Articles | Volume 25, issue 5
https://doi.org/10.5194/acp-25-2895-2025
© Author(s) 2025. This work is distributed under the Creative Commons Attribution 4.0 License.
Ozone trends in homogenized Umkehr, ozonesonde, and COH overpass records
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- Final revised paper (published on 10 Mar 2025)
- Preprint (discussion started on 08 Jul 2024)
Interactive discussion
Status: closed
Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor
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RC1: 'Comment on egusphere-2024-1821', Anonymous Referee #1, 22 Aug 2024
- AC1: 'Reply on RC1', Irina Petropavlovskikh, 22 Oct 2024
- AC2: 'Reply on RC2', Irina Petropavlovskikh, 22 Oct 2024
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RC2: 'Comment on egusphere-2024-1821', Anonymous Referee #2, 02 Sep 2024
- AC2: 'Reply on RC2', Irina Petropavlovskikh, 22 Oct 2024
- AC1: 'Reply on RC1', Irina Petropavlovskikh, 22 Oct 2024
Peer review completion
AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
AR by Irina Petropavlovskikh on behalf of the Authors (01 Nov 2024)
Author's response
Author's tracked changes
EF by Polina Shvedko (19 Nov 2024)
Manuscript
ED: Publish as is (26 Nov 2024) by Jayanarayanan Kuttippurath
AR by Irina Petropavlovskikh on behalf of the Authors (06 Dec 2024)
Author's response
Manuscript
Review of “Ozone trends in homogenized Umkehr, Ozonesonde, and COH overpass records” by Irina Petropavlovskikh et al.
Summary and General Comments:
The authors demonstrate improvements to the LOTUS MLR ozone trends model through addition of dynamical proxies applied to ground-based (Dobson Umkehr, ozonesonde) and satellite (NOAA COH overpass and zonal) ozone datasets. Ozone trends for the lower to upper stratosphere are first presented with the “standard” Reference LOTUS model (excluding the AOD proxy) for 2000-2020, after which individual additional proxies including tropopause pressure, Eddy Heat Flux, Equivalent Latitude, etc., are added to the model to determine the best choices for a “full” model trends calculation.
The authors find that, with a few exceptions in the lower stratosphere, the trend values are mostly unchanged in the full model. However, improvements to the model adjusted R2 values and p-values indicate that the addition of proxies specifically chosen for various stations and altitudes will lead to more confidence in trend detection, as well as the possibility of detecting trends smaller in magnitude compared to a base MLR with limited proxies (i.e., as would be used with zonally averaged data).
The paper is written exceptionally well, is highly detailed, and the decision-making process for choice of additional proxies in the model and other topics are carefully explained in the text and in extensive Appendices.
I have no major concerns with this manuscript, but I do wonder if the authors explored using the Payerne ozonesonde record in addition to the Hohenpeissenberg record for the Arosa/Davos station. The Payerne record is also extremely dense, Payerne is only 50 km farther in distance from Arosa/Davos, and that is an ECC record that does not have a correction factor applied as with the Hohenpeissenberg Brewer-Mast type ozonesondes. The inclusion of Payerne sonde trends could be illuminating.
Recommendation:
I recommend publication of this paper and have only minor and technical comments below.
Specific and Line-by-Line Comments:
Line 117 and 118: It looks like there are some extra parentheses on these lines.
Line 127: SHADOZ is “Southern Hemisphere Additional Ozonesondes”
Line 133: The vertical resolution of ozonesonde data is a factor of the time response of the instrument, not altitude.
Table 1: If using the OHP ozonesonde data from NDACC, I am assuming you are using the homogenized “Corrected Ozone partial pressure” ozone values in those files, correct?
Table 2: NOAA 11 appears twice in this Table.
Line 263: I think you are missing a “m =” here
Line 362: Change “interannual” to “interannually”
Line 413: The OHP sonde and Umkehr trend differences look quite large for all Layers 3-5 (not just 4), although always within the 2 standard errors.
Figures 3 and 5: Suggest changing “Height (hPa)” to “Pressure (hPa)”
Line 528: I’m not sure I would say the results point to the inability of the model to detect non-zero trends. At this point we really don’t know and probably cannot say that trends are non-zero here in Layer 6.
Line 606 and 794: “lower” stratospheric ozone records…
Table 13: A plot similar to Figure 7 with the adjusted R2 values, but for the p-values for the Ref and Full models could be helpful and would keep the reader from having to flip back and forth between the two Tables 6 and 13.
Lines 866-869: I think it would be useful to put these questions in the intro as well (or just move them there) to very clearly motivate this study.
Line 901: Change “in case of” to “for”