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The Wavelength dispersive X-ray spectroscopy is a method used to determine the energy spectrum of an X-ray radiation. It is mainly used in chemical analysis, in an X-ray fluorescence spectrometer, or in an electron microprobe (Castaing probe).

Explanation


The X-rays emitted by the analysed object are collimated by parallel copper blades (called collimator or Soller slits), and irradiate a known single crystal. The single crystal diffracts the photons (Bragg's law) and are collected by a detector, usually a scintillation counter or a proportional counter.

The single crystal and the detector are mounted on a goniometer which is a device similar to a traditional X-ray diffractometer. It is usually operated under vacuum to reduce the absorption of soft radiation (low-energy photons) by the air and thus increase the sensitivity for the detection and quantitation of light elements (between boron and oxygen).

See also


External links


  • The Science of Spectroscopy - supported by NASA, includes OpenSpectrum, a Wiki-based learning tool for spectroscopy that anyone can edit

  • Parallax Research Inc. - Suppliers of High Resolution WDS Systems for Light Element and Transition Element Microanalysis

analyse dispersive en longueur d'onde | Röntgenfluoreszenzanalyse

Spectroscopy

 

This article is licensed under the GNU Free Documentation License. It uses material from the "Wavelength dispersive X-ray spectroscopy".

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