Slices perpendicular to the disk plane. Left column: density slice in the outflow selection. Middle column: ratio of the Lorentz acceleration to the radiative acceleration. Right column: ratio of the radiative acceleration to the gravitational force. From top to bottom: Run  SUPA (super-Alfvénic, subsonic turbulence, 10 000 AU, t = 67.0 kyr, M = 8.2 M_⊙, L = 1.4 × 10⁴ L_⊙), run SUPAS (super-Alfvénic, supersonic turbulence, 4000 AU, t = 72.6 kyr, M = 5.6 M_⊙, L = 8 × 10³ L_⊙) and run SUBA (sub-Alfvénic, subsonic turbulence, 10 000 AU, t = 61.1 kyr, M = 9.6 M_⊙, L = 1.7 × 10⁴ L_⊙). The gas densities in the left column correspond to particle densities between ~ 10⁴ and ~ 10⁶ cm⁻³.