Astrophysical plasmas have the remarkable ability to preserve magnetic topology, which
inevitably gives rise to the accumulation of magnetic energy within stressed regions …

Modes and manifestations of the explosive activity in the Earth's magnetotail, as well as its
onset mechanisms and key pre-onset conditions are reviewed. Two mechanisms for the …

Coronal mass ejections (CMEs) and solar flares are the large-scale and most energetic
eruptive phenomena in our solar system and able to release a large quantity of plasma and …

The violent disruption of the coronal magnetic field is often observed to be restricted to the
low corona, appearing as a confined eruption. The possible causes of the confinement …

Magnetic flux ropes are characterized by coherently twisted magnetic field lines, which are
ubiquitous in magnetized plasmas. As the core structure of various eruptive phenomena in …

Solar eruptions, observed as flares and coronal mass ejections (CMEs), are the most
energetic visible plasma phenomena in the solar system. CMEs are the central component …

Solar flares are spectacular coronal events that release large amounts of energy. They are
classified as either eruptive or confined,, depending on whether they are associated with a …

Magnetic flux rope (MFR) is the core structure of the greatest eruptions, that is, the coronal
mass ejections (CMEs), on the Sun, and magnetic clouds are posteruption MFRs in …

The magnetic flux rope is among the most fundamental magnetic configurations in plasma.
Although its presence after solar eruptions has been verified by spacecraft measurements …

On 2017 September 6, the solar active region 12673 produced an X9. 3 flare, regarded to be
the largest to have occurred in solar cycle 24. In this work we have performed a …