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Field FTIR Measurements

Continuous Sampling

Open Path FTIR

Stable Isotopes

Solar IR Remote Sensing

Solar UV-B

Aerosol Optics

Chemical Transport Modeling

Solar  UV-B Spectroscopy

 

UV-B radiation provides the energy for many reactions in atmospheric chemistry. For instance, both CO and methane are removed from the clean atmosphere as a result of reaction with the hydroxyl radical. In this environment this is primarily generated by UV-B radiation.

Dr. Stephen Wilson is the lead Scientist responsible for UV-B measurements at the Cape Grim Baseline Air Pollution Station, situated in north-western Tasmania.

This research involves both the development and validation of measurement techniques and the interpretation of the results as they impact upon the clean air environment.

 

  
Photo: Bureau of Meteorology/ R. Bennett

We are also developing small UV and Visible diode array spectrometers to allow the determination of UV-B and aerosol optical properties.
  Last reviewed: 24 May, 2007 
 
University of Wollongong
Wollongong NSW 2522 Australia
Telephone +61 2 4221 3555

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