The GALAXIES inelastic hard X-ray scattering end-station at Synchrotron SOLEIL

Ablett, J.M.; Prieur, D.; Céolin, D.; Lassalle-Kaiser, B.; Lebert, B.; Sauvage, M.; Moreno, T.; Bac, S.; Balédent, V.; Ovono, A.; Morand M.; Gélebart, F.; Shukla, A.; Rueff, J.-P.

doi:10.1107/S160057751801559X

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Figure 10
1s2p RIXS–XMCD on Fe₃O₄ in the pre-edge region of the K-edge. Upper left: Fe Kα₁ intensity as a function of incident energy for left and right circularly polarized light (LCP and RCP) with the sample magnetized along the incident X-ray direction in a field of 0.7 T. Bottom left: the difference between RCP and LCP Fe Kα₁ intensity as a function of incident X-ray energy for the two magnetic field directions. Right: the RIXS–MCD map showing the dramatic magnetic contrast for RCP–LCP in a magnetic field of 0.7 T.

JOURNAL OF
SYNCHROTRON
RADIATION

ISSN: 1600-5775

Volume 26| Part 1| January 2019| Pages 263-271

https://doi.org/10.1107/S160057751801559X

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