Articles | Volume 16, issue 22
https://doi.org/10.5194/amt-16-5609-2023
https://doi.org/10.5194/amt-16-5609-2023
Research article
 | 
22 Nov 2023
Research article |  | 22 Nov 2023

MIPAS ozone retrieval version 8: middle-atmosphere measurements

Manuel López-Puertas, Maya García-Comas, Bernd Funke, Thomas von Clarmann, Norbert Glatthor, Udo Grabowski, Sylvia Kellmann, Michael Kiefer, Alexandra Laeng, Andrea Linden, and Gabriele P. Stiller

Data sets

Envisat GOMOS Level 2 - Atmospheric constituents profiles [GOM_NL__2P] European Space Agency https://doi.org/10.57780/EN1-b655562

SMILES Data, SMILES level-2 products JAXA/ISAS https://doi.org/10.17597/ISAS.DARTS/STP-00001

MIPAS ozone retrieval version 8: middle-atmosphere measurements M. López-Puertas, M. García-Comas, B. Funke, T. von Clarmann, N. Glatthor, U. Grabowski, S. Kellmann, M. Kiefer, A. Laeng, A. Linden, and G. P. Stiller, G. P. https://doi.org/10.35097/1803

MLS/Aura Level 2 Ozone (O3) Mixing Ratio V004 M. Schwartz, L. Froidevaux, N. Livesey, and W. Read https://doi.org/10.5067/AURA/MLS/DATA2017

MLS/Aura Level 2 Ozone (O3) Mixing Ratio V005 M. Schwartz, L. Froidevaux, N. Livesey, and W. Read https://doi.org/10.5067/Aura/MLS/DATA2516

Harmonized dataset of ozone profiles from satellite limb and occultation measurements V. F. Sofieva, N. Rahpoe, J. Tamminen, E. Kyrölä, N. Kalakoski, M. Weber, A. Rozanov, C. von Savigny, A., Laeng, T. von Clarmann, G. Stiller, S. Lossow, D. Degenstein, A. Bourassa, C. Adams, C. Roth, N. Lloyd, P. Bernath, R. J. Hargreaves, J. Urban, D. Murtagh, A. Hauchecorne, F. Dalaudier, M. van Roozendael, N. Kalb, and C. Zehner https://doi.org/10.5194/essd-5-349-2013

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Short summary
This paper describes a new version (V8) of ozone data from MIPAS middle-atmosphere spectra. The dataset comprises high-quality ozone profiles from 20 to 100 km, with pole-to-pole latitude coverage for the day- and nighttime, spanning 2005 until 2012. An exhaustive treatment of errors has been performed. Compared to other satellite instruments, MIPAS ozone shows a positive bias of 5 %–8 % below 70 km. In the upper mesosphere, this new version agrees much better than previous ones (within 10 %).