Atmospheric Chemistry and Physics www.atmos-chem-phys.net 1680-7316 1680-7324 10 3 2010 10.5194/acp-10-1133-2010 http://www.atmos-chem-phys.net/10/1133/2010/ http://www.atmos-chem-phys.net/10/1133/2010/acp-10-1133-2010.html http://www.atmos-chem-phys.net/10/1133/2010/acp-10-1133-2010.pdf 1133 1153 2010-02-03 First multi-year occultation observations of CO₂ in the MLT by ACE satellite: observations and analysis using the extended CMAM S. R. Beagley beagley@nimbus.yorku.ca C. D. Boone V. I. Fomichev J. J. Jin K. Semeniuk J. C. McConnell P. F. Bernath Department of Earth and Space Science and Engineering, York University, Toronto, Ontario, Canada Department of Chemistry, University of Waterloo, Waterloo, Ontario, Canada Department of Chemistry, University of York, Heslington, York, UK currently at: Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA This paper presents the first global set of observations of CO₂ in the mesosphere and lower thermosphere (MLT) obtained by the ACE-FTS instrument on SCISAT-I, a small Canadian satellite launched in 2003. The observations use the solar occultation technique and document the fall-off in the mixing ratio of CO₂ in the MLT region. The beginning of the fall-off of the CO₂, or "knee" occurs at about 78 km and lies higher than in the CRISTA-1 measurements (~70 km) but lower than in the SABER 1.06 (~80 km) and much lower than in rocket measurements. We also present the measurements of CO obtained concurrently which provide important constraints for analysis. We have compared the ACE measurements with simulations of the CO₂ and CO distributions in the vertically extended version of the Canadian Middle Atmosphere Model (CMAM). Applying standard chemistry we find that we cannot get agreement between the model and ACE CO₂ observations although the CO observations are adequately reproduced. There appears to be about a 10 km offset compared to the observed ACE CO₂, with the model "knee" occurring too high. In analyzing the disagreement, we have investigated the variation of several parameters of interest (photolysis rates, formation rate for CO₂, and the impact of uncertainty in turbulent eddy diffusion) in order to explore parameter space for this problem. 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