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

<table>(a) The X-ray reflectivity measurements of 0.1 mm float glass plate  (used in the <svg height="9.9499998" id="M77" 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">2</tspan>
<tspan style="font-size: 11.21px; " x="5.6040001" y="0">3</tspan>
<tspan style="font-size: 11.21px; " x="13.696176" y="0">×</tspan>
<tspan style="font-size: 11.21px; " x="23.357471" y="0">2</tspan>
<tspan style="font-size: 11.21px; " x="28.961472" y="0">3</tspan>
</text>
</g>
</g>
</svg> mm Schmidt objective). Au/NiCr layers coated the reflecting surfaces. (b) The X-ray reflectivity measurements for BOROFLOAT 1.1 mm thick flat sample (with no additional layers).</table>

X-Ray Optics and Instrumentation

fig31

Figure 31

Figure 31: Kirkpatrick-Baez (KB) and Lobster Eye (LE) Optics for Astronomical and Laboratory Applications 