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Fig. 5

image

Time needed to fully blow out dust particles from when they first enter the wind at twind,0 to the domain boundary, which they reach at tbnd (data points in cyan, mean in blue), and time needed to accelerate dust grains to vr,esc (data points in orange, mean in red); both for a selection of three a0. Keplerian orbital times (tdyn ≡ ΔtK) at the disk surface are included as dashed green lines. The rasterization of the data points results from a time-discrete particle tracking and a binning in R-direction; thus, one raster point may represent multiple data points. (For all a0, see Fig. C.2.)

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