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Fig. 2

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Measurements of the fraction of solar surface occupied by BPs, FCS, at eight heliocentric positions. Vertical bars represent the errors while horizontal bars show the range of heliocentric positions included in the finite extension of the FOV. The three different curves represent the three different solutions provided by our toy-model – the solid, the dashed, and the dot-dashed lines correspond to models a, b, and c in Table 2, respectively.

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