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

<table>Intensity distribution in the focal plane (<svg height="9.9499998" id="M66" style="vertical-align:-0.28125pt" version="1.1" viewbox="0 0 43.337502 9.9499998" width="43.337502" xmlns="http://www.w3.org/2000/svg">
<g transform="matrix(1.25,0,0,-1.25,0,9.95)">
<g transform="translate(72,-64.04)">
<text transform="matrix(1,0,0,-1,-71.95,64.37)">
<tspan style="font-size: 11.21px; " x="0" y="0">4</tspan>
<tspan style="font-size: 11.21px; " x="5.6040001" y="0">0</tspan>
<tspan style="font-size: 11.21px; " x="13.696176" y="0">×</tspan>
<tspan style="font-size: 11.21px; " x="23.357471" y="0">4</tspan>
<tspan style="font-size: 11.21px; " x="28.961472" y="0">0</tspan>
</text>
</g>
</g>
</svg> mm detector) according to mathematical ray-tracing for the identical test module and test arrangement as given above; the microroughness of reflecting surfaces are assumed to be 1 nm.</table>

X-Ray Optics and Instrumentation

fig27

Figure 27

Figure 27: Kirkpatrick-Baez (KB) and Lobster Eye (LE) Optics for Astronomical and Laboratory Applications 