The application of machine learning in solar physics has the potential to greatly enhance our
understanding of the complex processes that take place in the atmosphere of the Sun. By …

Strong solar flares and coronal mass ejections, here defined not only as the bursts of
electromagnetic radiation but as the entire process in which magnetic energy is released …

Context. The heating of the solar corona by small heating events requires an increasing
number of such events at progressively smaller scales, with the bulk of the heating occurring …

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

We present a new version of the MURaM radiative magnetohydrodynamics (MHD) code that
allows for simulations spanning from the upper convection zone into the solar corona. We …

X-ray and ultraviolet (UV) observations of the outer solar atmosphere have been used for
many decades to measure the fundamental parameters of the solar plasma. This review …

Magnetic reconnection is a key mechanism involved in solar eruptions and is also a prime
possibility to heat the low corona to millions of degrees. Here, we present ultra-high …

Solar coronal loops are the building blocks of the solar corona. These dynamic structures
are shaped by the magnetic field that expands into the solar atmosphere. They can be …

Coronal plumes are long, ray-like, open structures that have been considered as possible
sources of the solar wind. Their origin in the largely unipolar coronal holes has long been a …

We present a case study for the global extreme-ultraviolet (EUV) wave and its
chromospheric counterpart the Moreton-Ramsey Wave associated with the second X-class …