Open path monitoring of the atmosphere can be carried out using FTIR-spectr
ometers, for which high sensitive, nitrogen cooled mercury-cadmium-tellurid
e (MCT) detectors are routinely employed. Because of non-linearities in the
MCT-detector response during the interferogram measurement and not correct
ly compensated ambient blackbody emission, photometric inaccuracies arise f
or mainly employed bistatic instruments with the unmodulated source radiati
on being attenuated by atmospheric infrared absorbing species. Especially,
the mid-infrared fingerprint-range is affected where many pollutants have t
heir strongest spectral signatures. An important example is the determinati
on of benzene in atmospheric air using the strong Q-branch absorption at 67
3.9 cm(-1), which is severely overlapped by the vl band of carbondioxide. (
C) 1999 Elsevier Science B.V. All rights reserved.