Articles | Volume 15, issue 4
https://doi.org/10.5194/essd-15-1801-2023
© Author(s) 2023. This work is distributed under the Creative Commons Attribution 4.0 License.
Ocean cross-validated observations from R/Vs L'Atalante, Maria S. Merian, and Meteor and related platforms as part of the EUREC4A-OA/ATOMIC campaign
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- Final revised paper (published on 25 Apr 2023)
- Preprint (discussion started on 09 Dec 2022)
Interactive discussion
Status: closed
Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor
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- RC1: 'Comment on essd-2022-402', Anonymous Referee #1, 08 Jan 2023
- RC2: 'Comment on essd-2022-402', Anonymous Referee #2, 05 Feb 2023
- AC1: 'Comment on essd-2022-402', Pierre L'Hégaret, 28 Feb 2023
Peer review completion
AR – Author's response | RR – Referee report | ED – Editor decision | EF – Editorial file upload
AR by Pierre L'Hégaret on behalf of the Authors (28 Feb 2023)
Author's response
Author's tracked changes
EF by Polina Shvedko (01 Mar 2023)
Manuscript
ED: Publish subject to minor revisions (review by editor) (07 Mar 2023) by Dagmar Hainbucher
AR by Pierre L'Hégaret on behalf of the Authors (08 Mar 2023)
Author's response
Author's tracked changes
Manuscript
ED: Publish as is (14 Mar 2023) by Dagmar Hainbucher
AR by Pierre L'Hégaret on behalf of the Authors (24 Mar 2023)
Manuscript
General comments:
The manuscript describes an impressive observational effort in the tropical western North Atlantic. Four research vessels joint in the EUREC4A-OA experiment and conducted measurements in the region, when also deploying autonomous vehicles. A wealth of data was acquired, based on a multitude of different sensors.
I really appreciate the effort taken in this manuscript; combining data of various sources in order to assess their quality needs thorough procedures and considerations, as described here. Nevertheless, I think the manuscript should be improved in a few points:
Since the lists above and below are rather long, I suggest a major revision of the manuscript.
Specific comments:
Ln 2: change “large-scale currents” to “regional currents”; large scale gyres are not considered here
Ln 7: add “up to 400-2000 m depth” – otherwise, readers may think that the surface (0-400 m) was not covered
Ln 15: the reference points to the dataset from L’Atalante and Maria S. Merian, however, in the first paragraph four vessels and various platforms are mentioned. Define more clearly, which data are considered here (see major comments).
Ln 28-33: the paragraph seems a little out of place and focus. It is neither a full description of the working region, nor a broad overview. Add a sentence on the importance of the AMOC for the interhemispheric exchange, connecting the tropical South and North Atlantic, and the role of NBC rings. Give references (the only reference to a paper on the region is given in line 290, which is out of place as well). A map with currents would be helpful as well. The division in two regions “east of Barbados” and “to the south” is not conclusive either, what about the rest of the box in Figure 1 (north and west of Barbados)?
Ln 45: Assuming that the lab at IFREMER is shallower than 2000 m, the derived uncertainty is probably for a certain pressure, thus 2000 dbar?
Ln 151: no lab calibration was done before and after (?) the cruise
Ln 161: I guess there were also two SBE4 sensors? Please clarify
Ln 170: add “in” before Hood et al.
Ln 216 ff: What about Meteor? Did the Meteor CTD measure oxygen, with one or two SBE43 sensors? What happened to the data?
Ln 229: “each ship” – no, Meteor was not equipped with L-ADCP, see line 135
Ln 239: I don´t think it is reasonable to call the procedures for salinity and oxygen similar for all three vessels. Ideally, this would be the case, but many differences are listed in the text above. The most important flaw is of course the missing samples from Meteor.
Ln 248-250: move to the beginning or very end of the subsection, it seems out of place here. Why -9?
Ln 266: does this statement refer to all measurements described in this subsection or to PAR sensors only?
Ln 270: again, excluding Meteor
Ln 277: I do not understand why the positioning of the CTD station was different. Please explain.
Ln 279: It is an important result that the methods agree in the final dataset. Please give more details on “no major differences” and add a figure, showing calibrated profiles from the two toolboxes.
Ln 286/287: excluding Meteor
Ln 294: it would be nice to have a table listing the final uncertainties. What uncertainty was assigned to the Meteor data?
Ln 300: one CTD profile
Ln 312: measure
Ln 314 ff: what about Meteor? Were water samples taken and analyzed?
Ln 404: does not apply to ship CTD, delete
Ln 407: what was the cut-off frequency?
Ln 431: Hz
Ln 438: the term “calibrated” does not apply to S-ADCP data. They are processed.
Ln 458: “all were equipped with Seabird CTDs” contradicts line 448 (Kraken). What are the uncertainties for the IFM and UEA gliders?
Ln 460: “some devices” – please specify which devices
Ln 472: “than 30 km” is doubled
Ln 475/476: use “larger” or “higher” rather than “stronger”
Ln 476 ff: I cannot follow the conclusion here. When the profiles of the pairs are in close vicinity to each other, variability should be small. Cannot be the missing calibration of the Meteor CTD (no salinity samples) be the cause of the large differences for the UEA gliders, which are mainly based on comparisons with Meteor?
Ln 479: delete )
Ln 488: Figure 14 j
Ln 490: was the bias corrected? What is the final uncertainty and level?
Ln 532: add “in” before Argo
Ln 534: the value 2*10-4°C seems to be unrealistically small
Ln 552/553: what is the meaning of 5-3°C and 5-2psu?
Ln 571: add CTD error for consistency
Ln 579: second column
Ln 599: add “in” before Eaton et al.
Ln 602: what about Meteor S-ADCP data?
Figure 2: add TSG to the figure (e.g. as a point in the lower left corner)
Figure 9b, 11b: Shown are calibrated profiles, please clarify in the caption
Figure 10b: in the caption, delete the extra s in “R/Vs Maria S. Merian”
Figure 17a: caption: “specific”