Vertical dust structure as a function of radius for the high-resolution 2D r – z inviscid disk simulation with ϵ₀ = 0.01 and dust inflow at t = 1000 P_orb. The top panel shows a broader radial region, while the bottom panel shows a zoomed-in view of the dust ring region. In the top panel, the outer edge of the dust ring is indicated with a dashed red line. Each set of panels (from left to right) shows: the dust density, radial gas velocity, vertical gas velocity (both normalized by the azimuthal Keplerian velocity), and dust density overlaid with the vertical gas velocity.