Open Access
| Numéro |
2011
UVX 2010 - 10e Colloque sur les Sources Cohérentes et Incohérentes UV, VUV et X ; Applications et Développements Récents
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|---|---|---|
| Page(s) | 41 - 47 | |
| Section | Exposés invités | |
| DOI | https://doi.org/10.1051/uvx/2011006 | |
| Publié en ligne | 21 mars 2011 | |
UVX 2010 (2011) 41-47
SAMBA: The 4–40 keV X-ray absorption spectroscopy beamline at SOLEIL
Synchrotron SOLEIL, L’Orme des Merisiers, BP. 48, 91191 Gif-sur-Yvette, France
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