Ultimate large-Rm regime of the solar dynamo | Astronomy & Astrophysics (A&A)

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Fig. 1.

Butterfly diagrams ${\bar{B}}_{x} (z, t)$ $Mathematical equation: $ {\overline{B}}_{x}(z,t) $$ of large-scale non-linear helical dynamo modes vs Re and Rm. Run S01 (Pm = 0.5) is the rightmost plot; run T06 (Pm = 4) of R21 is the topmost plot. The parameter range spanned is shown at the bottom right. The same colour scale is used in all plots.

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