Key Performance Advantages：
1. Wide Wavelength Range (175–900 nm) for Full-Element Coverage
The combination of a mid-step grating + prism cross-dispersion system offers high energy throughput and exceptional resolution.
Easily covers typical wavelengths of trace elements including As, Pb, Cd, Cr, Ni, Ce, Sn, Pd, Ru, Si, Ag, Bi, K, Ca, Mg, I, Cl
Ideal for clients needing multi-matrix, multi-element analysis
2. High-Sensitivity -45°C Deep-Cooled CCD Detector
The CCD detector (165–900 nm) is cooled to –45°C, drastically reducing dark noise.
Quantum efficiency >30% @ 200 nm
Ensures stable, low-noise signals for both major and trace elements
Suitable for ppm to sub-ppm precision requirements
3. High Throughput for Multi-Element Laboratories
Simultaneous full-spectrum acquisition
Suitable for laboratories measuring 50–70+ elements per run
Ultra-fast nitrogen purging system (3–6 L/min) ensures stable vacuum-free UV detection
This helps laboratories shorten testing cycles while maintaining excellent precision.
4. Exceptional Stability & Repeatability
5. Robust Optical Architecture for Long-Term Reliability
440 mm focal length
Mid-step grating ensures high spectral resolution
Prism cross-dispersion eliminates spectral overlaps
Nitrogen flow system protects UV optics and extends their lifespan
Designed for demanding industrial environments.
6. Intelligent Software for Modern Laboratories
Our system includes an intuitive, multilingual ICP workstation designed for fast training and efficient workflows.
Built-in spectral library
Automatic wavelength selection
Customizable reporting templates
Supports LIMS integration
- Multi-user permission management
Typical Applications
Battery materials (Li, Ni, Co, Mn, Fe, Al, Cu, impurities)
Semiconductor and electronics-grade materials
Environmental water & soil monitoring
Rare earth & precious metals
Petrochemical additives and catalysts
Food and pharmaceutical elemental safety testing
Fertilizers and agricultural analysis
