

High-Resolution Echelle ICP-OES Spectrometer
高分辨率中阶梯光栅 ICP-OES 光谱仪
- SKU ICO-0006
- ICP-OES
- CE (to be confirmed)
- ISO 9001 manufacturing (to be confirmed)
- 21 CFR Part 11 software compliance (to be confirmed)
Price on request — FOB / CIF quoted per order
Prices depend on configuration, quantity and destination port.
Key specifications
| Wavelength range | 165–850 nm |
|---|---|
| Optical resolution | ≤ 0.005 nm at 200 nm |
| Detector | large CCD or CMOS array |
| Dispersion | echelle grating plus prism |
| Simultaneous elements | up to 70 |
| Detection limit | 0.5–10 µg/L typical |
By Lab Manufacturers China Technical TeamLast reviewed Standards: USP <730> Plasma Spectrochemistry, USP <233> Elemental Impurities — Procedures, ICH Q3D Elemental Impurities
What is the High-Resolution Echelle ICP-OES Spectrometer?
A high-resolution echelle ICP-OES spectrometer resolves closely spaced emission lines in composite, line-rich spectra. It is chosen for difficult rare-earth, iron-rich and similar samples where unresolved line overlap otherwise causes quantitation errors.
What is the High-Resolution Echelle ICP-OES Spectrometer?
A high-resolution echelle ICP-OES spectrometer resolves closely spaced emission lines in composite, line-rich spectra. It is chosen for difficult rare-earth, iron-rich and similar samples where unresolved line overlap otherwise causes quantitation errors.
Overview
Echelle optics combine a coarse echelle grating with a cross-disperser prism to produce a two-dimensional spectrum of high resolution and wide coverage on a single detector. This design resolves lines that are only fractions of a nanometre apart, which is essential when the sample emits a dense spectrum, such as rare-earth elements with hundreds of lines or iron-rich alloys where iron lines overlap analyte lines. The two-dimensional pattern is captured by a large array detector so many lines are measured simultaneously. Resolution is typically better than 0.005 nanometres in the ultraviolet. High-resolution instruments also improve detection limits by separating analyte lines from nearby interference and are widely used in geochemistry, metallurgy and advanced materials analysis where line-rich matrices are routine.
How does it work?
A radio-frequency generator drives a load coil around a quartz torch, sustaining an argon plasma at 6000 to 10000 K. The sample aerosol enters the plasma and is desolvated, vaporized, atomized and excited. Excited atoms and ions relax and emit light at wavelengths characteristic of each element. The emitted light is dispersed by an echelle grating or a CCD-based polychromator, and multiple lines are measured simultaneously. In radial viewing the plasma is observed from the side, which tolerates high dissolved solids and reduces self-absorption; in axial viewing the plasma is observed end-on, which lengthens the optical path and lowers detection limits. Dual-view instruments switch per element. Internal standards, background correction and interference algorithms correct for drift and overlapping lines. The wide dynamic range lets major, minor and trace elements be measured in one run.
What are the key features?
- Echelle grating with cross-disperser prism
- Two-dimensional spectrum on a large array detector
- Resolution better than 0.005 nm in the ultraviolet
- Resolves line-rich rare-earth and iron matrices
- Simultaneous measurement of many lines
- Improved detection limits by overlap suppression
What are the technical specifications?
A typical high-resolution echelle icp-oes spectrometer configuration offers wavelength range of 165–850 nm, optical resolution of ≤ 0.005 nm at 200 nm, detector of large CCD or CMOS array, dispersion of echelle grating plus prism, simultaneous elements of up to 70 and detection limit of 0.5–10 µg/L typical. 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 High-Resolution Echelle ICP-OES Spectrometer is used in rare-earth element analysis, iron, steel and alloy trace analysis, geological and geochemical research and advanced materials and catalyst testing. Across the wider ICP-OES class, laboratories also deploy it for multi-element water and wastewater analysis, pharmaceutical elemental impurity screening and food, feed and agricultural element analysis.
Which standards and certifications apply?
Relevant standards and methods include USP <730> Plasma Spectrochemistry, USP <233> Elemental Impurities — Procedures, ICH Q3D Elemental Impurities, ISO 11885 Water quality — ICP-OES determination of elements, US EPA Method 200.7, ASTM D5185 and ISO/IEC 17025. Certification candidates for this model are CE, ISO 9001 manufacturing and 21 CFR Part 11 software compliance; each is to be confirmed for the specific configuration before shipment, and certificates are supplied only where they have been issued.
