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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 11.

Time evolution of the integrated different components of the magnetic field on the equatorial plane. Left: the individual components of the field: radial (B r , solid black), vertical (B θ , dashed black), azimuthal (B ϕ , dotted black), and total (solid red). Right: the ratio of the individual components.

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