For a multi-element material, the mass absorption coefficients at a particular wavelength are multiplied by the mass fraction each element and summed to yield a bulk coefficient:
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Bulk mass absorption coefficients decrease with increasing energy (Table 3). Mass absorption coefficients for all elements (energies from 1 keV to 20 MeV!) are available at: http://physics.nist.gov/PhysRefData/XrayMassCoef/tab3.html. A technical presentation of mass absorption coefficients is available at: http://physics.nist.gov/PhysRefData/XrayMassCoef/cover.html.
Generally, more energetic radiation is absorbed less than lower energy radiation; however, higher energy radiation will be absorbed strongly if it is energetic enough to ionize another element (E > Ec). This produces "teeth" on the intensity curve (Figures 2.6.1a and 2.6.1b). These teeth are termed absorption edges. Absorption edge values for all elements are available at: http://www.bmsc.washington.edu/scatter/periodic-table.html.
MASS ABSORPTION COEFFICIENTS FOR Ka RADIATION (cm2/g)
|
Absorber |
Emitter |
|||||||||||||
|
Na |
Mg |
Al |
Si |
P |
S |
Cl |
K |
Ca |
Ti |
Cr |
Mn |
Fe |
Ni |
|
|
O |
3653 |
2169 |
1345 |
865 |
574 |
391 |
273 |
141 |
105 |
60 |
36 |
28 |
22 |
14 |
|
Na |
562 |
5409 |
3365 |
2170 |
1444 |
987 |
691 |
359 |
266 |
152 |
92 |
72 |
57 |
37 |
|
Mg |
768 |
463 |
4287 |
2768 |
1843 |
1261 |
883 |
460 |
341 |
195 |
118 |
93 |
74 |
48 |
|
Al |
1019 |
614 |
386 |
3451 |
2300 |
1575 |
1104 |
576 |
427 |
245 |
148 |
116 |
93 |
60 |
|
Si |
1319 |
794 |
499 |
325 |
2816 |
1929 |
1353 |
707 |
524 |
301 |
182 |
143 |
114 |
74 |
|
P |
1670 |
1006 |
632 |
411 |
276 |
2325 |
1632 |
854 |
633 |
364 |
220 |
174 |
138 |
90 |
|
S |
2076 |
1251 |
786 |
511 |
343 |
236 |
1940 |
1016 |
754 |
434 |
262 |
207 |
165 |
108 |
|
Cl |
2542 |
1531 |
962 |
626 |
420 |
289 |
204 |
1194 |
887 |
511 |
309 |
244 |
195 |
127 |
|
K |
3663 |
2207 |
1386 |
902 |
605 |
417 |
294 |
155 |
1188 |
686 |
415 |
329 |
262 |
171 |
|
Ca |
4326 |
2606 |
1637 |
1066 |
715 |
493 |
347 |
183 |
136 |
783 |
475 |
376 |
300 |
196 |
|
Ti |
5871 |
3571 |
2222 |
1446 |
970 |
668 |
471 |
249 |
185 |
107 |
607 |
480 |
384 |
251 |
|
Cr |
7728 |
4655 |
2924 |
1903 |
1277 |
880 |
620 |
327 |
244 |
141 |
86 |
68 |
478 |
313 |
|
Mn |
8780 |
5289 |
3323 |
2163 |
1451 |
1000 |
705 |
372 |
277 |
160 |
97 |
77 |
62 |
347 |
|
Fe |
9918 |
5975 |
3753 |
2443 |
1639 |
1129 |
796 |
420 |
313 |
181 |
110 |
87 |
70 |
382 |
|
Ni |
12464 |
7509 |
4717 |
3070 |
2060 |
1419 |
1001 |
528 |
393 |
228 |
138 |
110 |
88 |
57 |
As an example, consider the absorption of Ni-Ka and Co-Ka radiation in pyrite. Pyrite consists of 0.4655 Fe and 0.5345 S (weight fractions). The mass absorption coefficients are:
|
|
Ni-Ka |
Co-Ka |
|
S |
108 |
133 |
|
Fe |
382 |
56 |
Therefore, the bulk mass absorption coefficients are:
mNi =
0.5345 x 108 + 0.4655 x 382 = 236
mCo =
0.5345 x 133 + 0.4655 x 56 = 97
Notice that although Ni-Ka is more energetic than Co-Ka (7.48 keV vs. 6.91 keV), it is absorbed over twice as much because Ni-Ka radiation is sufficiently energetic to excite Fe-Ka radiation (Ec = 7.112 keV) from the pyrite. An excellent absorption calculator is available at: http://www-cxro.lbl.gov/optical_constants/atten2.html. Try entering various elements and compounds.
| Figure 2.6.1a. Schematic plot of the X-ray absorption curve for a single element of high atomic weight. The qualitative features of the curve remain the same whether the vertical axis represents the probability of X-ray absorption, the stopping power of the element, or the mass absorption coefficient. |
|
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Figure 2.6.1b. Actual plot of the mass absorption coefficients of samarium for energies between 0 and 25 keV. The marked discontinuities are the absorption edges; each corresponds to a critical excitation potential in the L and M spectral series (the K absorption edge is to the right of the plotted region at 46.8 keV). |
Copyright 1997-2003, James H. Wittke
Last update: 01/18/2006 01:47 PM.