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Figure 4
Dependence of the intensity of the lamellar reflections on the disk spacing. (a) The first, second-, third- and fourth-order reflections. (b) The sixth- and seventh-order reflections. (c) The eighth-, ninth- and tenth-order reflections. The fifth reflection was too weak to quantify. The integrated intensity of each order after correction with the Lorentz factor is given as a percentage of the sum of intensities of all ten reflections. The data from 13 ROSs are plotted.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 19| Part 4| May 2012| Pages 574-578
doi:10.1107/S0909049512018535
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