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Figure 5
Magnetic field distributions along z, measured before and after cooling. Arabic and roman numbers indicate the averaged peak fields generated at the VP and MXDy PPs over the four peak positions, respectively.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 26| Part 4| July 2019| Pages 1220-1225
https://doi.org/10.1107/S1600577519006052
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