Coronal loops are the building blocks of the X-ray bright solar corona. They owe their
brightness to the dense confined plasma, and this review focuses on loops mostly as …

Observations and models of solar prominences are reviewed. We focus on non-eruptive
prominences, and describe recent progress in four areas of prominence research:(1) …

Aims. Solar Orbiter, the first mission of ESA's Cosmic Vision 2015–2025 programme and a
mission of international collaboration between ESA and NASA, will explore the Sun and …

The corona is a layer of hot plasma that surrounds the Sun, traces out its complex magnetic
field, and ultimately expands into interplanetary space as the supersonic solar wind …

Observed in cool chromospheric lines, such as Hα or Ca ii H, coronal rain corresponds to
cool and dense plasma falling from coronal heights. Considered as a peculiar sporadic …

Abstract The Atacama Large Millimeter/submillimeter Array (ALMA) is a new powerful tool for
observing the Sun at high spatial, temporal, and spectral resolution. These capabilities can …

The solar corona produces coronal rain, hundreds of times colder and denser material than
the surroundings. Coronal rain is known to be deeply linked to coronal heating, but its origin …

Adopting the MPI-AMRVAC code, we present a 2.5-dimensional magnetohydrodynamic
simulation, which includes thermal conduction and radiative cooling, to investigate the …

We analyze coordinated observations of coronal rain in loops, spanning chromospheric,
transition region (TR), and coronal temperatures with sub-arcsecond spatial resolution …

We investigate the process of formation and subsequent evolution of prominence plasma in
a filament channel and its overlying arcade. We construct a three-dimensional time …