Cavity Enhanced Absorption Spectroscopy (CEAS) for Ozone Detection

Cavity Enhanced Absorption Spectroscopy (CEAS) for Ozone Detection (GSC-TOPS-214)
A pulsed light emitting diode (LED) configured to emit a light towards a photomultiplier tube (PMT).
Engineers at NASA's Goddard Space Flight Center tasked with measuring atmospheric Ozone, an important pollutant and greenhouse gas, quickly discovered that existing optical instrumentation would not be sufficient to achieve their performance requirements. Specifically, the current systems did not possess the precision necessary to make low concentration measurements at fast time resolution. This innovation utilizes Cavity Enhanced Absorption Spectroscopy (CEAS) with a simple and inexpensive optical and electrical design to overcome these limitations and achieve high quality Ozone measurements. The sensitivity of the instrument developed using CEAS exceeds that of commercially available instrumentations, and matches performance of complex chemiluminescence instruments.

The Technology
This technique takes advantage of Ozone's strong absorption at specific wavelengths in the UltraViolet (UV). To take measurements, UV light is projected through a cell bounded by highly reflective mirrors. These mirrors increase the path length of the cell by inducing the light to bounce back and forth within the cell, increasing the likelihood of Ozone absorption within the cell. Finally, an absorption measurement is taken via a detector outside the cell and opposite of the UV source. This innovation produces an ozone detection precision of 0.12 parts per billion (ppb) in 0.1 second integration. This corresponds to 0.012 ppb in ten seconds integration.
The yearly depletion of stratospheric ozone over Antarctica  more commonly referred to as the ozone hole
  • High precision allows detection of low concentrations
  • Fast time resolutions
  • Reduced parts lead to simple and inexpensive

  • Spectroscopy
  • Environmental Monitoring
Technology Details

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