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Figure 8
(a) Variations of the FC inclination γ along the `numerical' SP trajectories from Fig. 7[link]. (b) Energy dependences of α and r1 delivering the SP lineshape at constant γ = 20°, identifying the FI operation mode.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 18| Part 2| March 2011| Pages 134-142
https://doi.org/10.1107/S0909049510054452
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