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Figure 4
(a) Calculated X-ray reflectivity of a 300 nm Au-coated mirror as a function of the photon energy at different grazing-incidence angles. The open circles show the critical energies. (b) Critical angle for the Au mirror as a function of the photon energy. (c) Calculated total flux (0.5–30 keV) of the BIB, and with 1 m of air, and reflected by the Au-coated mirror at different incidence angles.

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SYNCHROTRON
RADIATION
ISSN: 1600-5775
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