The corona of the Sun is a unique environment in which magnetohydrodynamic (MHD)
waves, one of the fundamental processes of plasma astrophysics, are open to a direct study …

Solar eruptive phenomena embrace a variety of eruptions, including flares, solar energetic
particles, and radio bursts. Since the vast majority of these are associated with the eruption …

We present EUV solar observations showing evidence for omnipresent jetting activity driven
by small-scale magnetic reconnection at the base of the solar corona. We argue that the …

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 …

This paper outlines the current understanding of solar flares, mainly focused on
magnetohydrodynamic (MHD) processes responsible for producing a flare. Observations …

Solar eruptions are spectacular magnetic explosions in the Sun's corona, and how they are
initiated remains unclear. Prevailing theories often rely on special magnetic topologies that …

Solar X-ray jets are thought to be made by a burst of reconnection of closed magnetic field at
the base of a jet with ambient open field,. In the accepted version of the 'emerging …

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 …

This review article summarizes the advancement in the studies of Earth-affecting solar
transients in the last decade that encompasses most of solar cycle 24. It is a part of the effort …

We intend to provide a comprehensive answer to the question on whether all Coronal Mass
Ejections (CMEs) have flux rope structure. To achieve this, we present a synthesis of the …