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Magnetic reconnection is a process of fundamental importance for the dynamics of the Earth's plasma sheet. In this context, the development of thin current sheets in the near-Earth plasma sheet is a topic of special interest because they could be a possible cause of microscopic¯uctuations acting as collective non-idealness from a macroscopic point of view. Simulations of the near-Earth plasma sheet including boundary perturbations due to localized in¯ow through the northern (or southern) plasmadoi:10.1007/s005850050787 fatcat:n6kznfbm3jbh3pdevvt2tavn6m