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Nonideal Magnetohydrodynamic Instabilities in Protoplanetary Disks: Vertical Modes and Reflection Asymmetry

  • Authors: Lile Wang, Sheng Xu, Zhenyu Wang, Min Fang, Jeremy Goodman

Lile Wang et al 2024 The Astrophysical Journal 972 .

  • Provider: AAS Journals

Caption: Figure 3.

Nonideal MHD profiles for the fiducial model (Section 4.1) at (R/au) ∈ {0.5, 1, 2} presented in different columns. Top row: the dimensionless diffusivities (α O, α H/b, and α A/b 2) and Elsässer numbers (ΛO, ΛH, Am). Bottom row compares the key MHD profiles (ϱ, b R , b φ , μ R ) of the semi-analytic solutions to the simulation results (marked with “(Sim.)”) used in Nemer et al. (2020), Fang et al. (2023b). Note that, in the bottom row, different physical quantities are distinguished by colors, while dashed and solid line shapes indicate negative and positive values, respectively.

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