ICP-OES requires high-purity argon, substantial power, exhaust ventilation and a temperature-controlled room. Torch, injector and nebulizer condition strongly affect performance, so inspection and replacement schedules are important. High dissolved solids cause salt build-up on the torch and injector, blocking the plasma and changing sensitivity, so dilution and matrix matching are used. Sample preparation by acid digestion must avoid contamination. Daily checks include wavelength calibration, torch alignment, plasma stability and a check standard. Monitor the argon supply and the chiller, and record torch and nebulizer usage. Data integrity requires calibration verification, QC samples and defined acceptance criteria.
How do I select the right High-Resolution Echelle ICP-OES Spectrometer?
Select a high-resolution echelle instrument when the sample matrix produces dense spectra and line overlap is the limiting factor, as in rare-earth or iron-rich materials. Specify the elements and known interferences, and confirm the resolution and wavelength coverage for the critical lines. Compare with ICP-MS if the main limitation is detection limit rather than resolution.
How does it compare with other ICP-OES variants?
Select an ICP-OES spectrometer by viewing configuration, detector type, resolution and automation. Radial viewing is the best choice for high-matrix samples and major elements, axial viewing for the lowest detection limits in clean samples, and dual view for laboratories that handle both. Simultaneous CCD instruments measure many elements and lines quickly, while sequential scanning instruments are flexible and lower in cost but slower. High-resolution echelle optics help when many emission lines overlap, as in rare-earth or iron-rich samples. Confirm the wavelength range covers the elements and lines you need, including far-ultraviolet lines for halogens. Check argon and power consumption, sample introduction options, autosampler capacity and software features such as interference correction and audit trails.
Full specifications
| Wavelength range | 165–850 nm |
|---|---|
| Optical resolution | ≤ 0.005 nm at 200 nm |
| Detector | large CCD or CMOS array |
| Dispersion | echelle grating plus prism |
| Simultaneous elements | up to 70 |
| Detection limit | 0.5–10 µg/L typical |
| Viewing mode | axial, radial or dual |
| RF power | 1000–1600 W |
| Argon consumption | 14–20 L/min |
| Autosampler | up to 240 positions |
Indicative values for this product class. Final specifications are confirmed on the quotation and in the calibration documents supplied with the instrument.
Applications
- Rare-earth element analysis
- Iron, steel and alloy trace analysis
- Geological and geochemical research
- Advanced materials and catalyst testing
Key features
- Echelle grating with cross-disperser prism
- Two-dimensional spectrum on a large array detector
- Resolution better than 0.005 nm in the ultraviolet
- Resolves line-rich rare-earth and iron matrices
- Simultaneous measurement of many lines
- Improved detection limits by overlap suppression
Frequently asked questions about High-Resolution Echelle ICP-OES Spectrometer
Line overlap is most serious with rare-earth elements, which emit hundreds of lines, and with iron, cobalt, nickel and tungsten-rich matrices where matrix lines fall on analyte wavelengths. It causes positive bias and poor detection limits. High resolution, alternative lines and mathematical correction mitigate it.
Higher resolution separates the analyte line from nearby lines and from continuum background, so the measured peak contains less interference and the detection limit improves. The effect is largest in line-rich matrices; for simple matrices the benefit is modest and detector noise dominates.
The two-dimensional spectrum needs a wavelength calibration across both axes, which the instrument software handles with a multi-element standard. Operation is otherwise similar to other ICP-OES systems. Alignment and detector flat-field checks are part of routine maintenance.
Radial viewing observes a thin section of the plasma, which reduces self-absorption and tolerates high dissolved solids and major elements without saturating the detector. Axial viewing looks through the plasma length for lower detection limits in clean samples. Dual-view instruments combine both, and the operator selects the view per element.
Excited atoms and ions have many energy levels, so each element emits numerous lines, some strong and some weak. The analyst selects a line free from overlap and within the working range for the expected concentration. Weak lines suit high concentrations, and strong lines suit trace levels.
Yes, in principle, using far-ultraviolet emission lines, for example chlorine at 134.7 and 135.2 nanometres, bromine and iodine lines, and sulfur and phosphorus lines. These lines require a vacuum or purged optical path because air absorbs far-ultraviolet light. Sensitivity is lower than for metals, and ICP-MS may be preferred.
Related models





