Fig. 9From: Asymmetric deformation of the Earth’s magnetosphere under low Alfvén Mach number solar wind: Observations and MHD simulationResults of a global MHD simulation at 14:30 UT. The absolute value of current density a in the XY plane with magnetic field lines and b in the XZ plane are presented. In Panel (b), the Cluster 1 location is shown by a red triangleBack to article page