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Figure 7
Characterization of the horizontal mirror with the ZYGO white-light interferometer. This picture shows the power spectral density of the microroughness in the spatial range between 1 mm and 1.5 µm of the vertical mirror. The red line represents the best fit obtained with a power-law curve PSD(f) ≃ Knf−n.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 26| Part 5| September 2019| Pages 1462-1472
https://doi.org/10.1107/S1600577519007938
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