Dust-void evolution driven by turbulent dust flux can induce runaway migration of Earth-mass planets

Open Access

Fig. A.1

Colatitude resolution ratio for the models with a dust aspect ratio less than 0.1h_g. Note: in the domain between $θ = \frac{π}{2} - 0.01$ $\[\theta=\frac{\pi}{2}-0.01\]$ and $θ = \frac{π}{2}$ $\[\theta= \frac{\pi}{2}\]$ , the resolution is constant and it satisfies the minimum requirement h_d/Δθ = 10.86 in each model.

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