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Fig. 1


Modulus of the horizontal components ξθ (left panels) and ξϕ(right panels) of the displacement vector versus θ/π at some radial meshpoints in the intermediate region outside the convective core (upper panels) and near the stellar surface, including the convective shell, (lower two panels) for a (200) g-mode with frequency 1.713 cpd in the inertial frame. The arrow indicates the critical (co)latitude θc.

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