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Magnetic Reconnection at Planetary Bodies and Astrospheres
Magnetic reconnection is a fundamental mechanism for the transport of mass and energy in planetary magnetospheres and astrospheres. While the process...
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Magnetic Reconnection and Associated Particle Acceleration in High-Energy Astrophysics
Magnetic reconnection occurs ubiquitously in the universe and is often invoked to explain fast energy release and particle acceleration in...
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Magnetic reconnection: MHD theory and modelling
In this review we focus on the fundamental theory of magnetohydrodynamic reconnection, together with applications to understanding a wide range of...
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Laboratory Study of Collisionless Magnetic Reconnection
A concise review is given on the past two decades’ results from laboratory experiments on collisionless magnetic reconnection in direct relation with...
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Particle Acceleration by Magnetic Reconnection in Geospace
Particles are accelerated to very high, non-thermal energies during explosive energy-release phenomena in space, solar, and astrophysical plasma...
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Global-Scale Processes and Effects of Magnetic Reconnection on the Geospace Environment
Recent multi-point measurements, in particular from the Magnetospheric Multiscale (MMS) spacecraft, have advanced the understanding of micro-scale...
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Dimensionality of solar magnetic reconnection
Solar flares are the best examples of astrophysical magnetic reconnection in which the reconnection structure can be studied in detail. The structure...
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Recent progress on magnetic reconnection by in situ measurements
In the last decades, a few spacecraft missions have been launched to investigate the process of magnetic reconnection in space, during which magnetic...
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Turbulent magnetic reconnection generated by intense lasers
Turbulent magnetic reconnection is believed to occur in astrophysical plasmas, and it has been suggested to be a trigger of solar flares. It often...
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First-principles theory of the rate of magnetic reconnection in magnetospheric and solar plasmas
The rate of magnetic reconnection is of the utmost importance in a variety of processes because it controls, for example, the rate energy is released...
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Kinetic Alfven wave (KAW) eigenmode in magnetosphere magnetic reconnection
One prominent signature of collisionless magnetic reconnection in the magnetosphere is the Hall effect. In the ion-scale region of reconnection, ions...
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Direct observation of turbulent magnetic reconnection in the solar wind
Magnetic reconnection in a current sheet is commonly found in astrophysical plasma environments. If it is often bursty, releasing magnetic free...
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Enhancement of Energetic-Electron Population During Magnetic Reconnection Associated with Strong Tearing Mode in Non-Disruptive HL-2A Plasmas
AbstractLaboratory observations of enhancements of energetic-electron population are presented during magnetic reconnection associated with strong...
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Magnetic reconnection in the era of exascale computing and multiscale experiments
Astrophysical plasmas have the remarkable ability to preserve magnetic topology, which inevitably gives rise to the accumulation of magnetic energy...
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Kinetic properties of collisionless magnetic reconnection in space plasma: in situ observations
In collisionless plasmas, magnetic reconnection is widely recognized as one of the most important energy conversion and dissipation processes....
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Study of Reconnection Dynamics and Plasma Relaxation in MHD Simulation of a Solar Flare
Self-organization in continuous systems is associated with dissipative processes. In particular, for magnetized plasmas, it is known as magnetic...
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The origin of underdense plasma downflows associated with magnetic reconnection in solar flares
Magnetic reconnection is a universal process that powers explosive energy-release events such as solar flares, geomagnetic substorms and some...
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CME-Flare Association and the Role of Reconnection in CME Acceleration
The association of coronal mass ejections (CMEs) with flares is related to the question of whether reconnection is necessary for the CME eruption....
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Energy extraction via magnetic reconnection in Lorentz breaking Kerr–Sen and Kiselev black holes
Black holes can accumulate a large amount of energy, responsible for highly energetic astrophysical phenomena. Although the Blandford–Znajek is...
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Energy Spectra vs. Element Abundances in Solar Energetic Particles and the Roles of Magnetic Reconnection and Shock Acceleration
We reexamine the relationship between energy spectral indices and element abundance enhancements in solar energetic particle (SEP) events at energies...
