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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 2.

Panel 1: visualization of h f as a function of normalized t and zct for Run A: k f/ k 1 = 5, Re = 0.4, Re M = 9, and Sh = 0.95. Here c = 0.6η t0 k 1 is the actual speed of the dynamo wave. Panels 2–4 give the z dependence of h f, for i = x, y, and the z-component of , averaged in the comoving frame over the time of the first panel.

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