Fig. 10From: 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, in the \(X=-3.46\) \(R_E\) plane on which Geotail was located. The contours of a plasma density and b the absolute value of current density are shownBack to article page