the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Improving ocean bottom pressure fields using space gravity data in state estimation
Abstract. Ocean bottom pressure (pb) is critical for monitoring and understanding ocean variability, yet global observations from GRACE and GRACE Follow-On suffer from limited spatiotemporal coverage. State estimation methods allow for the dynamical interpolation of sparse data by optimally combining observations with models. Here we examine the effects of assimilating GRACE data (local pb anomalies and global mean), along with other datasets, on state estimates produced by the project for Estimating the Circulation and Climate of the Ocean (ECCO). The ECCO optimization leads to large adjustments in pb fields at monthly and longer timescales. A substantial part of those adjustments is directly induced by GRACE constraints, with largest impacts occurring at high latitudes. Additionally, the mean ocean mass constraint is essential for mitigating large imbalances in freshwater fluxes derived from atmospheric reanalyses (used as prior forcing) and for producing a realistic barystatic sea level curve. Interpretation of remaining ECCO and GRACE differences highlights issues with non-oceanographic data signals. Our findings indicate that GRACE data contain information complementary to that available in other datasets, quantifying their value for determining pb and associated circulation fields.
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Status: open (until 21 Apr 2026)
- RC1: 'Comment on egusphere-2026-947', Detlef Stammer, 15 Mar 2026 reply
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RC2: 'Comment on Ponte et al., "Improving ocean bottom pressure fields..."', Don Chambers, 19 Mar 2026
reply
Like Professor Stammer, I also feel this paper is worth publishing after some revisions are made. My major concerns (as indicated in the point-by-point comments below) concern the lack of some quantified statistics in the discussion. The discussion throughout could be improved by giving explicit values of differences (e.g., X% of the oceans have a change > 1 cm RMS).
It is a shame that the authors do not have an assimilation run on hand that was done in the same framework without assimilating GRACE data. I understand the reason why (computation costs are expensive), but I do encourage the authors to consider Dr. Stammer’s suggestion on a potential way forward by considering an older run (in a slightly different assimilation framework) and comparing for that specific period around 2002 when GRACE data is introduced. This would provide the best evidence that it’s not Argo profile measurements that cause the change at that period.
With that said, I do find Figure 8 and 9 compelling evidence that it is GRACE that drives the improvement. However, I note the evidence that suggests this is the gap between the end of GRACE and the start of GRACE-FO, but this is not explicitly discussed in the section (see Point 9 below). I encourage the authors to take another look at this particular time-period and perhaps do some additional analysis on it to tease out the GRACE improvements further with the data they have.
Point-by-Point Comments
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- Although the figure captions clarify that global means are removed before computing Pb variance, this should be discussed more in the text as to why this is done – i.e., there is a ± 1-2 cm variation in global mass (barystatic sea level), primarily with seasonal periods but also a trend. By removing monthly global means, the authors are focusing on the dynamic ocean mass variations, not geodetic. This information is glossed over in the introduction and data description but should be discussed.
- Lines 115-120: “In areas of western boundary currents (e.g., Agulhas retroflection, Gulf Stream extension, Argentine Basin), GRACE fields look more energetic than both ECCOv4r5 and ECCOctrl, consistent with the presence in GRACE of eddy variability that cannot be represented in either ECCOv4r5 or ECCOctrl, as discussed in relation to Figure 1a”. Some more discussion is warranted here. For example, the authors should reference previous works (e.g., Fu’s studies in the Argentine Basin) indicating there are known and large variation is barotropic sea level (Pb) at mesoscales in these regions. While the ECCO resolution can’t capture the magnitude of Pb variance due to the resolution, GRACE does capture more of it. I doubt GRACE is capturing the full magnitude or resolving the mesoscale signals, but it does likely have information there that ECCO is not capturing. It should also be noted that the GRACE data is explicitly down-weighted in these regions (see Figure 1a), which may explain why it has limited influence on ECCO there.
- Some quantification should be added in the discussion around Figure 2, especially Figure 2d. For example, what are the values of RMSD in certain areas (e.g., the Weddell Sea). The color bars make it difficult to see a difference between 2.5 and 1.5 cm, for instance. It may be that even though the change looks small, it still may be significant. This is shown to some extent in Figure 2d, but the authors need to guide the reader a little more on what the negative vs. positive values mean – e.g., negative means the assimilation pulled it closer to GRACE while positive pulled it away. Also, please add some statistics: what percentage of the ocean improved? By how much? What was the average RMSD increase in smaller areas where there is a larger change.
