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Figure 1
Example of the Einstein fit on the parallel mean-square relative displacement: MSRD∥(T) calculated by dynamical simulation (open circles), relative differences δMSRD∥(T) with respect to 0 K (open squares) and corresponding Einstein fit (line). The resulting MSRD∥(T) from the Einstein fit (full circles) is shifted with respect to the correct MSRD∥(T) (open circles).

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 15| Part 5| July 2008| Pages 514-518
doi:10.1107/S0909049508017688
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