posted on 2015-02-04, 12:01authored byGraeme M. Hansford, S. M. R. Turner, D. Staab, D. Vernon
A novel method to separate diffraction and fluorescence peaks in energydispersive
X-ray diffraction (EDXRD) is described. By tuning the excitation
energy of an X-ray tube source to just below an elemental absorption edge, the
corresponding fluorescence peaks of that element are completely suppressed in
the resulting spectrum. Since Bremsstrahlung photons are present in the source
spectrum up to the excitation energy, any diffraction peaks that lie at similar
energies to the suppressed fluorescence peaks are uncovered. This technique is
an alternative to the more usual method in EDXRD of altering the scattering
angle in order to shift the energies of the diffraction peaks. However, in the
back-reflection EDXRD technique [Hansford (2011). J. Appl. Cryst. 44, 514–
525] changing the scattering angle would lose the unique property of
insensitivity to sample morphology and is therefore an unattractive option.
The use of fluorescence suppression to reveal diffraction peaks is demonstrated
experimentally by suppressing the Ca K fluorescence peaks in the backreflection
EDXRD spectra of several limestones and dolomites. Three
substantial benefits are derived: uncovering of diffraction peak(s) that are
otherwise obscured by fluorescence; suppression of the Ca K escape peaks; and
an increase in the signal-to-background ratio. The improvement in the quality of
the EDXRD spectrum allows the identification of a secondary mineral in the
samples, where present. The results for a pressed-powder pellet of the geological
standard JDo-1 (dolomite) show the presence of crystallite preferred
orientation in this prepared sample. Preferred orientation is absent in several
unprepared limestone and dolomite rock specimens, illustrating an advantage of
the observation of rocks in their natural state enabled by back-reflection
EDXRD.
History
Citation
Journal of Applied Crystallography, 2014, 47, pp. 1708-1715
Author affiliation
/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy