the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
| 21 Mar 2023
Evaluation of the CMCC global eddying ocean model for the Ocean Model Intercomparison Project (OMIP2)
Abstract. This paper describes the global eddying ocean-sea ice simulation produced at the Euro-Mediterranean Center on Climate Change (CMCC) obtained following the experimental design of the Ocean Model Intercomparison Project phase 2 (OMIP2). The eddy-rich model is based on the NEMOv3.6 framework, with a global horizontal resolution of 1/16° and 98 vertical levels, and was originally designed for an operational short-term ocean forecasting system. Here, it is driven by one multi-decadal cycle of the prescribed JRA55-do atmospheric reanalysis and runoff dataset in order to perform a long-term benchmarking experiment.
To access the accuracy of simulated 3D ocean fields, and highlight the relative benefits of mesoscale activities, the GLOB16 performances are evaluated via a selection of key climate metrics against observational datasets and two other NEMO configurations at lower resolutions: an eddy-permitting resolution (ORCA025) and a non-eddying resolution (ORCA1) designed to form the ocean-sea ice component of the fully coupled CMCC climate model.
The well-known biases in the low-resolution simulations are significantly improved in the high-resolution model. The evolution and spatial pattern of large-scale features (such as sea surface temperature biases and winter mixed layer structure) in GLOB16 are generally better reproduced, and the large-scale circulation is remarkably improved compared to the low-resolution oceans. We find that eddying resolution is an advantage in resolving the structure of western boundary currents, the overturning cells, and flow through key passages. GLOB16 might be an appropriate tool for ocean climate modeling effort, even though the benefit of eddying resolution does not provide unambiguous advances for all ocean variables in all regions.
-
Notice on discussion status
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
-
Preprint
(7773 KB)
-
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(7773 KB) - Metadata XML
- BibTeX
- EndNote
- Final revised paper
Journal article(s) based on this preprint
Interactive discussion
Status: closed
-
CC1: 'Comment on egusphere-2023-469', Alexander Shchepetkin, 23 Mar 2023
It looks like here is some typo or confusion in Table 1 on pagge 4, line130:
Barotropic sub-steop [sec] 30 64 120
these numbers does not look right.
At first, they are probably in reverse order, as 1 degree model should allow larger (not smaller step).
Secondly, assuming maximum barotropic wave speed of 240 m/sec = sqrt(g*h) = sqrt(9.8 * 6000), it takes approximately 400 seconds to cover 100km, which corresponds to 1 grid box of 1-degree model at Equator. I high latittudes the grid box is smaller (in km), so it will take less than 400 sec, and from this point of view 120sec barotropic ime step looks reasonable, thought a bit conservative, I would try 200 sec or so. But i also depends on numerical time stepping algorithm in barotropic mode.
Refining resolution by a factor of 4 twice, 1degree --> 1/4 --> 1/16, requires reducing barotropic step by he same factor (this does not necessarily works for barolinic step - the model tend to develop larger velocitties as the resolution goes finer, but for he barotropic i is pretty straightforward). So ne figures in this row of the table should be proportional to 1:0.25::0.0625, say 200 50 12.5.
It is highly unlikely that you an run your model at 0.0625 degree resoluion wih barotropic step of not only 120, but also 32 seconds: making the same estimate as above, it takes 25 seconds to cross 1 grid box of 1/16-degree model near Equator, half this time at 60-degrees Norh, or in Acctic (whatever the curvilinear grid is used tthere). Assuming generalized forward-backward shcheme of ROMS (also used in modern versions of NEMO), its maximum allowed Courant number is 0.87. this bring you o he estimate of 10 ... 12 second barotropic time step.
Citation: https://doi.org/10.5194/egusphere-2023-469-CC1 -
CC2: 'Reply on CC1', Doroteaciro Iovino, 05 Apr 2023
Thank you for the comment and for spotting the error in table 1.
Numbers are actually correct, but they do not represent the barotropic sub-step in second (as written in the table), but the number of iterations of barotropic mode during one time step used for the three dimensional prognostic variables. So the barotropic time step correcly decreases with finer resolution.
line130 in Table 1 will be corrected as we revise the manuscript.
Citation: https://doi.org/10.5194/egusphere-2023-469-CC2 -
CC3: 'Reply on CC2', Alexander Shchepetkin, 05 Apr 2023
Still something is wrong here. At the first approximation, the ratio of baroclinic-to-barotropic time step size is determined by the ration of phase speeds of barotropic and first baroclinic mode, and therefore should not depend on resolution.
Looking into more detail, barotropic time step size is striclly restricted by phase speed of external mode, sqrt(g*h), as any other factor (advection velocity, Coriolis term) are much less restrictive. So, given the same depth, barotropic step is strictly proportional to horizontal grid size.
For the baroclinic it is a bit more nonlinear: generally propagation of the first baroclinic mode is the fastest process, however, if horizontal grid is too coarse, the time step should still resolve inertial oscillations, so time step cannot be set too large, even if an estimate based on baroclinic mode speed allows. Thypically this happens when time step is larger than 1 hour. For fine resolution models inertial oscillations are not restrictive (time step is too small any way), but other factors kick in: advection velocity because of more active currents, and eventually vertical advection. So maximum allowed time step needs to be a bit smaller than based solely on first baroclinic mode.
Assuming that numbers 30, 64, 120 in your table are the ratios of baroclinic/barotropic time steps, your barotropic steps are
3600/30=120 sec for 1-degree model, which is reasonable.
1200/64=18.75 sec for 0.25-degree, which is not so reasonable, too small, as it takes approximately 100 seconds for barotropic signal propagating as speed of 250 m/sec [=sqrt(9.81*6000)] to cover distance of one grid box; and
200/120 = 1.666 sec for 0.0625-degre model, which is EXTREMELY WASTEFUL, because now it takes about 25 seconds to cover one grid box, and now your Courant number for barotropic mode is 15 times smaller than it should be.
