Fig. 3

Computed aperture diffraction PSF at λ = 3000 Å, source at infinity, of a grazing-incidence parabolic mirror with f = 10 m, a minimum radius R0 = 150 mm, and a length L1 = 300 mm, resulting in a circular corona aperture of 2.25 mm width. The dashed line is the usual diffraction pattern of a straight slit of equal width, while the accurate computation (solid line) is obtained by computing the exact diffraction pattern integrated over circular coronae. A high-frequency modulation in the latter would also be superimposed owing to the diffraction of the 2R0 diameter circular aperture, but in real cases is canceled out by the finite resolution of the detector.
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