Fig. 2From: Asymmetric deformation of the Earth’s magnetosphere under low Alfvén Mach number solar wind: Observations and MHD simulationGeotail observations from 10:00 to 22:00 UT on February 11, 2007. From the top, a omni-directional electron energy-time spectrogram, b omni-directional ion energy-time spectrogram from LEP-EAi, c ion density for reference (the absolute value is not authorised), d ion temperature, e ion velocity, and f magnetic field. The spacecraft locations in the GSM and GSE coordinate systems are presented at the bottomBack to article page