Fig. 2.

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Magnetometer data, all three components and magnitude and the radial distance from Venus in VSO coordinates. The dashed vertical line is the time of the bow shock crossing, the dotted vertical lines show the region ±1 RV. The blue shaded intervals indicate where the field has the direction of the upstream solar wind. The colouring of the traces is according to which activity is observed in the magnetic field, as in Fig. 1.

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