Fig. 12
From: 3-D global hybrid simulations of magnetospheric response to foreshock processes
Case II global view of \(N\) at \(t = 100~\Omega _{{i0}}^{{ - 1}}\) in the noon-meridian and equatorial planes, showing the 3-D structures of the global system. The white dashed lines roughly mark the magnetopause and bow shock positions, respectively, and typical magnetic field lines are also displayed. The foreshock disturbances and the magnetosheath density are much weaker compared with Case I