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 solar atmosphere is a complex, coupled, highly dynamic plasma environment, which
shows rich structuring due to the presence of gravitational and magnetic fields. Several …

Pores and sunspots are ideal environments for the propagation of guided
magnetohydrodynamic (MHD) waves. However, modelling such photospheric waveguides …

Magnetic bright points on the solar photosphere mark the footpoints of kilogauss magnetic
flux tubes extending toward the corona. Convective buffeting of these tubes is believed to …

In the following short review we will outline some of the possible interaction processes of
lower solar atmospheric plasma with the embedded small-scale solar magnetic fields. After …

Magnetoacoustic waves in solar magnetic flux tubes may be affected by the presence of
background rotational flows. Here, we investigate the behaviour of m= 0 and m=±1 modes of …

In this study, we explore the possibility of simplifying the modeling of magnetohydrodynamic
slow body modes observed in photospheric magnetic structures such as the umbrae of …

In this paper, we provide clear direct evidence of multiple concurrent higher-order
magnetohydrodynamic (MHD) modes in circular and elliptical sunspots by applying both …

Aims. This study is motivated by observations of coordinated transverse displacements in
neighboring solar active region loops, addressing specifically how the behavior of kink …

Fast sausage modes (FSMs) in flare loops have long been invoked to account for rapid
quasi-periodic pulsations (QPPs) with periods of order seconds in flare lightcurves …