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 …

Hinode is Japan's third solar mission following Hinotori (1981–1982) and Yohkoh (1991–
2001): it was launched on 2006 September 22 and is in operation currently. Hinode carries …

Aims. To demonstrate the capabilities of regularized inversion to recover differential
emission measures (DEMs) from multi-wavelength observations provided by telescopes …

Abstract The Multi-slit Solar Explorer (MUSE) is a proposed mission composed of a multislit
extreme ultraviolet (EUV) spectrograph (in three spectral bands around 171 Å, 284 Å, and …

The physical processes causing energy exchange between the Sun's hot corona and its
cool lower atmosphere remain poorly understood. The chromosphere and transition region …

ABSTRACT The High-resolution Coronal Imager (Hi-C) has provided Fe xii 193Å images of
the upper transition region moss at an unprecedented spatial (∼ 0 farcs 3–0 farcs 4) and …

We present a comprehensive radiative magnetohydrodynamic simulation of the quiet Sun
and large solar active regions. The 197 Mm wide simulation domain spans from 18 (10) Mm …

It is largely agreed that many coronal loops—those observed at a temperature of about 1 MK—
are bundles of unresolved strands that are heated by storms of impulsive nanoflares. The …

The" smoking gun" of small-scale, impulsive events heating the solar corona is expected to
be the presence of hot (> 5 MK) plasma. Evidence for this has been scarce, but has …

We present spatially resolved EUV spectroscopic measurements of pervasive, faint Fe xix
592.2 Å line emission in an active region observed during the 2013 April 23 flight of the …