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Fig. 6


Meridional cuts in the Oz-V2 plane from a 3D MHD simulation showing the distribution of the solar wind density (cm-3) for different times when the interaction region propagates in the heliosheath. The plot a) corresponds to the moment of time t = 1 yr; b) t = 1.1 yr; c)t = 1.2 yr; and d) t = 1.3 yr.

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