Fig. 6
Central slices of a) the OFP Φ•(r) and b) the solar disc B⊙(r), showing the center-to-limb variation normalized to 1 at the center. Parameters used here are: circular occulter of 1.5 m diameter, central dark zone of 0.2 m, distance from the occulter of 139.6 m and wavelength of 0.55 μm.
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