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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 2.

Mean toroidal field as a function of latitude and time as in Figure 1(d) (same radial level, color scale, saturation ±4 kG) with (a) α 0 = 1 m s −1, (b), (c) α 0 = 10 m s −1, and (d), (e) α 0 = 100 m s −1. Frame (c) represents a continuation of frame (b) at much later times. Frame (e) is a zoomed-in portion of frame (d) highlighting the magnetic cycles.

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