Fig. 1
Distribution of the specific turbulent torque exerted on a 3 M⊕ planet obtained from a turbulent simulation in which the turbulent potential of Eq. (7) with γ = 10-4 is applied to the disc (solid line), and obtained from a laminar simulation in which the turbulent force of Eq. (10) with C = 17 is applied to the planet (dashed line).
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