Dust polarization radiative transfer results performed at λ = 0.87 µm with f_high−J = 1.0, L_★=100 L_⊙, and a_max = 10 µm, after spatial filtering with the CASA simulator, mimicking ALMA interferometric observations. Top panel: synthetically observed dust continuum total intensity (Stokes I, color scale) plotted with the velocity field of the central slice in the MHD simulation (white arrows) and the density-weighted magnetic field lines (yellow lines). Stokes I is shown when I >3 σ_I, where σ_I = 0.10 mJy beam⁻¹. Bottom panel: the color scale is the total linearly polarized intensity, which is shown where Ρ>3 σ_P, where σ_Ρ = 10 µJy beam⁻¹. The line segments represent the magnetic field orientations inferred from the dust polarization map. They are plotted where Ρ > 5 σ_Ρ. The white circle at the bottom-left corner is the resolution of the ALMA synthetic observations and is 100 au in size.