Articles | Volume 22, issue 1
https://doi.org/10.5194/os-22-587-2026
© Author(s) 2026. This work is distributed under the Creative Commons Attribution 4.0 License.
Special issue:
Characterising marine heatwaves in the Svalbard Archipelago and surrounding seas
Download
- Final revised paper (published on 12 Feb 2026)
- Supplement to the final revised paper
- Preprint (discussion started on 04 Sep 2025)
Interactive discussion
Status: closed
Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor
| : Report abuse
-
RC1: 'Comment on egusphere-2025-4269', Anonymous Referee #1, 05 Sep 2025
- AC1: 'Reply on RC1', Marianne Williams-Kerslake, 27 Nov 2025
-
RC2: 'Comment on egusphere-2025-4269', Anonymous Referee #2, 28 Oct 2025
- AC2: 'Reply on RC2', Marianne Williams-Kerslake, 27 Nov 2025
Peer review completion
AR – Author's response | RR – Referee report | ED – Editor decision | EF – Editorial file upload
AR by Marianne Williams-Kerslake on behalf of the Authors (08 Jan 2026)
Author's response
Author's tracked changes
Manuscript
ED: Referee Nomination & Report Request started (12 Jan 2026) by Yonggang Liu
RR by Anonymous Referee #1 (19 Jan 2026)
RR by Marylou Athanase (27 Jan 2026)
ED: Publish subject to minor revisions (review by editor) (27 Jan 2026) by Yonggang Liu
AR by Marianne Williams-Kerslake on behalf of the Authors (03 Feb 2026)
Author's response
Author's tracked changes
Manuscript
ED: Publish as is (03 Feb 2026) by Yonggang Liu
AR by Marianne Williams-Kerslake on behalf of the Authors (03 Feb 2026)
Post-review adjustments
AA – Author's adjustment | EA – Editor approval
AA by Marianne Williams-Kerslake on behalf of the Authors (10 Feb 2026)
Author's adjustment
Manuscript
EA: Adjustments approved (10 Feb 2026) by Yonggang Liu
The authors presented a comprehensive MHW study in the Svalbard Archipelago region using TOPAZ analysis, which is validated by various moorings and OISST analysis. They presented MHWs changes in timescales of decade and season, vertical and horizontal extent, provided heat budget analysis for each MHW events, and concluded that the most MHWs are driven by the ocean heat transport. The manuscript is well written and can be published in EGUsphere after revision. My major concern is what drive the deep MHW, if the surface heat flux, how?
Here are my detailed comments (L=line):
L54: Use consistent time unit in L54 °C year-1, L57 %y-1, L62 °C per decade
L110, 90th percentile. I am not sure whether the region is ice free during the summer from 1991-2022. If not, how the MHWs are defined in the ice covered region, since water temperature changes a lot when ice is melted. E.g. the threshold, which is calculated using the temperature with ice in the early period, may be difficult to applied to the time when ice in melted in the later period. Can you test how much MHW features are changed if the threshold is set to 95th percentile?
L128, equation (2), why is Tref is needed?
Figures A1B, A2B and other figures with p-value: 1.43e-24, 1.27e-17, check and revise.
L211-219, Figs. A5 (low correlation) and A6 (bifurcated correlation), these figures may indicate the biases of TOPAZ model in the coastal regions.
L234, note that the intensity decreases in many regions although frequency and duration increase in most of the regions. Therefore it might be helpful to use the cumulative intensity by integrating SSTA and time in units of degree-day (e.g. Huang et al. 2025, DOI 10.1175/BAMS-D-24-0337.1), which will enable us to see how MHWs intensify with time.
L240-246, it might be helpful to add implications or causes of those features, e.g. warming is strong in winter than summer etc.
L248-252, The definition of MHW differences is not straightforward: there are many regions without MHWs in left panels marked as “missing”, which results the difference in right panel are marked as “missing” or blank. Can the “missing” in the left panels be marked as “zero”? This should make the difference more reasonable. One alternative way is to assess the differences is to integrate MHWs in space and then compare their time evolution.
L279, “Note that MHWs are not analysed north of the sea ice edge (sea ice concentration ≥ 15%).” This might be noted much earlier in definition in section 2.1.
Figures 5, 6, “peak date of each MHW”. How is this defined? MHW evolution may not be synchronized in different regions, and therefore it is not straightforward to define “one” MHW within a large region (more than one grid point). What the black dots represent?
L315, 332, “With the exception of events in 2016 and 2017 (deep events),” Does this imply that the deep MHWs are driven by the surface heat flux, which is hard to imagine. If not, what drive the deep MHWs? “With the exception of events in 2016 and 2017 (deep events),” why?
Figure 10, suggest exchange the dotted with solid lines, which will highlight the MHWs.
Section 4, Discussion, The discussion is lengthy and should be shortened.