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A statistical study on the current sheet shows that there are different types of the current sheets.
The thickness of the current sheets changes from 1 to 40 magnetosheath-proton thermal gyro-radii.
Its magnetic topology is dominated by strong multipole components and multiple current sheets.
Thus, Alfvén instability should dominate ion acoustic instability in thin current sheets.
The phase portraits in single- and double-humped current sheets are not strictly identical though.
We devote our attention to the formation of very thin current sheets (TCSs) in the magnetotail.
We model the solar wind as multiple cells separated by current sheets.
The simulations show the formation of current sheets, with the current density increasing exponentially in time.
The adaptive procedure is applied to study singular current sheets in the tilt instability problem of ideal magnetohydrodynamics. Numerical results indicate a more accurate resolution of current sheets with higher-order methods than with piecewise-linear approximations.
The elements structuring the CCP i.e., current sheets, magnetic ropes, magnetic islands appear as the result of the electromagnetic (e.m).m
Recently Li et al. (2011) proposed that the presence of current sheets may be the cause of the Kolmogorov scaling.
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