Dust dynamics in current sheets within protoplanetary disks - I. Isothermal models including ambipolar diffusion and Ohmic resistivity

Open Access

Fig. 2

Edge-on slices of the relative dust fraction variations for O10A10 (fiducial run), O1A1, O10A1 and O1A10 (more resistive runs), from left to right. The slices are displayed at t ~ 8 yr (~50 Ω⁻¹), except for run O 10A10BETA7500 for which they are displayed at t ~ 32 yr (~200 Ω⁻¹). The dust grain size increases from top to bottom.

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