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Figure 3
The continuous line shows the quantity [\hat{R}_{\rm{in}}] of equation (22)[link], when the compensated spectra S(l) are evaluated for Rin (in the abscissa) using formula (14)[link], for the run without X-ray attenuator at 56 kHz. Its intersection with the dashed line representing [\hat{R}_{\rm{in}}] = Rin that is nearest to the origin is the solution of equation (22)[link].

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 25| Part 2| March 2018| Pages 484-495
https://doi.org/10.1107/S1600577517018318
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