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Fig. 22

image

Babcock-Leighton-type dynamo solutions with the same setup as in Fig. 21, but for the low turbulent magnetic diffusivity ηT = 1011 cm2/ s. Left: classical solar case with a poloidal-field generation by active regions at low latitudes. Right: observationally driven case with a poloidal-field generation around 70° latitudes.

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