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Fig. A.1.

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Family of azimuthal velocity profiles for the solar wind, derived using different hybrid velocity profiles (vr) and for a range of Alfvén point locations as indicated by the colorbar on the right. (Top left) Azimuthal velocity profiles using a hybrid velocity profile with rs = 0.1. (Top right) Azimuthal velocity profiles using a hybrid velocity profile with rs = 2.7. (Bottom left) The same family of profiles as the top right panel but including earlier measurements of vϕ as indicated in the legend. (Bottom right) The same as bottom left but including newer measurements of vϕ from Parker Solar Probe. The black rectangle indicates the field of view of the plot on the left.

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