The CLS 06ID‐1 Hard X‐ray Micro‐Analysis Beamline (HXMA) is a general purpose hard X‐ray spectroscopy beamline (5 to 40 keV) designed to serve users in XAFS, diffraction and microprobe communities. The beamline uses the synchrotron radiation from a superconducting wiggler. The primary beamline optics include a 1.2 m water‐cooled silicon collimating mirror (separate Rh and Pt coating stripes), a liquid nitrogen cooled double crystal monochromator (Kohzu CMJ‐1) housing two crystal pairs (Si 111 and 220), and a 1.15 m long water‐cooled silicon toroidal focusing mirror (separate Rh and Pt coating stripes). All mirrors are equipped with dynamical meridian benders. The experimental hutch hosts three experimental setups for XAFS, diffraction and microprobe, respectively. Primary design considerations and some commissioning results are discussed.
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19 January 2007
SYNCHROTRON RADIATION INSTRUMENTATION: Ninth International Conference on Synchrotron Radiation Instrumentation
28 May-2 June 2006
Daegu (Korea)
Research Article|
January 19 2007
Wiggler‐base Hard X‐ray Spectroscopy Beamline at CLS
D. T. Jiang;
D. T. Jiang
1Canadian Light Source, University of Saskatchewan, Saskatoon, SK Canada
2Department of Physics, University of Guelph, Guelph ON N1G 2W1 Canada
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N. Chen;
N. Chen
1Canadian Light Source, University of Saskatchewan, Saskatoon, SK Canada
3Geological Sciences Department, University of Saskachewan, Saskatoon, SK Canada
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W. Sheng
W. Sheng
1Canadian Light Source, University of Saskatchewan, Saskatoon, SK Canada
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AIP Conf. Proc. 879, 800–803 (2007)
Citation
D. T. Jiang, N. Chen, W. Sheng; Wiggler‐base Hard X‐ray Spectroscopy Beamline at CLS. AIP Conf. Proc. 19 January 2007; 879 (1): 800–803. https://doi.org/10.1063/1.2436181
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