Review Article

Kirkpatrick-Baez (KB) and Lobster Eye (LE) Optics for Astronomical and Laboratory Applications

Figure 30

Intensity distribution in the focal plane ( 1 5 × 1 5  mm detector) for the 2 3 × 2 3  mm Schmidt objective, mathematical raytracing for micro roughness rms = 1 nm and wavelength = 1 nm.
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