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Fig. 2


Cut from a 3D MHD simulation showing the log of the solar wind number density (cm-3), the velocity (km s-1), the log of thermal pressure (dyn/cm2), and the magnitude of the magnetic field (nT) in the Oz-V2 plane. The plots show the formation of a forward-reverse shock pair that propagates along the Voyager 2 direction (dashed white line). The forward shock (FS), reverse shock (RS), and termination shock (TS) are denoted. Black boundaries show the regions of the grid refinement.

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