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Transition to Turbulent Dynamo Saturation

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Academic year: 2021

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Figure

FIG. 2. Snapshots of the saturated state for Pm ¼ 4 . 25 × 10 −5 , γl 2 =η ¼ 5 . 1 × 10 −3 , and Rm ¼ 0
FIG. 3. Magnetic energy as a function of the departure from onset, for several values of the magnetic Prandtl number

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