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Figure 9
(a) ΔE dependences of r1 along the `numerical' SP trajectory for 530 eV from Fig. 7[link] calculated with different Δα. In their minimum ΔE is almost independent of Δα, identifying the MA mode. (b) Energy dependences of α and r1 for the MA mode.

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SYNCHROTRON
RADIATION
ISSN: 1600-5775
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