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Figure 3
Intensity correction factors for peak integration of GIXD data. Normalized inverses of the Lorentz correction when integrating in (a) Cartesian reciprocal-space coordinates (qx, qy, qz), (b) cylindrical reciprocal-space coordinates (qxy, qz, φ) and (c) spherical reciprocal-space coordinates (q, ψ, φ). In every case, the Lorentz correction is independent of the unshown dimension [i.e. qy for panel (a), and φ for panels (b) and (c)].

Journal logoJOURNAL OF
APPLIED
CRYSTALLOGRAPHY
ISSN: 1600-5767
Volume 58| Part 1| February 2025| Pages 96-106
https://doi.org/10.1107/S1600576724010628
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