Solar prominences are one of the most common features of the solar atmosphere. They are
found in the corona but they are one hundred times cooler and denser than the coronal …

Magnetohydrodynamic (MHD) oscillatory processes in different plasma systems, such as the
corona of the Sun and the Earth's magnetosphere, show interesting similarities and …

Magnetic reconnection is a multi-faceted process of energy conversion in astrophysical,
space and laboratory plasmas that operates at microscopic scales but has macroscopic …

In this review, our present day understanding of the Sun's global photospheric and coronal
magnetic fields is discussed from both observational and theoretical viewpoints. Firstly, the …

Prominences are intriguing, but poorly understood, magnetic structures of the solar corona.
The dynamics of solar prominences has been the subject of a large number of studies, and …

Magnetic fields suspend the relatively cool material of solar prominences in an otherwise hot
corona. A comprehensive understanding of solar prominences ultimately requires complex …

Prominences and filaments are manifestations of magnetized, levitated plasma within the
solar coronal atmosphere. Their structure is assumed to be driven by the ambient magnetic …

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

This publication provides an overview of magnetic fields in the solar atmosphere with the
focus lying on the corona. The solar magnetic field couples the solar interior with the visible …

Stellar coronal mass ejections (CMEs) have recently received much attention for their
impacts on exoplanets and stellar evolution. Detecting prominence eruptions, the initial …