Atmos. Chem. Phys. Discuss., 8, 3027-3142, 2008
www.atmos-chem-phys-discuss.net/8/3027/2008/
doi:10.5194/acpd-8-3027-2008
© Author(s) 2008. This work is distributed
under the Creative Commons Attribution 3.0 License.
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This discussion paper has been under review for the journal Atmospheric Chemistry and Physics (ACP). Please refer to the corresponding final paper in ACP.
Validation of NO2 and NO from the Atmospheric Chemistry Experiment (ACE)
T. Kerzenmacher1, M. A. Wolff1, K. Strong1, E. Dupuy2, K. A. Walker1,2, L. K. Amekudzi3, R. L. Batchelor1, P. F. Bernath2,4, G. Berthet5, T. Blumenstock6, C. D. Boone2, K. Bramstedt3, C. Brogniez7, S. Brohede8, J. P. Burrows3, V. Catoire5, J. Dodion9, J. R. Drummond1,10, D. G. Dufour11, B. Funke12, D. Fussen9, F. Goutail13, D. W. T. Griffith14, C. S. Haley15, F. Hendrick9, M. Höpfner6, N. Huret5, N. Jones14, J. Kar1, I. Kramer6, E. J. Llewellyn16, M. López-Puertas12, G. Manney17,18, C. T. McElroy1,19, C. A. McLinden19, S. Melo20, S. Mikuteit6, D. Murtagh8, F. Nichitiu1, J. Notholt3, C. Nowlan1, C. Piccolo21, J.-P. Pommereau13, C. Randall22, P. Raspollini23, M. Ridolfi24, A. Richter3, M. Schneider6, O. Schrems25, M. Silicani20, G. P. Stiller6, J. Taylor1, C. Tétard7, M. Toohey1, F. Vanhellemont9, T Warneke3, J. M. Zawodny26, and J. Zou1
1Department of Physics, University of Toronto, Toronto,Ontario, Canada
2Department of Chemistry, University of Waterloo, Waterloo, Ontario, Canada
3Institute of Environmental Physics, Institute of Remote Sensing, Universität Bremen, Germany
4Department of Chemistry, University of York, Heslington, York, U.K.
5Laboratoire de Physique et Chimie de l'Environnement, CNRS – Université d'Orléans, Orléans, France
6Forschungszentrum Karlsruhe and Universität Karlsruhe, Institut für Meteorologie und Klimaforschung (IMK), Karlsruhe, Germany
7Laboratoire d'Optique Atmosphérique, Universitédes sciences et technologies de Lille, Villeneuve d'Ascq, France
8Department of Radio and Space Science, Chalmers University of Technology, Göteborg, Sweden
9Belgisch Instituut voor Ruimte-Aëronomie – Institut d'Aéronomie Spatiale de Belgique (IASB-BIRA), Bruxelles, Belgium
10Department of Physics & Atmospheric Science, Dalhousie University, Halifax, Nova Scotia, Canada
11Picomole Instruments Inc., Edmonton, Alberta, Canada
12Instituto de Astrofísica de Andalucía, CSIC, Granada, Spain
13Service d'aéronomie – CNRS, Verrières-le-Buisson, France
14School of Chemistry, University of Wollongong, Australia
15Centre for Research in Earth and Space Science, York University, Toronto, Ontario, Canada
16Institute of Space and Atmospheric Studies, University of Saskatchewan, Saskatoon, Saskatchewan, Canada
17Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
18New Mexico Institute of Mining and Technology, Socorro, New Mexico, USA
19Environment Canada, Downsview, Ontario, Canada
20Canadian Space Agency, St Hubert, Quebec, Canada
21Atmospheric, Oceanic and Planetary Physics, University of Oxford, Oxford, UK
22Laboratory for Atmospheric and Space Physics & Department of Atmospheric and Oceanic Sciences, University of Colorado, Boulder, Colorado, USA
23Istituto di Fisica Applicata “Nello Carrara” (IFAC) del Consiglio Nazionale delle Ricerche (CNR), Firenze, Italy
24Dipartimento di Chimica Fisica e Inorganica, Universitá di Bologna, Bologna, Italy
25Alfred Wegener Institute for Polar and Marine Research, Bremerhaven, Germany
26NASA Langley Research Center, Hampton, Virginia, USA

Abstract. Vertical profiles of NO2 and NO have been obtained from solar occultation measurements by the Atmospheric Chemistry Experiment (ACE), using an infrared Fourier Transform Spectrometer, ACE-FTS, and an ultraviolet-visible-near-infrared spectrometer, MAESTRO (Measurement of Aerosol Extinction in the Stratosphere and Troposphere Retrieved by Occultation). In this paper, the quality of the ACE-FTS version 2.2 NO2 and NO and the MAESTRO version 1.2 NO2 data are assessed using other solar occultation measurements (HALOE, SAGE II, SAGE III, POAM III, SCIAMACHY), stellar occultation measurements (GOMOS), limb measurements (MIPAS, OSIRIS), nadir measurements (SCIAMACHY), balloon measurements (SPIRALE, SAOZ) and ground-based measurements (UV-VIS, FTIR). Time differences between the comparison measurements were reduced using either a tight coincidence criterion, or where possible, chemical box models. ACE-FTS NO2 and NO and the MAESTRO NO2 are generally consistent with the correlative data. The ACE-FTS NO2 VMRs agree with the satellite data sets to within about 20% between 25 and 40 km, and suggest a negative bias between 23 and 40 km of about \textminus10%. In comparisons with HALOE, ACE-FTS NO VMRs typically agree to ±8% from 22 to 64 km and to +10% from 93 to 105 km. Partial column comparisons for NO2 show that there is fair agreement between the ACE instruments and the FTIRs, with a mean difference of +7.3% for ACE-FTS and +12.8% for MAESTRO.

Citation: Kerzenmacher, T., Wolff, M. A., Strong, K., Dupuy, E., Walker, K. A., Amekudzi, L. K., Batchelor, R. L., Bernath, P. F., Berthet, G., Blumenstock, T., Boone, C. D., Bramstedt, K., Brogniez, C., Brohede, S., Burrows, J. P., Catoire, V., Dodion, J., Drummond, J. R., Dufour, D. G., Funke, B., Fussen, D., Goutail, F., Griffith, D. W. T., Haley, C. S., Hendrick, F., Höpfner, M., Huret, N., Jones, N., Kar, J., Kramer, I., Llewellyn, E. J., López-Puertas, M., Manney, G., McElroy, C. T., McLinden, C. A., Melo, S., Mikuteit, S., Murtagh, D., Nichitiu, F., Notholt, J., Nowlan, C., Piccolo, C., Pommereau, J.-P., Randall, C., Raspollini, P., Ridolfi, M., Richter, A., Schneider, M., Schrems, O., Silicani, M., Stiller, G. P., Taylor, J., Tétard, C., Toohey, M., Vanhellemont, F., Warneke, T, Zawodny, J. M., and Zou, J.: Validation of NO2 and NO from the Atmospheric Chemistry Experiment (ACE), Atmos. Chem. Phys. Discuss., 8, 3027-3142, doi:10.5194/acpd-8-3027-2008, 2008.
 
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