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Figure 4
Calculated bump leakage variation as a function of the ratio of two sextupole strengths in the bump orbit. Here the strengths of the bump magnets are adjusted to close the bump orbit at its peak amplitude in consideration of sextupole non-linearity. A pulse width of 3 µs was used in the calculation.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
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