

Energy-Dispersive X-Ray Fluorescence Spectrometer
能量色散 X 射线荧光光谱仪
- SKU XRF-0001
- XRF
- CE (to be confirmed)
- Radiation safety enclosure (to be confirmed)
- ISO 9001 manufacturing (to be confirmed)
Price on request — FOB / CIF quoted per order
Prices depend on configuration, quantity and destination port.
Key specifications
| Element range | Na to U (Mg to U in air) |
|---|---|
| Detection limit | 1–100 mg/kg typical |
| X-ray tube power | 10–50 W |
| Detector | silicon drift detector |
| Measurement time | 30–300 s |
| Sample types | solids, powders, liquids, films |
By Lab Manufacturers China Technical TeamLast reviewed Standards: ASTM E1621 Wavelength dispersive X-ray fluorescence, ASTM D4294 Sulfur in petroleum products by EDXRF, ISO 3497 Metallic coatings — X-ray spectrometric thickness
What is the Energy-Dispersive X-Ray Fluorescence Spectrometer?
An energy-dispersive XRF spectrometer measures photon energies directly with a semiconductor detector and records the entire spectrum at once. It is the fast, compact workhorse for routine multi-element screening and quality control.
What is the Energy-Dispersive X-Ray Fluorescence Spectrometer?
An energy-dispersive XRF spectrometer measures photon energies directly with a semiconductor detector and records the entire spectrum at once. It is the fast, compact workhorse for routine multi-element screening and quality control.
Overview
A low-power X-ray tube excites the sample, and fluorescence passes to a silicon drift detector that measures the energy of each photon. A multichannel analyzer builds a spectrum in which peak positions identify elements and peak areas give concentrations. Collecting the whole spectrum simultaneously makes measurement fast, often 30 to 300 seconds, and the design has no moving analyzer crystals, which keeps the instrument compact and robust. Secondary targets or filters can be inserted to shape the excitation spectrum and reduce background. Light elements need vacuum or helium purge, and matrix effects are corrected with fundamental parameters or empirical calibrations. Energy-dispersive XRF is widely used for alloy identification, RoHS screening, cement and minerals, environmental samples and quality checks where speed and flexibility matter more than the lowest detection limits.
How does it work?
A primary X-ray beam from a tube or radioisotope source ejects inner-shell electrons from sample atoms. Electrons from higher shells fall into the vacancies and emit X-ray photons whose energies equal the difference between the two levels, which is unique to each element. The intensity of each characteristic line is proportional to the amount of that element, so calibration with reference materials gives concentration. Energy-dispersive instruments use a semiconductor detector such as silicon drift to measure photon energies directly and record the whole spectrum at once. Wavelength-dispersive instruments use analyzing crystals to diffract specific wavelengths to a detector, giving better resolution and lower detection limits, especially for light elements. Matrix effects from absorption and secondary excitation are corrected by fundamental parameters or empirical influence coefficients, and sample form is matched to calibration standards.
What are the key features?
- Silicon drift detector with multichannel analyzer
- Simultaneous full-spectrum acquisition
- Measurement times of 30 to 300 seconds
- Secondary targets and filters to reduce background
- Vacuum or helium purge for light elements
- Compact benchtop design with few moving parts
What are the technical specifications?
A typical energy-dispersive x-ray fluorescence spectrometer configuration offers element range of Na to U (Mg to U in air), detection limit of 1–100 mg/kg typical, X-ray tube power of 10–50 W, detector of silicon drift detector, measurement time of 30–300 s and sample types of solids, powders, liquids, films. Values are indicative of the product class; the exact figures for each configuration are confirmed on the quotation and the calibration documents supplied with the instrument.
Which applications is it used for?
The Energy-Dispersive X-Ray Fluorescence Spectrometer is used in alloy and material identification, roHS and restricted substance screening, cement, glass and ceramic analysis and environmental and geological samples. Across the wider XRF class, laboratories also deploy it for elemental analysis of alloys, ceramics and glass, roHS and restricted substance screening and coating thickness and thin-film composition.
Which standards and certifications apply?
Relevant standards and methods include ASTM E1621 Wavelength dispersive X-ray fluorescence, ASTM D4294 Sulfur in petroleum products by EDXRF, ISO 3497 Metallic coatings — X-ray spectrometric thickness, IEC 62321 Determination of restricted substances in electrotechnical products, US EPA Method 6200 Field portable XRF for soil, ISO 13196 Soil quality — Screening of selected elements by EDXRF, IEC 61010-2-091 and ISO/IEC 17025. Certification candidates for this model are CE, Radiation safety enclosure and ISO 9001 manufacturing; each is to be confirmed for the specific configuration before shipment, and certificates are supplied only where they have been issued.
