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Fig. 7

image

View of the magnetic power from the night side of the exoplanet for different IMF orientations and exoplanet magnetic field topologies (different dipolar-to-quadrupolar component ratios). The first color bar is related to the Bx–Bxneg IMF orientations, and the second color bar is related to the other IMF orientations. The plotted surface is defined between the bow shock and the magnetopause where the magnetic power reaches its maxima.

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