Coronal jets represent important manifestations of ubiquitous solar transients, which may be
the source of significant mass and energy input to the upper solar atmosphere and the solar …

Magnetic waves are a relevant component in the dynamics of the solar atmosphere. Their
significance has increased because of their potential as a remote diagnostic tool and their …

Abstract The Solar Upper Transition Region Imager (SUTRI) onboard the Space Advanced
Technology demonstration satellite (SATech-01), which was launched to a Sun …

In the lower solar atmosphere, the chromosphere is permeated by jets known as spicules, in
which plasma is propelled at speeds of 50 to 150 kilometers per second into the corona. The …

As the interface between the Sun's photosphere and corona, the chromosphere and
transition region play a key role in the formation and acceleration of the solar wind …

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

Modern observatories have revealed the ubiquitous presence of magnetohydrodynamic
waves in the solar corona. The propagating waves (in contrast to the standing waves) are …

Spicules are rapidly evolving fine-scale jets of magnetized plasma in the solar
chromosphere. It remains unclear how these prevalent jets originate from the solar surface …

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 …

The European Solar Telescope (EST) is a project aimed at studying the magnetic
connectivity of the solar atmosphere, from the deep photosphere to the upper …