In a thin elongated current sheet, it is likely that more than one X-line forms and thus multiple magnetic islands are produced. The islands are then subject to merging. By simulating such a case with a two-dimensional full-particle code, we show that a merger forming a large island produces the most energetic electron population in the system. By setting the lateral extent of the simulation box to be as large as ∼ 100 ion inertial lengths, we introduce many (16) small islands in the initial thin current sheet ( ∼ 1 ion inertial length thickness). Merging of these islands proceeds to leave only two islands in the system. Then, strong electron acceleration is seen upon the final merger that produces the single island in the large simulation ...
Aims. Magnetic reconnection in large Harris-type reconnecting current sheets (RCSs) with a single X-...
The role of magnetic islands in collisionless driven reconnection has been investigated from the sta...
We present observations in Earth's magnetotail by the Magnetospheric Multiscale spacecraft that are ...
The system size dependence of electron acceleration during large-scale magnetic island coalescence i...
Aims. Magnetic reconnection in large Harris-type reconnecting current sheets (RCSs) with a single X-...
Magnetic reconnection is a fundamental plasma process. Recent theoretical studies and numerical simu...
Using analytical and numerical methods (fluid and particle-in-cell simulations) we study a number of...
Context. Charged particles are accelerated to high energies in solar flares. Although we know that m...
Magnetic reconnection converts magnetic energy into particle kinetic energy, and satellite observati...
Aims. Particles are known to have efficient acceleration in reconnecting current sheets with multipl...
We present an analysis of the electron dynamics during rapid island merging in asymmetric magnetic r...
Electron acceleration in a drastically evolved current sheet under solar coronal conditions is inves...
The mechanism that accelerates particles to the energies required to produce the observed high-energ...
This paper identifies the non-equilibrium evolution of magnetic field structures at the onset of lar...
Aims. Magnetic reconnection in large Harris-type reconnecting current sheets (RCSs) with a single X-...
Aims. Magnetic reconnection in large Harris-type reconnecting current sheets (RCSs) with a single X-...
The role of magnetic islands in collisionless driven reconnection has been investigated from the sta...
We present observations in Earth's magnetotail by the Magnetospheric Multiscale spacecraft that are ...
The system size dependence of electron acceleration during large-scale magnetic island coalescence i...
Aims. Magnetic reconnection in large Harris-type reconnecting current sheets (RCSs) with a single X-...
Magnetic reconnection is a fundamental plasma process. Recent theoretical studies and numerical simu...
Using analytical and numerical methods (fluid and particle-in-cell simulations) we study a number of...
Context. Charged particles are accelerated to high energies in solar flares. Although we know that m...
Magnetic reconnection converts magnetic energy into particle kinetic energy, and satellite observati...
Aims. Particles are known to have efficient acceleration in reconnecting current sheets with multipl...
We present an analysis of the electron dynamics during rapid island merging in asymmetric magnetic r...
Electron acceleration in a drastically evolved current sheet under solar coronal conditions is inves...
The mechanism that accelerates particles to the energies required to produce the observed high-energ...
This paper identifies the non-equilibrium evolution of magnetic field structures at the onset of lar...
Aims. Magnetic reconnection in large Harris-type reconnecting current sheets (RCSs) with a single X-...
Aims. Magnetic reconnection in large Harris-type reconnecting current sheets (RCSs) with a single X-...
The role of magnetic islands in collisionless driven reconnection has been investigated from the sta...
We present observations in Earth's magnetotail by the Magnetospheric Multiscale spacecraft that are ...