Ozone profiles and total column amounts derived at Izaña, Tenerife Island, from FTIR solar absorption spectra, and its validation by an intercomparison to ECC-sonde and Brewer spectrometer measurements

Since February 1999 high-resolution Fourier transform infrared (FTIR) solar absorption spectra are recorded at the Izaña Observatory (28∘18′N,16∘29′W, 2370 m a.s.l.), which forms part of the network for detection of stratospheric change (NDSC). The vertical distribution of the ozone amount was deduced from the spectra by using the retrieval code PROFFIT. Two microwindows at 782.5 and 789cm-1 are used whereby an individually and regularly determined instrumental line shape (ILS) was applied. A detailed error analysis of the ozone retrieval is performed, i.e. the height-dependent impact of all important error sources on the retrieved profiles is estimated. The retrieved total column amounts and profiles as well as their estimated error budgets are verified by comparisons with column amounts and profiles derived from Brewer spectrometer and ECC-sonde measurements performed simultaneously at the same location. Whereas the mean difference of 1.9% of the FTIR total column amounts and the Brewer data lies within the precision of the instruments, systematic differences of up to 9% between FTIR and ECC-sonde profile are observed above 26km. The assumed precisions of the experiments are consistent with the experimental results, which demonstrates the excellent characterization of the FTIR data. The analysis of systematic errors allows to conclude that the systematic differences are mainly due to the sonde data since the systematic errors in the FTIR profile can only explain a small part of them.