Fig. 6.
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Top row: Magnetograms of the radial magnetic field components from (left to right) 2019.4, 2019.9, 2020.1, 2020.6, 2022.9. Middle row: Radial wind velocity in the equatorial plane, produced using the above ZDI maps. The white contour is the intersection of the Alfvén surface with the equatorial plane. We note that the scale of this plot is too small to include the orbital distance of the habitable zone. Bottom row: Radial wind velocity in the planetary frame. Wind velocity values are presented for two estimates for the habitable zone of AD Leo: 102 R* (dotted line) and 81 R* (solid line).
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