Selected flow lines near the (B, V) plane for the cases with V = 2 km s⁻¹, B = 7 µG, (model 5, upper panel), and V = 2 km s⁻¹, B =20 µG, (model 17, lower panel). The two-stream structure of the stellar plasma flow (L and R streams) and the possible tail region (T) are indicated. The circles indicate the distances of 2 R_TS, 4 R_TS, and 6 R_TS from the star, where R_TS is the distance to the termination shock.