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Fig. 6.

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Area coverage fraction of Hα deficit regions in percent (left row), the mean intensity of the Hα deficit regions (right row), and the imaging Hα deficit D100 (middle row) averaged for all Carrington rotations during the maximum phase of Solar Cycle 24 (upper column) and the declining phase of Solar Cycle 24 (lower column). The shaded areas indicate the standard deviation. In the middle row, we provide the Spearman correlation coefficient ρD, A of the Hα deficit and the area coverage fraction, the correlation coefficient ρD, I of the Hα deficit and the mean intensity, and the correlation coefficient of the area coverage fraction and the mean intensity ρA, I.

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