Abstract
The SAMBA X-ray Absorption beamline has been operating for users since January 2008. The beamline covers a large energy range from 4 up to 40 keV in two working modes: a "high flux" mode using a sagittally focusing monochromator and a "time-resolved" mode using a dedicated Quick-EXAFS monochromator. Herein a technical description of the main beamline components is given and results concerning energy resolution, available flux and time resolved performances are presented. © Owned by the authors, published by EDP Sciences, 2011.
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CITATION STYLE
Briois, V., Fonda, E., Belin, S., Barthe, L., La Fontaine, C., Langlois, F., … Villain, F. (2011). SAMBA: The 4-40 keV X-ray Absorption spectroscopy beamline at SOLEIL. In UVX 2010 - 10e Colloque sur les Sources Coherentes et Incoherentes UV, VUV et X: Applications et Developpements Recents (pp. 41–47). EDP Sciences. https://doi.org/10.1051/uvx/2011006
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