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Figure 4
(a) Intensity error computed between the predicted and measured data using the full projection matrix. The yellow star indicates that the error is zero when the full dataset is used for reconstruction. (b) RSM reconstruction error under the same conditions. (c) Comparison of intensity errors between full-projection and next-five-projection. (d) Predicted intensity of random direction (83rd) from using the full dataset (after azimuthal binning processing). Predicted intensities from reconstructions using 60 projections by (e) SUS, (f) DUS and (g) SNUS (corresponding to open-square curve), while the insets illustrate the corresponding distributions. Reconstructed RSM in a random single voxel using (h) the full dataset, (i) 40 SUS, (j) 40 DUS and (k) 40 SNUS projections (corresponding to the open-square curve).

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 33| Part 4| July 2026|
https://doi.org/10.1107/S1600577526005308
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