The influence of small bipolar magnetic regions on basic solar quantities

Open Access

Fig. 10.

Estimating the toroidal flux loss and the toroidal flux loss noise. (a) Integrand of Eq. (35) (green solid) and the tangent power law at the steepest point (blue dashed). (b) Same but for the integrand of Eq. (36). The vertical grey lines marks the lower flux limits of AMR and LMR.

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