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 …

Energetic particle fluxes in the outer zone radiation belts can vary over orders of magnitude
on a variety of timescales. Power at ULF frequencies, on the order of a few millihertz, have …

ABSTRACT Motivated by recent Transition Region and Coronal Explorer (TRACE)
observations of damped oscillations in coronal loops, we consider analytically the motion of …

The present 15th volume of the ISSI Space Science Series is devoted to Auroral Plasma
Physics. The aurora is arguably the most intriguing phenomenon in space plasma physics …

Ultra low frequency (ULF) waves incident on the Earth are produced by processes in the
magnetosphere and solar wind. These processes produce a wide variety of ULF …

Recent observations have indicated that in addition to the classical “inverted‐V” type
electron acceleration, auroral electrons often have a field‐aligned distribution that is broad …

We report in situ observations from the Cluster and FAST spacecraft showing the deposition
of energy into the auroral ionosphere from broadband ULF waves in the cusp and low …

Observations have revealed ubiquitous transverse velocity perturbation waves propagating
in the solar corona. However, there is ongoing discussion regarding their interpretation as …

Context. Kink oscillations are ubiquitously observed in solar coronal loops, and
understanding them is crucial in the contexts of coronal seismology and atmospheric …

Recent numerical studies revealed that transverse motions of coronal loops can induce the
Kelvin–Helmholtz instability (KHI). This process could be important in coronal heating …