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Figure 3
Autocorrelation functions [g^{{(2)}}(q,\tau)] plotted as a function of the time delay τ from the XPCS analysis and speckle contrast factors [\beta(q,T)] as a function of the integration time T from the XSVS analysis over three q rings of pixels (a) at q = 2.63 × 10-3 Å−1, (b) at q = 2.74 × 10-3 Å−1 and (c) at q = 2.95 × 10-3 Å−1. The experimental [g^{{(2)}}(q,\tau)] (empty circles) are fitted by equation (3[link]) (solid line) for the XPCS analysis. The experimental [\beta(q,T)] (filled circles) are fitted by equation (13[link]) (dashed line) for the XSVS analysis. Note that the horizontal axis is labeled as `Time' for simplicity but has different meanings for the two methods.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 21| Part 6| October 2014| Pages 1288-1295
doi:10.1107/S1600577514015847
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