Longitude-latitude distributions of the flow lines crossing points on the sphere with a radius of 300 AU and the centre at the host star for two cases with low inflow speed: V = 0.5 km s⁻¹, n_H,IS = 0.1 cm⁻³ (model 4, upper panel), V = 2km s⁻¹, n_H,IS =0.1 cm⁻³ (model 5, lower panel). B = 7 µG in all cases. Crossed lines show the direction and anti-direction of the interstellar field.