Image Details
Caption: Figure 2.
Snapshots of simulations G101Dn5In4 (left), G101Dn6In4 (middle), and G105Dn5In3 (right) at ﹩t=0.4\,{{\rm{\Omega }}}_{{\rm{KH}}}^{-1}﹩. The density distribution (color scale), poloidal velocity field (black arrows), and magnetic field lines (solid white lines) are shown. The scale of the poloidal velocity is shown at the top right of each panel. The magnetic field lines are depicted by the contours of the poloidal magnetic flux at several specific levels. The bottom panels present zoomed-in views of the corresponding top panels. The brown dashed lines mark the disk scale height. The gray meshes illustrate a coarser representation of the numerical grid, with each displayed cell corresponding to a 4 × 4 block of the actual grid cells. Here and throughout, “lg” denotes the base-10 logarithm.
© 2026. The Author(s). Published by the American Astronomical Society.