We review the presence and signatures of the non-equilibrium processes, both non-
Maxwellian distributions and non-equilibrium ionization, in the solar transition region …

We report on the structure and evolution of a current sheet that formed in the wake of an
eruptive X8. 3 flare observed at the west limb of the Sun on 2017 September 10. Using …

An important aspect of solar energetic particle (SEP) events is their source populations.
Elemental abundance enhancements of impulsive SEP events, originating in presumed …

In situ measurements of interplanetary coronal mass ejection (ICME) composition, including
elemental abundances and charge states of heavy ions, open a new avenue to study …

On 2017 September 10, a major eruption on the west solar limb produced a class X-8.2 flare
and a superfast coronal mass ejection (CME). During the eruptive process, the geometric …

A small number of interplanetary coronal mass ejections (ICMEs) have been identified that
contain measurable contributions from prominence plasma. In situ measurements from …

After the peak intensity of many large solar flares, magnetic and thermodynamic processes
give rise to a phenomenon known as supra-arcade downflows (SADs). SADs are sunward …

As one of the most spectacular energy release events in the solar system, solar flares are
generally powered by magnetic reconnection in the solar corona. As a result of the re …

The intensity of the O iv 2s 2 2p 2 P–2s2p 2 4 P and S iv 3 s 2 3p 2 P–3s 3p 2 4 P
intercombination lines around 1400 Å observed with the Interface Region Imaging …

The excess broadening of high-temperature spectral lines, long observed near the tops of
flare arcades, is widely considered to result from magnetohydrodynamic turbulence …