TY  - JOUR
  - Darby, SB,Smith, PD,Venables, DS
  - 2012
  - January
  - Analyst
  - Cavity-enhanced absorption using an atomic line source: application to deep-UV measurements
  - Validated
  - WOS: 13 ()
  - RING-DOWN SPECTROSCOPY LASER ULTRAVIOLET MERCURY SPECTRA LIQUIDS PHASE N2O5 NO3
  - 137
  - 2318
  - 2321
  - Optical cavities are commonly used to increase the sensitivity of absorption measurements, but have not been extensively used below 300 nm, mainly owing to the limited light sources at these wavelengths. While some progress has been made using cavity ring-down spectroscopy, these systems rely on complex and expensive lasers. Here we investigate an approach combining Cavity-Enhanced Absorption Spectroscopy (CEAS) with an inexpensive low vapour pressure mercury lamp for sensitive absorption measurements at 253.7 nm. We demonstrate that the CEAS absorption in our system is 50 times greater than the absorption found in a single-pass configuration; using this approach, we obtained limits of detection of 8.1 pptv (66 ng m(-3)) for gaseous elemental mercury and 8.4 ppbv for ozone. We evaluate the performance of the system and discuss potential improvements and applications of this approach.
  - http://hdl.handle.net/10468/786
  - 10.1039/c2an35149h
DA  - 2012/01
ER  - 

@article{V146554526,
   = {Darby,  SB and Smith,  PD and Venables,  DS },
   = {2012},
   = {January},
   = {Analyst},
   = {Cavity-enhanced absorption using an atomic line source: application to deep-UV measurements},
   = {Validated},
   = {WOS: 13 ()},
   = {RING-DOWN SPECTROSCOPY LASER ULTRAVIOLET MERCURY SPECTRA LIQUIDS PHASE N2O5 NO3},
   = {137},
  pages = {2318--2321},
   = {{Optical cavities are commonly used to increase the sensitivity of absorption measurements, but have not been extensively used below 300 nm, mainly owing to the limited light sources at these wavelengths. While some progress has been made using cavity ring-down spectroscopy, these systems rely on complex and expensive lasers. Here we investigate an approach combining Cavity-Enhanced Absorption Spectroscopy (CEAS) with an inexpensive low vapour pressure mercury lamp for sensitive absorption measurements at 253.7 nm. We demonstrate that the CEAS absorption in our system is 50 times greater than the absorption found in a single-pass configuration; using this approach, we obtained limits of detection of 8.1 pptv (66 ng m(-3)) for gaseous elemental mercury and 8.4 ppbv for ozone. We evaluate the performance of the system and discuss potential improvements and applications of this approach.}},
   = {http://hdl.handle.net/10468/786},
   = {10.1039/c2an35149h},
  source = {IRIS}
}