Space constraints also result in the spectrometers having mechanical limits in Bragg angle range. In the Cameca MBX and SX-50 microprobes, 2q ranges from 25° to 112°, and in the JEOL 733 microprobe, from 25° to 130°. Thus, crystals with different d-spacings are necessary to cover the entire range of wavelengths of interest. The most commonly used crystals are:
Lithium fluoride 200 (LIF), 2d = 4.028 Å
Potassium acid pthalate 1011 (KAP), 2d = 26.6 Å
Ammonium dihydrogen phosphate 011 (ADP), 2d = 10.648 Å
Rubidium acid pthalate (RAP), 2d = 26.1 Å
Pentaerythritol 002 (PET), 2d = 8.742 Å
Thallium acid pthalate 1011 (TAP), 2d = 25.75 Å, and
Lead sterate or Lead octodecamoate (ODPB), 2d = 100 Å.
LIF is an ionic solid, PET, a KAP, RAP and TAP are organic crystals, and ODPB is a pseudo-crystal, in which Pb atoms are interlayered with a fatty-acid salt to produce regularly spaced planes equivalent to interplanar crystal spacing; it is periodic in only one direction. The approximate range of analyzable elements for Cameca MBX microprobes are:
|
|
|
||||||||||||||||||||
For example, Fe-Ka with a wavelength of 1.937 Å, is located at 2q of 57.5° on LIF, 25.6° on PET, and 8.6° on TAP. Fe-Ka radiation is at or outside the mechanical limits of the MBX spectrometers (2q from 25o to 112o) for PET and TAP. The table below shows the crystals and sinq values for most geologically important elements.
SINQ POSITIONS
|
|
TAP (2d = 25.75) |
PET (2d = 8.742) |
LIF (2d = 4.028) |
|||
|
Ka |
La |
Ka |
La |
Ka |
La |
|
|
F |
0.71315 |
|
|
|
|
|
|
Na |
0.46363 |
|
|
|
|
|
|
Mg |
0.38499 |
|
|
|
|
|
|
Al |
0.32463 |
|
|
|
|
|
|
Si |
0.27750 |
|
0.81445 |
|
|
|
|
P |
0.23968 |
|
0.70376 |
|
|
|
|
S |
|
|
0.61405 |
|
|
|
|
Cl |
|
|
0.54040 |
|
|
|
|
K |
|
|
0.42765 |
|
|
|
|
Ca |
|
|
0.38374 |
|
|
|
|
Sc |
||||||
|
Ti |
|
|
0.31416 |
|
0.68261 |
|
|
V |
|
|
0.28616 |
|
0.62178 |
|
|
Cr |
|
|
0.26172 |
|
0.56866 |
|
|
Mn |
|
0.75714 |
0.24024 |
|
0.52200 |
|
|
Fe |
|
0.68473 |
|
|
0.48090 |
|
|
Co |
|
0.62175 |
|
|
0.44430 |
|
|
Ni |
|
0.56682 |
|
|
0.41175 |
|
|
Cu |
|
0.51914 |
|
|
0.38261 |
|
|
Zn |
|
0.47702 |
|
|
|
|
|
Sr |
|
0.26715 |
|
0.78443 |
|
|
|
Zr |
|
0.23631 |
|
0.69387 |
|
|
|
Nb |
|
|
|
0.65430 |
|
|
|
Ba |
|
|
|
0.31730 |
|
0.68943 |
|
La |
|
|
|
0.30470 |
|
0.66204 |
|
Ce |
|
|
|
0.29279 |
|
0.63617 |
The efficiency of an X-ray spectrometer, in part, depends on the crystal design and crystals are bent and/or ground to improve their efficiency. This can be done in two ways (Figure 3.5.4a):
Unfortunately, it is not possible to grind all types of crystals, so the use of Johann optics is more common.
|
|
Figure 3.5.4a. The essential geometry of fully focusing Johannson (left) and semi-focusing Johann (right) X-ray spectrometer optics. These diagrams are not drawn to scale and exaggerate the loss of resolution in a semi-focusing spectrometer. The effect is much less pronounced than they suggest, and semi-focusing spectrometers are commonly used in microprobes (after Williams 1987). |
A number of characteristics are required for a good spectrometer crystal. Some are more obvious than others:

Note that higher order reflections are better dispersed and that the 2d-spacing of the crystal is an important factor. Where high resolution is desired, it is best to avoid low q and wide 2d-spacings even at the loss of intensity. Such conditions pertain when analyzing trace amounts of V in Ti-bearing materials and the analysis of rare earth elements.
|
|
Figure 3.5.4b. Curves of temperature coefficient of linear expansion for some common crystals (after Jenkins & de Vries, 1967). |
Copyright 1997-2003, James H. Wittke
Last update: 01/18/2006 01:47 PM.