Articles | Volume 25, issue 20
https://doi.org/10.5194/acp-25-12843-2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.The global O2 airglow field as seen by the MATS satellite: strong equatorial maximum and planetary wave influence
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- Final revised paper (published on 15 Oct 2025)
- Preprint (discussion started on 17 Apr 2025)
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-2025-1470', Anonymous Referee #1, 28 Apr 2025
- AC1: 'Reply on RC1', Björn Linder, 11 Jul 2025
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RC2: 'Comment on egusphere-2025-1470', Anonymous Referee #2, 04 May 2025
- AC2: 'Reply on RC2', Björn Linder, 11 Jul 2025
Peer review completion
AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
AR by Björn Linder on behalf of the Authors (11 Jul 2025)
Author's response
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ED: Publish as is (20 Jul 2025) by John Plane
AR by Björn Linder on behalf of the Authors (05 Aug 2025)
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This paper reports on the nature of large-scale structures observed in Feb-Apr 2023 O2 limb emissions from the MATS satellite, which is in a Sun-synchronous ascending/descending dusk/dawn (17:30/05:30) orbit. It is well-written, provides new insights into the interaction between dynamics and chemistry, and is a nice addition to the literature.
specific comments
The authors do an excellent job explaining the complexities of the measurements in terms of dependencies on ascending vs descending, dayglow vs. nightglow, solar zenith angle, and month, so that geographical dependencies in the emissions can be ascribed to the underlying atmospheric dynamics.
The authors make creative use of the CTMT vertical winds to explain the equatorial enhancements in the 17:30 LST emissions at the equator and some aspects of the latitude and longitude dependencies, although this approach is limited by the fact that the Feb-April 2023 dynamics probably differs to any unknown degree from the 7-year climatology represented by the CTMT.
The authors also credibly argue that the emissions at high latitudes are modulated by the quasi-10-day planetary wave.
The arguments put forth by the authors in the context of previously published work is at about the right level, and the references to the literature are sufficient.
In future work the authors may wish to consider looking for eastward-propagating 2d-4d period ultra-fast Kelvin wave signals in their 10S-10N VER emissions.
I recommend publication of this paper as is.
technical corrections
Figure 1 caption should explain the meaning of the grey shading and cross-hatching.