Agilent Vista Axially Viewed ICP-OES Application Note

This paper reviews the latest advances in axially viewed simultaneous ICP-OES for elemental analysis, including improvements in detector design, software, and sample introduction systems.


Agilent Vista Axially Viewed ICP-OES Application Note - cover page
Brand
Agilent
Category
Other
Document type
Application Note
Language
English
Pages
10
File format
PDF
File size
1.1 MB
Published
12 June, 2012
Updated
29 September, 2023
MD5 checksum
6B7306F01FA4A3BB77153BE57D5EA33E

About this manual

This document discusses the evolution of Inductively Coupled Plasma Optical Emission Spectrometry (ICP-OES) from radial viewing to axially viewed systems. It highlights how modern Agilent Vista systems overcome historical limitations regarding injector tube blockage and linear dynamic range. The text details the transition from photomultiplier tubes and segmented array CCDs to advanced VistaChip and Vista-MPX detectors that offer simultaneous detection with wide dynamic ranges.

What's inside

  • Author Background
  • Advances in ICP-OES Detector Design
  • Advances in Axial Viewing Systems
  • VistaChip CCD
  • Vista-MPX
  • Cooled Cone Interface
  • Detection Limits Comparison

Specifications

VistaChip CCD spectral coverage96% of the analytical spectrum
Vista-MPX pixel countover 1.1 million pixels
Axial viewing sensitivity improvement4-10x improvement
CCI argon gas flow requirement2.5 L/min

Frequently asked questions

What is the main advantage of axially viewed ICP-OES over radial viewing?

Axially viewed systems provide improved signal to noise ratio and better detection limits by observing a longer path length in the analyte-rich central channel.

How does the VistaChip CCD differ from earlier segmented array designs?

The VistaChip uses over 70,000 pixels positioned to exactly match the free spectral range, providing 96% coverage compared to the 5.7% coverage of segmented array designs.

What is the benefit of Agilent's Cooled Cone Interface (CCI)?

The CCI displaces the cooler tail flame of the plasma away from the optical path, resulting in greater linear dynamic range and a significant reduction in atomization and recombination interferences.

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