had previously been reported along with periodic structural distortions of the flux …

Over the past 20 yr, there has been increasing evidence of the existence of sausage waves
in the solar atmosphere. These observations make them useful tools in the context of …

Observations show that there are twisted magnetic flux tubes and plasma flow throughout
the solar atmosphere. The main purpose of this work is to obtain the damping rate of …

An analysis of the oscillatory motions and wave processes in active regions requires
knowledge of the structure of the magnetic fields in the chromosphere and corona. We study …

Context. Observations indicate variable widths exhibited by fan coronal loops and flare
loops that tend to widen towards the apex. Short-period, quasi-periodic pulsations in solar …