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Figure 5
Correspondence between the simulated structure (calculated using the programme CMPR) and the measured GISAXS images in MTES–TEOS (a) and (b), and TEOS films (c) and (d), calcined at 473 K.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 12| Part 6| October 2005| Pages 734-738
doi:10.1107/S0909049505014585
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