Plasma flow across the cusp-magnetosheath boundary under northward IMF

In this paper, we have used two closely spaced (INTERBALL-1 and MAGION-4) satellites orbiting in the region adjacent to the magnetopause with motivation to determine the structure of the cusp-magnetosheath boundary under steady solar wind conditions and under the northward interplanetary magnetic field (IMF). Two-point observations reveal that a steady reconnection takes place tailward of the cusp and the position of the reconnection site moves in accordance with the actual IMF direction. Reconnection produces a latitudinally dispersed cusp precipitation with highest energies in the cusp poleward edge. The reconnection site is widely spread in local time and thus changes of the IMF By component only slightly modulate observed patterns. The change of the plasma flow direction suggests the presence of the vortex-like structure in the exterior cusp.