Validation of ozone measurements from the Atmospheric Chemistry Experiment (ACE)
Authors: Dupuy E. , Walker K. A. , Kar J. , Boone C. D. , McElroy C. T. , Bernath P. F. , Drummond J. R. , Skelton R. , McLeod S. D. , Hughes R. C. , Nowlan C. R. , Dufour D. G. , Zou J. , Nichitiu F. , Strong K. , Baron P. , Bevilacqua R. M. , Blumenstock T. , Bodeker G. E. , Borsdorff T. , Bourassa A. E. , Bovensmann H. , Boyd I. S. , Bracher A. , Brogniez C. , Burrows J. P. , Catoire V. , Ceccherini S. , Chabrillat S. , Christensen T. , Coffey M. T. , Cortesi U. , Davies J. , De Clercq C. , Degenstein D. A. , De Mazière M. , Demoulin P. , Dodion J. , Firanski B. , Fischer H. , Forbes G. , Froidevaux L. , Fussen D. , Gerard P. , Godin-Beekman S. , Goutail F. , Granville J. , Griffith D. , Haley C. S. , Hannigan J. W. , Höpfner M. , Jin J. J. , Jones A. , Jones N. B. , Jucks K. , Kagawa A. , Kasai Y. , Kerzenmacher T. E. , Kleinböhl A. , Klekociuk A. R. , Kramer I. , Küllmann H. , Kuttippurath J. , Kyrölä E. , Lambert J.-C. , Livesey N. J. , Llewellyn E. J. , Lloyd N. D. , Mahieu E. , Manney G. L. , Marshall B. T. , McConnell J. C. , McCormick M. P. , McDermid I. S. , McHugh M. , McLinden C. A. , Mellqvist J. , Mizutani K. , Murayama Y. , Murtagh D. P. , Oelhaf H. , Parrish A. , Petelina S. V. , Piccolo C. , Pommereau J.-P. , Randall C. E. , Robert C. , Roth C. , Schneider M. , Senten C. , Steck T. , Strandberg A. , Strawbridge K. B. , Sussmann R. , Swart D. P. J. , Tarasick D. W. , Taylor J. R. , Tétard C. , Thomason L. W. , Thompson A. M. , Tully M. B. , Urban J. , Vanhellemont F. , von Clarmann T. , von der Gathen P. , von Savigny C. , Waters J. W. , Witte J. C. , Wolff M. , Zawodny J. M. 
Published: April 2010

Abstract. This paper presents extensive validation analyses of ozone observations from the Atmospheric Chemistry Experiment (ACE) satellite instruments: the ACE Fourier Transform Spectrometer (ACE-FTS) and the Measurement of Aerosol Extinction in the Stratosphere and Troposphere Retrieved by Occultation (ACE-MAESTRO) instrument. The ACE satellite instruments operate in the mid-infrared and ultraviolet-visible-near-infrared spectral regions using the solar occultation technique. In order to continue the long-standing record of solar occultation measurements from space, a detailed quality assessment is required to evaluate the ACE data and validate their use for scientific purposes. Here we compare the latest ozone data products from ACE-FTS and ACE-MAESTRO with coincident observations from satellite-borne, airborne, balloon-borne and ground-based instruments, by analysing volume mixing ratio profiles and partial column densities. The ACE-FTS version 2.2 Ozone Update product reports more ozone than most correlative measurements from the upper troposphere to the lower mesosphere. At altitude levels from 16 to 44 km, the mean differences range generally between 0 and +10% with a slight but systematic positive bias (typically +5%). At higher altitudes (45–60 km), the ACE-FTS ozone amounts are significantly larger than those of the comparison instruments by up to ~40% (typically +20%). For the ACE-MAESTRO version 1.2 ozone data product, agreement within ±10% (generally better than ±5%) is found between 18 and 40 km for the sunrise and sunset measurements. At higher altitudes (45–55 km), systematic biases of opposite sign are found between the ACE-MAESTRO sunrise and sunset observations. While ozone amounts derived from the ACE-MAESTRO sunrise occultation data are often smaller than the coincident observations (by as much as −10%), the sunset occultation profiles for ACE-MAESTRO show results that are qualitatively similar to ACE-FTS and indicate a large positive bias (+10 to +30%) in this altitude range. In contrast, there is no significant difference in bias found for the ACE-FTS sunrise and sunset measurements. These systematic effects in the ozone profiles retrieved from the measurements of ACE-FTS and ACE-MAESTRO are being investigated. This work shows that the ACE instruments provide reliable, high quality measurements from the tropopause to the upper stratosphere and can be used with confidence in this vertical domain.