2005
DOI: 10.1238/physica.topical.115a00980
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SAMBA a New Beamline at SOLEIL for XRay Absorption Spectroscopy in the 440keV Energy Range

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Cited by 34 publications
(24 citation statements)
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“…Spectra from extended X-ray absorption fine structure (EXAFS) spectroscopy were recorded at the Pb L III -edge (13.055 keV) at the French National Synchrotron Facility (SOLEIL, St. Aubin, France) on the SAMBA beam line equipped with a Si(111) double crystal monochromator (Belin et al 2005). The bulk spiked soil was dried, ground in an agate mortar, and pressed as 5-mm-diameter pellets using a hydraulic press generating a pressure of 30 bars.…”
Section: Soil and Plant Analysismentioning
confidence: 99%
“…Spectra from extended X-ray absorption fine structure (EXAFS) spectroscopy were recorded at the Pb L III -edge (13.055 keV) at the French National Synchrotron Facility (SOLEIL, St. Aubin, France) on the SAMBA beam line equipped with a Si(111) double crystal monochromator (Belin et al 2005). The bulk spiked soil was dried, ground in an agate mortar, and pressed as 5-mm-diameter pellets using a hydraulic press generating a pressure of 30 bars.…”
Section: Soil and Plant Analysismentioning
confidence: 99%
“…The chemical composition of the samples in set2 was determined by Electron Probe Micro Analysis (EPMA, CAMECA SX100). X-ray absorption spectroscopy was carried out on the SAMBA beamline 43 at SOLEIL synchrotron source, using a fixed sagitally focusing Si(111) double crystal monochromator. XANES spectra were recorded in transmission mode, in the 8800-9000 eV energy range (including LIII-Yb edge), with a 0.3eV resolution in the edge jump, at five different temperatures: 20 K, 70 K, 130 K, 200 K and 300 K. Spectra were normalized using the MAX-Package 44 .…”
Section: Methodsmentioning
confidence: 99%
“…The mirrors are used over the whole 4-40 keV energy range available on SAMBA by tilting the mirrors from 10 mrad to 1 mrad depending on the desired cut-off energy for removing the harmonic X-rays [5]. The reflective Pd surfaces are 1200 mm long per 88 mm wide allowing a horizontal acceptance of ∼6.2 mrad on the first collimating mirror located at 14.1 m from the source.…”
Section: Collimating and Focusing Mirrorsmentioning
confidence: 99%