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Fig. 3.

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Magnetic field configurations: inside the 1.6 Mγ Dor star near ZAMS (a), at mid-MS (b), inside the 5 M SPB near ZAMS (c), at mid-MS (d), and near TAMS (e). Values are normalised by the maximum field amplitude, and mixed poloidal (black lines) and toroidal (colour scale) magnetic fields are modelled using the formalism of Duez & Mathis (2010) (see our Eq. (59)). We focus here on the effects of the toroidal component as discussed in the text.

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