Energy-Dispersive Detector Energy Calibration |
Energy-Dispersive Detector Energy Calibration
Energy-dispersive detectors require calibration for both energy scale and fixed scattering angle, 2θ. The data is collected using a multichannel analyser with typically 4096 channels; the channel number, n, being approximately proportional to the energy of the measured X-ray photon, E. At very high energies, a non-linear behaviour is observed so that in practice a quadratic expression is used for the relationship between n and E:
The quadratic coefficients, a, b, c, are obtained by measuring the channel number for certain well-defined energies. For the higher energies, γ-emitting radioactive sources, such as 241Am (59.5412 keV) or 57Co (122.0607 and 136.4736 keV), may be used as shown in the figure below:
The broad peak at approximately 50 keV next to the Tb Kβ1 peak is due to Compton scattering. A table of values for the fluorescence lines indicated above is provided below. A complete listing of K (and L) emission X-ray lines are available in the International Tables for Crystallography, Volume C, page 177-182 (or in the old volume III).
Kα2 | Kα1 | Kβ1 | Kβ2 | |
---|---|---|---|---|
Cu | 8.042 keV | |||
(1.54178 Å) | ||||
Rb | 13.377 keV | 14.963 keV | ||
(0.92688 Å) | (0.82863 Å) | |||
Mo | 17.446 keV | 19.610 keV | ||
(0.71069 Å) | (0.63225 Å) | |||
Ag | 22.108 keV | 24.946 keV | 25.459 keV | |
(0.56083 Å) | (0.49701 Å) | (0.48701 Å) | ||
Ba | 31.820 keV | 32.197 keV | 36.382 keV | 37.261 keV |
(0.38965 Å) | (0.38509 Å) | (0.34079 Å) | (0.33275 Å) | |
Tb | 43.745 keV | 44.478 keV | 50.399 keV | 51.747 keV |
(0.28343 Å) | (0.27876 Å) | (0.24601 Å) | (0.23960 Å) |
© Copyright 1997-2006. Birkbeck College, University of London. | Author(s): Jeremy Karl Cockcroft |