Fig. C.1.
Second-order Fourier series models fitted to 100 sub-epochs of SMEI data, cf. Sect. 4.2. Insufficient data were available for the 27th epoch. Peak-to-peak amplitudes are indicated in each panel. Time increases across the figure from left to right and top to bottom. In each panel, observation dates are grayscaled from white to black. The ordinate (SMEI magnitude) and abscissa (phase) ranges are −0.05 to 0.05 mag and −0.1 to 1.1, respectively, in all panels.
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