Image Details
Caption: Figure 5.
Vorticity magnitude in the protolunar disk midplane at ∼180 hr post-impact for models with linear resolution Δx ≃ 175 km and initial field strengths (a) B0 ≃ 1 μG and (b) B0 ≃ 1 kG. Evidently the weak field model is nearly laminar, while the strong field model is turbulent.
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