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Fig. 1.
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Line-center image of the 5 × 5 × 5 Mm3 model prominence just above the solar limb used in this paper, observed from Earth with a FOV of 20″ × 20″, at the line center of the academic line at 5000 Å. The disk illumination is given by the disk center intensity and center-to-limb variation in Allen (1976).
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