Articles | Volume 25, issue 19
https://doi.org/10.5194/acp-25-11673-2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.Investigating the ability of satellite occultation instruments to monitor possible geoengineering experiments
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- Final revised paper (published on 30 Sep 2025)
- Preprint (discussion started on 14 Mar 2025)
Interactive discussion
Status: closed
Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor
| : Report abuse
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CC1: 'Comment on egusphere-2025-1005', Travis N. Knepp, 14 Mar 2025
- AC1: 'Reply on CC1', Anna Lange, 02 Jun 2025
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RC1: 'Comment on egusphere-2025-1005', Anonymous Referee #1, 08 Apr 2025
- AC2: 'Reply on RC1', Anna Lange, 02 Jun 2025
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RC2: 'Comment on egusphere-2025-1005', Anonymous Referee #2, 15 Apr 2025
- AC3: 'Reply on RC2', Anna Lange, 02 Jun 2025
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RC3: 'Comment on egusphere-2025-1005', Anonymous Referee #3, 25 Apr 2025
- AC4: 'Reply on RC3', Anna Lange, 02 Jun 2025
Peer review completion
AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
AR by Anna Lange on behalf of the Authors (02 Jun 2025)
Author's response
Author's tracked changes
Manuscript
ED: Referee Nomination & Report Request started (04 Jun 2025) by Marc von Hobe
RR by Anonymous Referee #2 (24 Jun 2025)

RR by Anonymous Referee #3 (30 Jun 2025)

ED: Publish subject to minor revisions (review by editor) (01 Jul 2025) by Marc von Hobe

AR by Anna Lange on behalf of the Authors (11 Jul 2025)
Author's response
Author's tracked changes
Manuscript
ED: Publish as is (01 Aug 2025) by Marc von Hobe

AR by Anna Lange on behalf of the Authors (01 Aug 2025)
Manuscript
Hello Anna! Thank you for submitting this paper.
The authors present a non-sophisticated (simplicity is beauty), simple evaluation of a solar occultation instrument's (here, SAGE III/ISS) ability to detect changes in stratospheric aerosol load with a continual injection of 1-2 Tg S/year. This study is elegant in its simplicity. Here, the authors determine that such changes would be detectable. To carry out this study the authors use MAECHAM5-HAM model to generate extinction coefficients at 500 and 550 nm, which were then converted to 520 nm (via Angstrom parameterisation), which was then fed into SCIATRAN to produce transmission data, which was then used to retrieve 520 nm extinction. I believe the accuracy of the authors' conclusions depends on the quality of these models, which I am not qualified to judge.
Overall, this paper is well written and I believe makes an important contribution to the scientific community. It would be interesting to see this study continue to evolve (e.g., if your "natural variability" included pyrocbs and volcanic eruptions (i.e., the stratospheric conditions that SAGE III/ISS has observed under), would you still have the requisite sensitivity to detect changes?; by continually injecting S you are changing the baseline stratospheric aerosol distribution...how does that impact particle growth and radiative transfer after another eruption, etc.), but the authors present an interesting and convincing proof of concept that stands on its own.
I only have minor suggestions for improving the paper.
1. In Fig. 1 (b), when does injection start? Did it start in January? I apologize if this was mentioned in the text and I missed it, but adding this information to the caption would aid the reader.
2. For Figures 2, 4, 5, 9, have the authors considered making the x-axis scale logarithmic? Especially in Fig. 4/5 this would help the reader appreciate the magnitude of change from background to enhanced conditions. Currently, I can barely tell that background is different from zero and a log scale would help the reader quantify this.
3. Do you have any information on how particle size may change with these injections? That level of information would be very interesting (at least to me).
Again, well done on the paper. I look forward to seeing this published; best of luck.