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Fig. 4.

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Logarithmic density maps in PLUTO units (ρPLUTO = 2.48 × 10−15 g cm−3; left) and logarithmic mass flux maps, also in PLUTO units (ρVPLUTO = 2.75 × 10−8 g cm−2 s−1; right). We plot simulation case D.1 at PLUTO time = 30, 50, 75, and 100. 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.

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