Comparison of the Stokes number of the dust particles in the CPDs of Jupiter (top) and Saturn (bottom) in the fragmentation limited regime (black solid lines), assuming vf = 1 m s−1 and α = 10−4, and the drift limited regime (black dashed lines), assuming Ṁ0 = 10−9 Mp yr−1 and r0 = 10 RJup∕Sat. The solid and dashed gray curves show the physical sizes of the dust grains in the fragmentation and drift limited regimes, respectively.
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