We introduce how the catastrophe model for solar eruptions predicted the formation and
development of the long current sheet (CS) and how the observations were used to …

Magnetic reconnection is the topological reconfiguration of the magnetic field in a plasma,
accompanied by the violent release of energy and particle acceleration. Reconnection is as …

This review of scaling theories of magnetohydrodynamic (MHD) turbulence aims to put the
developments of the last few years in the context of the canonical time line (from Kolmogorov …

Simulations of particle acceleration in turbulent plasma regions with multiple contracting and
merging (reconnecting) magnetic islands emphasize the key role of temporary particle …

Plasmoid Instability in Evolving Current Sheets and Onset of Fast Reconnection - IOPscience
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Turbulence plays a key role in forming the complex geometry of the large-scale current
sheet (CS) and fast energy release in a solar eruption. In this paper, we present full 3D high …

The plasmoid instability has revolutionized our understanding of magnetic reconnection in
astrophysical environments. By preventing the formation of highly elongated reconnection …

In eruptive solar flares, termination shocks (TSs), formed when high-speed reconnection
outflows collide with closed dense flaring loops, are believed to be one of the possible …

Magnetohydrodynamic turbulence is ubiquitous in the process of solar eruptions, and it is
crucial for the fast release of energy and the formation of complex thermal structures that …

The mechanism that accelerates particles to the energies required to produce the observed
high-energy impulsive emission in solar flares is not well understood. Drake et al. proposed …