- I understand the “Model Cost” concept, but I wonder if expressing it int erms of percent variance reduced/explained (or a similar metric) would be understood by a broader audience. Remember, this is not just being written for modelers or experts on data assimilation.
- I notice there is no discussion of correlation. My first thought reading this is does the temporal correlation in each grid improve with assimilation? And by how much? I suggest adding some analysis on this.
- One aspect of the trends in the control run that are not mentioned but are quite obvious to me is the negative trend throughout the Atlantic much of the Southern Ocean and positive trends throughout the Indian and Pacific Oceans north of north of about 60°S. This indicates a relatively large exchange of mass between those basins, enough to cause a change of ± 6 cm over the 20+ year period! This is indicative of a large-scale drift in the control run which is fixed via the assimilation. While there are some mentions of changes in the Southern Ocean, I feel this should be more explicitly discussed. In some respects, it’s a bigger change than some of the more localized differences. That “mode” does seem to be captured in EOF3 (Figure 7). One can especially see the change in the system in that mode when GRACE is introduced. I don’t see this is even discussed in that section! I think it is one of the more obvious impacts starting around 2002!
- For the annual analysis, I would be interested in seeing a phase analysis. I know the authors use a climatology, so a phase value is not a direct estimate (unlike with a sinusoid fit). However, they could look at the month of the peak value and see if there is any evidence of a phase shift from the control to the assimilation run. Looking at the EOF analysis, I think there will be and it would be an interesting thing to show.
- For Figure 8. Please add some statistics of the actual values with GRACE obs and without. It will be a small change, maybe 1 cm RMS, but worth noting with a quantified metric. Same for Figure 9 – What’s the percentage of the ocean where changes are > 0.5 cm? Between 0 and 0.5 cm? etc.
- One of the important periods for assessing the impact of GRACE is for the year when GRACE observations ended and before GRACE-FO came on-line. No other change in the observing system occurred then (unlike before 2002 with the introduction of Argo profiles into the assimilation as well). It is clear from Figure 8 that the updates to the control run Pb return to the pre-2002 levels, then move back up in 2018 when GRACE-FO is used. I see no discussion of this at all, but to me, it is the clearest indicator in the analysis that GRACE is responsible and not another data set.
Citation: https://doi.org/10.5194/egusphere-2026-947-RC2
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- 1
The authors aim to examine the effect of assimilating GRACE data, along with other datasets, on state estimates produced by the project for Estimating the Circulation and Climate of the Ocean (ECCO). By way of comparing the results against a reference run that does not include any data constraints the authors claim that the ECCO optimization leads to large adjustments in bottom pressure (pb) fields at monthly and longer timescales largely upon assimilation of GRACE data. Another conclusion drawn is that a mean ocean mass constraint is essential for mitigating large imbalances in freshwater fluxes derived from atmospheric reanalyses (used as prior forcing) and for producing a realistic barystatic sea level curve. Inspecting the residuals, the authors also point to problems with the GRAC data that appear to be inconsistent with other information about the ocean circulation and its variability.
The subject of the paper is important, and ultimately the manuscript should be published. However, some mayor shortcomings must be remedied first. First and foremost, the experimental setup is flawed in that only one assimilation experiment constraint simultaneously by many data sets is being used to pinpoint the influence of a specific data set – the GRACE data - by comparing the results against a reference run in which no data were assimilated at all. Obviously, this cannot work and conclusions drawn are not backed up by the results shown. This holds even more so as the GRACE data kick in at the same time when Argo data become available and so the solution will be impacted in all its aspect by both data sets and all other data as well. Ideally, exactly the same set-up should be run twice with and without GARCE data involved. At a minimum, what the authors need to do here is compare results against a previous optimization run (Release 4 described in detail by Fukumori et al. (2019) which included almost all data as constraints, but not the GRACE data. Moreover, many important details are missing in the paper regarding the approach but also the assimilation experiment itself that need to be added. More detailed comments are provided below. Once all those have been addressed satisfactorily I belief that the paper can become a significant contribution.
Major Comments:
Minor Comments: