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Convective Babcock-Leighton Dynamo Models

  • Authors: Mark S. Miesch and Benjamin P. Brown

Miesch & Brown 2012 The Astrophysical Journal Letters 746 L26.

  • Provider: AAS Journals

Caption: Figure 3.

Parity of the mean toroidal field as a function of time for the simulation shown in Figures 2(d) and (e) (α 0 = 100 m s −1).

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