Articles | Volume 19, issue 19
https://doi.org/10.5194/gmd-19-9325-2026
© Author(s) 2026. This work is distributed under the Creative Commons Attribution 4.0 License.
Short-lived halogen sources and chemistry in the Community Earth System Model v2 (CESM2-SLH)
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- Final revised paper (published on 05 Oct 2026)
- Supplement to the final revised paper
- Preprint (discussion started on 13 Oct 2025)
- Supplement to the preprint
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-2025-3250', Anonymous Referee #1, 08 Dec 2025
- AC1: 'Reply on RC1', Rafael Pedro Fernandez, 15 May 2026
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RC2: 'Comment on egusphere-2025-3250', Anonymous Referee #2, 12 Dec 2025
- AC2: 'Reply on RC2', Rafael Pedro Fernandez, 15 May 2026
Peer review completion
AR – Author's response | RR – Referee report | ED – Editor decision | EF – Editorial file upload
AR by Rafael Pedro Fernandez on behalf of the Authors (15 May 2026)
Manuscript
ED: Referee Nomination & Report Request started (10 Jun 2026) by Patrick Jöckel
RR by Anonymous Referee #2 (23 Jun 2026)
RR by Anonymous Referee #1 (29 Jun 2026)
ED: Publish subject to minor revisions (review by editor) (30 Jun 2026) by Patrick Jöckel
AR by Rafael Pedro Fernandez on behalf of the Authors (10 Jul 2026)
Author's response
Author's tracked changes
Manuscript
ED: Publish as is (24 Jul 2026) by Patrick Jöckel
AR by Rafael Pedro Fernandez on behalf of the Authors (24 Jul 2026)
Post-review adjustments
AA – Author's adjustment | EA – Editor approval
AA by Rafael Pedro Fernandez on behalf of the Authors (24 Sep 2026)
Author's adjustment
Manuscript
EA: Adjustments approved (24 Sep 2026) by Patrick Jöckel
The manuscript by Fernandez et al. describes the implementation of short-lived halogen chemistry already available in CESM1 into CESM2, thereby making it accessible to the broader CESM community. It provides a detailed description of the implemented SLH chemistry (incl. offline/online emissions, chemical reactions and deposition), an analysis of the SLH budgets, spatial/vertical distributions and impacts on oxidants. The analysis is very detailed and can act as benchmark evaluation for future studies using CESM2-SLH. It fits well into the scope of GMD and I see no reason why it should not be published after addressing the following minor comments.
General comments
1.
Parts of the manuscript (especially the beginning of Section 2 and Section 2.5) read a bit like a CESM user manual. The information is without doubt very useful for CESM users. However, some adaptions might help to make it easier to follow for readers outside the CESM community. The manuscript is also relatively long, so the authors might want to consider moving some more technical parts to the supplement.
Suggestions:
Abstract: Avoid using the (I think) CESM-specific term “compset” in the abstract.
l. 138 – l. 164: The authors might want to consider merging this section and Section 2.5 as some of the information is redundant (e.g. CESM branches, compsets), and it would be beneficial to have the information at the same place. Additionally, a definition/introduction of “compset” would be helpful. I understand that it is the CESM name for “simulation setup” and specifies the used BC and emissions, and settings like resolution etc.. It would be helpful if Table 6 would be referenced here (if not merged) to summarise the mentioned compsets. Additional columns could be introduced in Table 6 to explain the difference between compsets. For example, I assume that FCnudged means nudged meteorology and FCHIST historical free-running, bit it is not explained explicitly. Also the difference between FCnudged and FWnudged is not explained explicitly. What is FCASE?
l. 606: It is not clear to me what the difference between cesm2.2-asad-branch_slh and cam_cesm2_2_rel09_slh is. Could you clarify why you need two branches?
l. 610-619: Could be moved to the supplement? The information could be presented in a table listing the additional species, and if they emit, dry/wet deposit etc.
l. 662-686: Could be moved to the supplement?
Also Section 4 “Final Remarks is quite technical (e.g. l. 1602 – 1606). I think it would be valuable here to discuss if the performance of CESM2-SLH (regarding SLH budgets and impact on atmospheric composition) is similar/better/worse compared to CESM1-SLH/ CAM4-Chem, and other models including SLH chemistry.
2.
The comparison with observations is somewhat limited. In Section 3.2.2. “Evaluation of SLH Abundance with Observations” Source Gas Injection and Product Gas Injection to the stratosphere is compared to observations. It would be beneficial to extend the evaluation to SLH abundance to the (lower) troposphere, MBL or surface (for example comparison to station data). In Section 2, a comparison of VSL halocarbons to observation is mentioned (e.g. in l. 273), but no details are given.
Specific comments
Figure 2: Could you provide a bit more context on the differences in the trends of O3, OH, and NO2 between CESM2-SLH and CESM1-SLH shown in Figure 2? You explain that these differences drive differences in the trends of halogen budgets. Are the differences of O3, OH, and NO2 mainly caused by differences in prescribed boundary conditions and emissions (e.g. NOx and VOCs) or by model updates? Are differences between CESM2 and CESM1 (without SLH) similar to the differences shown here? How do the trends compare to other models and observations (e.g. are differences between CESM1 and CESM2 small compared to inter-model differences or biases towards observations)?
l. 914: An even more recent estimate for GEOS-Chem might be given by Wang et al., 2021 (https://acp.copernicus.org/articles/21/13973/2021/)
Table 9: This table provides really interesting information. Considering the following question might make it even more valuable:
Figure 16: Panels c) and f) of Figure 16 suggests that the total ozone loss is the same in FCnudged_SLH and FCnudged_NOH, and that only the contribution of different families changes. Could you confirm that this is indeed the case? It might be worth mentioning.
Technical corrections