Atmospheric Chemistry and Physics www.atmos-chem-phys.net 1680-7316 1680-7324 7 10 2007 10.5194/acp-7-2671-2007 http://www.atmos-chem-phys.net/7/2671/2007/ http://www.atmos-chem-phys.net/7/2671/2007/acp-7-2671-2007.html http://www.atmos-chem-phys.net/7/2671/2007/acp-7-2671-2007.pdf 2671 2690 2007-05-22 Evaluation of ozonesondes, HALOE, SAGE II and III, Odin- OSIRIS and -SMR, and ENVISAT-GOMOS, -SCIAMACHY and -MIPAS ozone profiles in the tropics from SAOZ long duration balloon measurements in 2003 and 2004 F. Borchi borchi@aerov.jussieu.fr J.-P. Pommereau CNRS, Service d'Aéronomie, Verrières le Buisson, France The performances of satellite and sondes ozone measuring instruments available in the tropics between 10 and 26 km during the southern hemisphere summer in 2003 and 2004, have been investigated by comparison with series of profiles obtained by solar occultation in the visible Chappuis bands using a SAOZ UV-Vis spectrometer carried by long duration balloons. When compared to SAOZ, systematic positive or negative altitude shifts are observed in the satellite profiles, varying from <50 m for the GOMOS v6.0b stellar occultation instrument, followed by +100/200 m for solar occultation systems (SAGE II v6.2, HALOE v19 above 22 km), but as large as −900 m for the OSIRIS limb viewing system. The ozone relative biases are generally limited, between −4% and +4%, for measurements in the visible Chappuis bands (SAGE II and SAGE III moon v3, GOMOS above 22 km and OSIRIS), the near IR (HALOE above 22 km) and the ozonesondes, but increase to +5.5% (SCIAMACHY IUP v1.63) though still in the visible, and +7% in the mid-IR (MIPAS NL v4.61) and the submillimetric range (SMR v222). 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