Impact of embedded circumplanetary winds on the circumstellar disk - I. Reshaping the local accretion environment

Open Access

Fig. A.1

Reference frames used for the wind parameterization. The global frame S (black) is the inertial frame centered on the star. The comoving frame S′ (blue) is centered on the planet. The wind is defined in frame S″ (red), which is rotated from S′ so that its ${\hat{z}}^{''}$ $Mathematical equation: ${\hat z^{\prime \prime }}$$ -axis aligns with the wind’s primary direction, represented by the vector Γ.

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