Fig. 11From: Asymmetric deformation of the Earth’s magnetosphere under low Alfvén Mach number solar wind: Observations and MHD simulationCluster 1 and 3 observations from 13:30 to 17:00 UT on February 11, 2007, including southern high-latitude magnetopause encounters. From the top, a omni-directional ion energy-time spectrogram, b omni-directional electron energy-time spectrogram, c ion density, d ion temperature, e ion velocity, f magnetic field from Cluster 1. g–l Data from Cluster 3 are plotted in the same formatBack to article page