Stellar wind characterisation at the optimistic (O_I−HZ, red) and conservative (C_I−HZ, yellow) inner edges of the HZ of HD 22049. Similarly, the 1 AU boundary is used as reference (cyan). In all cases, we consider rings extending to ± 5° in inclination from the equatorial plane (slightly exaggerated in the figure for visualisation purposes). The wind structure is the same as in Fig. 6 (bottom-left), rotated by 90° clockwise.