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Figure 4
CNR, as expressed by equation (13)[link], in the setups with parameters from Tables 1[link] and 2[link], 0.1 m ≤ R2 ≤ 20 m, Iin(λ) = 1 µm−2, and different X-ray wavelengths (energies): λ = 0.4769 Å (E = 26 keV, dotted line), λ = 0.3875 Å (E = 32 keV, solid line), λ = 0.2952 Å (E = 42 keV, dashed line). The optimal magnification in this case is equal to MCNR ≃ 1.087 (R2 ≃ 11.2 m).

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 33| Part 2| March 2026| Pages 395-408
https://doi.org/10.1107/S1600577525010732
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