Partially ionized plasmas are found across the Universe in many different astrophysical
environments. They constitute an essential ingredient of the solar atmosphere, molecular …

The solar atmosphere is full of complicated transients manifesting the reconfiguration of the
solar magnetic field and plasma. Solar jets represent collimated, beam-like plasma …

This paper presents a theory of weakly nonlinear wave propagation in superposed fluids in
the existence of magnetic fields. The extended direct algebraic approach has been utilized …

Aims. We aim to study the standing fundamental kink mode of coronal loops in the nonlinear
regime, investigating the changes in energy evolution in the cross-section and oscillation …

Context. Recent numerical studies of oscillating flux tubes have established the significance
of resonant absorption in the damping of propagating transverse oscillations in coronal …

Magnetohydrodynamic (MHD) waves permeate the solar atmosphere and constitute
potential coronal heating agents. Yet, the waves detected so far may be but a small subset of …

The recent rediscovery of magnetic field switchbacks or deflections embedded in the solar
wind flow by the Parker Solar Probe mission lead to a huge interest in the modeling of the …

The solar atmosphere is known to be replete with magneto-hydrodynamic wave modes, and
there has been significant investment in understanding how these waves propagate through …

Magnetic twist is thought to play an important role in many structures of the solar
atmosphere. One of the effects of twist is to modify the properties of the eigenmodes of …

Why the atmosphere of the Sun is orders of magnitudes hotter than its surface is a long
standing question in solar physics. Over the years, many studies have looked at the potential …