XRF instruments are regulated radiation devices, so installation requires shielding, interlocks, radiation surveys and trained operators, with portable units also needing safe work procedures. Sample preparation strongly affects accuracy: surface contamination, insufficient thickness and particle size effects bias results, and powders are best pressed or fused. Calibration must match the sample matrix, and drift is monitored with check standards. Vacuum or helium systems need clean seals and gas supplies for light elements. Detector windows and X-ray tubes are wear parts with finite life. Keep records of tube hours, calibration and checks, and dispose of X-ray components according to radiation regulations.
How do I select the right Energy-Dispersive X-Ray Fluorescence Spectrometer?
Select energy-dispersive XRF for fast, flexible multi-element screening when detection limits in the low parts per million range are adequate. Specify the element range, sample types and required throughput. Add vacuum or helium purge if light elements are needed, and confirm that calibration standards matching your matrices are available.
How does it compare with other XRF variants?
Select an XRF configuration by element range, detection limit and sample type. Energy-dispersive instruments are compact, fast and well suited to routine screening and multi-element analysis, with moderate resolution. Wavelength-dispersive instruments cost more and are slower but excel for light elements, precise major-oxide analysis and low detection limits. Total reflection instruments reach ultratrace levels on small sample spots and serve semiconductor, water and biological analysis. Polarized energy-dispersive instruments lower background for trace work without the cost of wavelength dispersive optics. Micro-XRF adds spatial resolution for inclusions, coatings and forensic samples. Consider sample size, whether vacuum or helium purge is needed for light elements, automation level and the regulatory method your laboratory must follow before deciding.
Full specifications
| Element range | Na to U (Mg to U in air) |
|---|---|
| Detection limit | 1–100 mg/kg typical |
| X-ray tube power | 10–50 W |
| Detector | silicon drift detector |
| Measurement time | 30–300 s |
| Sample types | solids, powders, liquids, films |
| Atmosphere | air, vacuum or helium |
| Spot size | 1–10 mm |
| Sample changer | optional 10 to 20 positions |
| Interface | Ethernet / USB |
Indicative values for this product class. Final specifications are confirmed on the quotation and in the calibration documents supplied with the instrument.
Applications
- Alloy and material identification
- RoHS and restricted substance screening
- Cement, glass and ceramic analysis
- Environmental and geological samples
Key features
- Silicon drift detector with multichannel analyzer
- Simultaneous full-spectrum acquisition
- Measurement times of 30 to 300 seconds
- Secondary targets and filters to reduce background
- Vacuum or helium purge for light elements
- Compact benchtop design with few moving parts
Frequently asked questions about Energy-Dispersive X-Ray Fluorescence Spectrometer
Typical measurement times range from 30 seconds for a quick screening scan to about five minutes for better precision and lower detection limits. Longer counting times improve statistics because more photons are collected. Quality-control methods balance time against the required precision.
A secondary target is a plate that is excited by the primary X-ray beam and re-emits fluorescence, which then irradiates the sample. This creates a more selective excitation spectrum and polarized radiation that lowers the background under analyte peaks, improving detection limits for trace elements.
It can be accurate when matrix-matched standards and appropriate correction models are used, achieving relative errors of a few percent for major elements. Peak overlap and detector resolution limit light-element and trace performance compared with wavelength-dispersive systems, so the technique is often used for screening or for well-characterized matrices.
EDXRF measures photon energies directly with a semiconductor detector and records the whole spectrum simultaneously, giving speed and a compact design. WDXRF uses analyzing crystals to diffract selected wavelengths and offers higher resolution, better light-element performance and lower detection limits at higher cost and longer measurement times.
The sample must be thick enough that the full primary beam is absorbed within it and fluorescence from deeper layers does not change the result, a condition called infinite thickness. This thickness depends on the element and matrix, ranging from micrometres for heavy elements in light matrices to millimetres for light elements, and it is verified during method development.
The intensity of an element line depends not only on its concentration but also on how other elements absorb the primary and fluorescent X-rays and on secondary excitation. These matrix effects can change intensities by large factors, so accurate analysis requires matrix-matched standards or correction models based on fundamental parameters or influence coefficients.




