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A Magnetized, Moon-forming Giant Impact

  • Authors: P. D. Mullen, and C. F. Gammie

2020 The Astrophysical Journal Letters 903 L15.

  • Provider: AAS Journals

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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