An Overview of XRF Basics
3. Sample Preparation Techniques
for XRF Analysis
3.1 Introduction
X-ray fluorescence (XRF) analysis is a fast, non-destructive and environmentally friendly analysis method with very high accuracy and reproducibility. All elements of the periodic table from beryllium to californium can be measured qualitatively, semi-quantitatively and quantitatively in powders, solids and liquids. Concentrations of up to 100% are analyzed directly, without any dilution, with reproducibilities better than ±0.1%. Typical limits of detection are from 0.1 to 10 ppm. Most modern X-ray spectrometers with modular sample changers enable fast, flexible sample handling and adaptation to customer-specific automation processes.
XRF samples can be solids such as glass, ceramic, metal, rock, coal, or plastic. They can also be liquids, like petrol, oil, paint, solutions, blood or even wine. With an XRF spectrometer both very small concentrations of very few ppm and very high concentrations of up to 100% can be analyzed directly without any dilution process. Based on its simple and fast sample preparation requirements, XRF analysis is a universal analysis method, that has been widely accepted in the fields of research and industrial process control. XRF is particularly effective for complex environmental analysis and for production and quality control of intermediate and end products.
The quality of sample preparation for XRF analysis is at least as important as the quality of measurements.
An ideal sample is prepared so that it is:
- representative of the material
- homogeneous
- thick enough to meet the requirements of an infinitely thick sample
- without surface irregularities
- composed of small enough particles for the wavelengths to be measured
With XRF it is not necessary to bring solid samples into solution and then dispose of solution residues, as is the case with all wet-chemical methods. The main prerequisite for exact and reproducible analysis is a plain, homogeneous and clean analysis surface. For analysis of very light elements, e.g. beryllium, boron and carbon, the fluorescence radiation to be analyzed originates from a layer whose thickness is only a few atom layers to a few tenths of micrometer and which strongly depends on the sample material (Table 6). Careful sample preparation is therefore extremely important for analysis of light elements.
| Sample matrix | Graphite | Glass | Iron | Lead | |
|---|---|---|---|---|---|
| Line | h_(90%, µm) | h_(90%, µm) | h_(90%, µm) | h_(90%, µm) | |
| U | Lα1 | 28000 | 1735 | 154 | 22.4 |
| Pb | Lβ1 | 22200 | 1398 | 125 | 63.9 |
| Hg | Lα1 | 10750 | 709 | 65.6 | 34.9 |
| W | Lα1 | 6289 | 429 | 40.9 | 22.4 |
| Ce | Lβ1 | 1484 | 113 | 96.1 | 6.72 |
| Ba | Lα1 | 893 | 71.3 | 61.3 | 4.4 |
| Sn | Lα1 | 399 | 44.8 | 30.2 | 3.34 |
| Cd | Kα1 | 144600 | 8197 | 701 | 77.3 |
| Mo | Kα1 | 60580 | 3600 | 314 | 36.7 |
| Zr | Kα1 | 44130 | 2668 | 235 | 28.9 |
| Sr | Kα1 | 31620 | 1947 | 173 | 24.6 |
| Br | Kα1,2 | 18580 | 1183 | 106 | 55.1 |
| As | Kβ1 | 17773 | 1132 | 102 | 53 |
| Zn | Kα1,2 | 6861 | 466 | 44.1 | 24 |
| Cu | Kα1,2 | 5512 | 380 | 36.4 | 20 |
| Ni | Kα1,2 | 4394 | 307 | 29.8 | 16.6 |
| Fe | Kα1,2 | 2720 | 196 | 164 | 11.1 |
| Mn | Kα1,2 | 2110 | 155 | 131 | 9.01 |
| Cr | Kα1,2 | 1619 | 122 | 104 | 7.23 |
| Ti | Kα1,2 | 920 | 73.3 | 63 | 4.52 |
| Ca | Kα1,2 | 495 | 54.3 | 36.5 | 3.41 |
| K | Kα1,2 | 355 | 40.2 | 27.2 | 3.04 |
| Cl | Kα1,2 | 172 | 20.9 | 14.3 | 2.19 |
| S | Kα1,2 | 116 | 14.8 | 10.1 | 4.83 |
| Si | Kα1,2 | 48.9 | 16.1 | 4.69 | 2.47 |
| Al | Kα1,2 | 31.8 | 10.5 | 3.05 | 1.7 |
| Mg | Kα1,2 | 20 | 7.08 | 1.92 | 1.13 |
| Na | Kα1,2 | 12 | 5.56 | 1.15 | 0.728 |
| F | Kα1,2 | 3.7 | 1.71 | 0.356 | 0.262 |
| O | Kα1,2 | 1.85 | 2.50 | 0.178 | 0.143 |
| N | Kα1,2 | 0.831 | 1.11 | 0.08018 | 0.07133 |
| C | Kα1,2 | 13.6 | 0.424 | 0.03108 | 0.03124 |
| B | Kα1,2 | 4.19 | 0.134 | 0.01002 | 0.01166 |