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The current sheet creation above the preflare active region 20 MAY, 1991 has been numerically simulated in 3D MHD approximation.
Yoo, J. et al. Laboratory study of magnetic reconnection with a density asymmetry across the current sheet.
In recent years the Current Sheet Disruption model has been proposed as an alternative.
One of the important parameters in magnetotail studies is the thickness of the current sheet.
The simulation also features wave-like structure across the current sheet.
Therefore the whistler-mode waves can grow quickly in the current sheet.
Disruption of the current sheet was observed in the same region.
The first step is acceleration by the strong electric field present inside the current sheet.
The performance of the present code is evaluated for the simulations of the current sheet evolution.
In the reconnection layer, the thickness of the current sheet becomes comparable to the ion skin depth as well as the ion gyro-radius1,2.
Using a 2.5-D particle-in-cell (PIC) model of the current sheet it is shown that due to the tearing mode instability the current sheet tears into plasmoids and these plasmoids later on coalesce into larger ones.
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