Fig. 2From: Anisotropy evolution of magnetic field fluctuation through the bow shockTime series plots of the magnetic field magnitude observed by Cluster-1 for orbit A (top, quasi-parallel shock crossing) and B (bottom, quasi-perpendicular shock crossing). Intervals 1,..., 6 represent the solar wind, the foreshock, the magnetosheath, the solar wind, the magnetosheath, and the cusp region that are used for the analysis, respectively.Back to article page