MIPAS observations of ozone in the middle atmosphere

López-Puertas, Manuel; García-Comas, Maya; Funke, Bernd; Gardini, Angela; Stiller, Gabriele P.; von Clarmann, Thomas; Glatthor, Norbert; Laeng, Alexandra; Kaufmann, Martin; Sofieva, Viktoria F.; Froidevaux, Lucien; Walker, Kaley A.; Shiotani, Masato

doi:https://doi.org/10.5194/amt-11-2187-2018

Articles | Volume 11, issue 4

https://doi.org/10.5194/amt-11-2187-2018

© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.

https://doi.org/10.5194/amt-11-2187-2018

© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.

Articles | Volume 11, issue 4

Research article

|

18 Apr 2018

Research article |

| 18 Apr 2018

MIPAS observations of ozone in the middle atmosphere

Manuel López-Puertas, Maya García-Comas, Bernd Funke, Angela Gardini, Gabriele P. Stiller, Thomas von Clarmann, Norbert Glatthor, Alexandra Laeng, Martin Kaufmann, Viktoria F. Sofieva, Lucien Froidevaux, Kaley A. Walker, and Masato Shiotani

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Final revised paper (published on 18 Apr 2018)
Preprint (discussion started on 09 Jan 2018)

Interactive discussion

Status: closed

AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment

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- Supplement

RC1: 'Review of "MIPAS observations of ozone in the middle atmosphere" (amt-2017-467)', Anonymous Referee #1, 16 Jan 2018
- AC1: 'Reply RC1', Manuel López-Puertas, 09 Mar 2018
RC2: 'Comment on "MIPAS Observations of Ozone in the Middle Atmosphere" by López-Puertas et al.', Anonymous Referee #2, 25 Feb 2018
- AC2: 'Reply to RC2', Manuel López-Puertas, 09 Mar 2018

Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision

AR by Manuel López-Puertas on behalf of the Authors (09 Mar 2018) Author's response Manuscript

ED: Publish as is (18 Mar 2018) by William Ward

AR by Manuel López-Puertas on behalf of the Authors (23 Mar 2018)

Short summary

This paper describes the inversion of O₃ data from MIPAS middle atmosphere spectra which requires non-LTE. The O₃ dataset comprises from 20 to 100 km, has a pole-to-pole latitude coverage, day and nighttime, and span from 2005 until 2012. A validation of the data against other satellite measurements and an overall description of O₃ is also presented. This is an important dataset for the community and describes the major characteristics of stratospheric and mesospheric O₃.