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Figure 1
Layout of the IMBL (a) with (1) the X-ray source, a 62 poles, 4.2 Tesla superconducting wigger (Häusermann et al., 2010BB9); (2) beam-defining slits; (3) filters to remove low-energy X-rays and reduce the thermal load on the monochromator; (4) a double-crystal Laue-type monochromator; (5) secondary slits; (6) clean-up slits, an imaging shutter and an ionization chamber to monitor the beam intensity; (7) a 90 m-long beam-transfer line to the IMBL satellite building with enclosure 3B (see the main text); (8) pre-sample clean-up slits; (9) a multi-axes CT stage; and (10) the Ruby imaging detector. The IMBL is 145 m long with a maximum sample-to-detector distance of 8 m. (b) The monochromator used to acquire sCT images at the Australian Synchrotron IMBL.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 28| Part 6| November 2021| Pages 1769-1777
https://doi.org/10.1107/S1600577521010493
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