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Magnetic Helicity Flux in the Presence of Shear

  • Authors: Alexander Hubbard and Axel Brandenburg

Hubbard & Brandenburg 2011 The Astrophysical Journal 727 11.

  • Provider: AAS Journals

Caption: Figure 3.

Same as Figure 3, but for Run B: k f/ k 1 = 3, Re = 9, Re M = 90, and Sh = 0.5. In this case, c = 1.04η t0 k 1. The vertical bars in the first panel denote the time interval over which the functions in the other three panels are averaged. Note also that after u rms k f t ≈ 7800 the dominant dynamo mode changes and the field becomes x dependent.

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