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Three-dimensional, Time-dependent MHD Simulation of Disk–Magnetosphere–Stellar Wind Interaction in a T Tauri, Protoplanetary System

  • Authors: Ofer Cohen, Cecilia Garraffo, Jeremy J. Drake, Kristina Monsch, Igor V. Sokolov, Julián D. Alvarado-Gómez, Federico Fraschetti

Ofer Cohen et al 2023 The Astrophysical Journal 949 .

  • Provider: AAS Journals

Caption: Figure 1.

Top: the grid structure in the simulation displayed on a sphere of r = 1.1R , and on the z = 0, and x = 0 (top left only) slices. The full domain is shown on the top left panel, while the top middle and top right panels show a zoom-in view at different levels, respectively. Bottom: the initial condition of the simulation. The bottom left panel shows a three-dimensional view of the z = 0 and y = 0 slices colored with number density contours, and selected magnetic field lines are shown in gray. The bottom middle and bottom right panels show a similar display of the y = 0 and x = 0 slices, respectively.

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