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Fig. 9


View of the magnetic power from the night side of the exoplanet for different IMF orientations and exoplanet magnetic axis tilts. The color bars of the model tilt90 for the Bx–Bxneg IMF orientations are different from those in the rest of the panels. The plotted surface is defined between the bow shock and the magnetopause where the magnetic power reaches its maxima.

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