Fig. D.1
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Hα amplitude (right panels) versus inclination due to plages (solid line) and filaments (dashed line), and ratio between plage and filament amplitudes (left panels) for different configurations: average solar latitude (LT1 in Table 6) and r=10 (upper panels), stronger latitude differences (LT2) and r=10 (middle panels), and average solar latitude and r=1 (lower panels).
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