347 21
Si
E 0 = 20 keVaCounts1000000100 00010 0001000100
0.0 1.0 2.0 3.0
Photon energy (keV)4.0 5.0 6.0 7.0 8.0 9.0 10.0Si_20kV10nA14%DTSi
Cr
Cu
E 0 = 20 keVbCounts1000000100 00010 0001000100
Photon energy (keV)0.0 1.0 2.0 3.0 4.0 5.0 6.0 7.0 8.0 9.0 10.0Si_20kV10nA14%DT
Cr_20kV10nA9%DT
Cu_20kV10nA10%DT. Fig. 21.4 a SDD-EDS spectrum of Si (20 keV; 1000 nA-s; 0.1–20 keV = 22 million counts) with energy windows defined for Al, Cr, and Cu.
b Spectrum for Si with the spectra of Cr and Cu superimposed
. Table 21.3 Estimated limits of detection kDL for a Si
spectrum with 110 million counts (0.1–20 keV)
Element kDL ZAF CDL (mass conc) CDL (ppm)Al 0.000115 1.12 0.000129 129
Cr 0.000133 1.01 0.000134 134
Cu 0.000113 1.00 0.000113 113interaction volume into the K412 glass to excite secondary
fluorescence. The calculated spectrum shown in. Fig. 21.6
shows the presence of an apparent trace level of Fe (and to a
lesser extent, Ca, Si, Al, and Mg) in the Cu, corresponding to
k = 0.0028 relative to a pure Fe standard. The Fe k-ratio as a
function of beam position in the Cu is also shown in
. Fig. 21.6. Even with the beam placed in the Cu at a distance
of 40 μm from the K-412, there is an apparent Fe trace level
in the Cu of k = 0.0004, or about 400 ppm.
Range of characteristic-induced fluorescence
Range of direct electron excitation
in 75Ni-25Fe at E 0 = 25 keVRange of secondary X-ray excitation
(characteristic fluorescence)
of Fe K-L 3 by Ni K-L 3Ni K-L 3 in 75Ni-25Fe10 μm50%
75%
90%99%. Fig. 21.5 Range of secondary fluorescence of FeKα by NiKα in a
75Ni-25Fe alloy at E 0 = 25 keV
21.3 · Measurements of Trace Constituents by Electron-Excited Energy Dispersive X-ray Spectrometry