Fig. 2

Velocity streamlines for the two MHD simulations in Li et al. (2013). The simulations are rendered with paraview (http://www.paraview.org). Left: 3D MHD simulation of a collapsing uniform sphere with the magnetic field vector perpendicular to the rotation axis. Right: The simulation with magnetic field vector aligned with the rotation axis. The color of the arrows indicate the azimuthal velocity vector, υφ, in km s-1. The solid black arrows indicate the general stream lines in the two simulations. The dark shaded colors indicate the density isocontours of nH2 = 107.5 cm-3 up to 1010.5 cm-3 (red).
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