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Figure 2
Calculated brilliance, beginning at the sixth harmonic, for (solid line) the 33 mm-period undulator with the 2.5° phase error and (dotted line) for an undulator with 4.6° phase error at 1.15 cm gap. The brilliance above 50 keV has been multiplied by a factor of four for clarity. While this difference in phase error has no effect at low harmonics, it would affect the brilliance at high harmonics.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 5| Part 3| May 1998| Pages 189-195
https://doi.org/10.1107/S0909049597013769
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