Simulation case D.2, which is representative of the second solution type. Panel a shows the logarithmic density map in PLUTO units (ρ_PLUTO = 2.48 × 10⁻¹⁵ g cm⁻³) and panel b the logarithmic mass flux map, also in PLUTO units (ρV_PLUTO = 2.75 × 10⁻⁸ g cm⁻² s⁻¹). The velocity vectors are shown as black arrows, and the magnetic field lines are represented by the solid white lines. The distances on the vertical (z) and horizontal (ϖ) axis are represented in astronomical units. The plot refers to PLUTO time = 30, which corresponds to 3.6 stellar rotations.