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Figure 3
Source spectral power as a function of the photon energy (blue, 231 W), source spectrum without power specularly reflected (black, 227.5 W), energy spectrum of the absorbed power in the mirror (red, 215.1 W, 94.5%) and spectrum of the power scattered by the first mirror (green, 12.4 W, 5.5%). The Compton profiles and the Cu [K_\alpha] and [K_\beta] lines can be observed.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 18| Part 3| March 2011| Pages 515-521
doi:10.1107/S0909049511008624
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