Citation: https://doi.org/10.5194/egusphere-2023-469-CC3 -
CC4: 'Reply on CC3', Doroteaciro Iovino, 15 May 2023
This is correct. The barotropic time step used in the high-resolution run is small. The ratio baroclinic/barotropic time steps of 120 was chosen for the GLOB16 configuration based on larger time steps that we were unable to achieve at run time for the OMIP2 simulation. Unfortunately we did not modify it. Likely, this choice does affect the computational model performance, not the results.
Citation: https://doi.org/10.5194/egusphere-2023-469-CC4
-
CC4: 'Reply on CC3', Doroteaciro Iovino, 15 May 2023
-
CC3: 'Reply on CC2', Alexander Shchepetkin, 05 Apr 2023
-
CC2: 'Reply on CC1', Doroteaciro Iovino, 05 Apr 2023
-
RC1: 'Comment on egusphere-2023-469', Anonymous Referee #1, 01 May 2023
The present manuscript presents a high level overview of the differences and similarities between three configurations of the CMCC ocean model in forced simulations. The comparisons are limited to the simulated state - no of process level explanations of the differences are provided. Further, while the emphasis is on the impact of horizontal resolution, there are a large number of other differences in the models being compared: vertical resolution, topography, the sea ice component model and the sea ice initialization, the salinity restoring timescale, the way that runoff forcing is applied, along with the more typical adjustments to viscous and diffusive parameterizations. So, while the authors have put in a considerable amount of effort in compiling model metrics, the resulting manuscript is rather unsatisfying. We have little new insight into how and why the explicit representation versus parameterization of the mesoscale impacts the simulated ocean state. As a documentation of what was done the manuscript may be adequate with some additional work to correct imprecise descriptions, but I do not envision the manuscript having much of an impact beyond those who might wish to use the CMCC models and it is unlikely to advance the field. Additionally, the manuscript suffers from being poorly prepared with many missing references and poor language constructions.
Detailed Comments:
Line 26 “enforces our ability in understanding ”: poor wording, perhaps is a prerequisite to develop our understanding
Line 29-30: ensemble size is a mother strong trade-off in both prediction and climate modeling.
Line 31 “start grid spacing”: rather, typical grid spacing. No standard (a specification) exists.
Line 33 “miss key processes”: it is not necessarily the case that key processes are missed. They may be parameterized.
Line 36 “Despite”: While simulations at this resolution …
Line 38: “access to which” : to assess to what extent
Line 60 “resolution dependent”: as discussed at top this is not a convergence study in the sense of numerical analysis. Many other aspects of the simulation besides horizontal resolution are change.
Line 68: Manral et al 2013 ref missing
Line 104: suggest starting new paragraph with sentence beginning “While the best …”
Line 154 “in coupled runs”: all the runs described herein are forced not coupled?
Line 189: do not correspond to what _was_ found in
Line 203-204: I do not understand this distinction. The difference from the initial state taken from observations is the model bias?
Line 210: Lellouche et al 2021 ref missing
Table 2: is the standard deviation stated the inter annual standard deviation of the global mean SST or the mean standard deviation of the global spatial deviation of SST?
Line 254: I don’t understand the difference between “model physics”, which I generally take to be parameterizations and “unresolved processes” which require parameterization?
Line 260: Most of the SST biases are reduced”: This is not visually that obvious. State the rms error of annual mean SST at each resolution.
Section 3.3.2 and Figures 5-6: This discussion would be much improved by showing panels with the summer MLD (JJA for NH and JFM for SH) as a single plot and winter MLD (vice versa) as a single plot with the color scale appropriate to each season. The discussion of similarities in summer or lower latitude features is completely obscured by the full annual range color scale. This is also a very long section with little insight beyond that they are different. To what extent can we attribute differences to changes in preconditioning of water masses due to differences in large scale flow versus changes in the restartification power of mixed layer eddies in each case? Does the ORCA1 model include a parameterization (e.g. Fox-Kemper e al) of submesoscale mixed laser restratification included in its GM parameterization?
Line 338-342 discussion of higher order statistics in Johnson and Lyman 2022: What is the relevance to this study none of these statistics are evaluated in the paper
Line 349: Johnson and Lyman 2022 ref missing
Line 350: again, the use of the full dynamic range in the axis scale makes it difficult to compare the quality of the simulation of shallower mixed layers. The relative error could be just as large as for deeper M.
Line 374 “representations is underrepresented”: nonsensical phrase
Line 377: “unable to represent flow instabilities …”: yes, but the figure is showing mean low speed, not EKE
Line 385: “dependent on model numerics”: how so? Don’t all of the models use the same numerical methods to solve the equations of motion?
Line 386: “impact of mesoscale dynamics”: This has not been shown. It could simply be the impact of viscous boundary layer dynamics or topography which also differ across configurations
Line 404 “passed”: past
Line 421 “Figure 10 shows role of mesoscale eddy field …” : again, the figure shows the mean flow and no analysis of eddy-mean flow interaction is provided.
Section 3.3.2 (sigma overturning): A more precise definition of how the stream function was calculated at each resolution is required. Was it computed from Eulerian mean (monthly, annual, climatological?) velocity and density fields? Was the GM eddy-induced velocity included in the ORCA1 result? The authors should write down the integral with averaging operators in the appropriate places for clarity. This is important in trying to understand whether differences seen are related to “bolus velocity”, diapycnal processes or surface forcing. The reference to Andrews and McIntyre suggest that we should be interpreting something about eddy induced transport, but the discussion is unclear. One of the major differences is the structure of the strong clockwise cell in the ACC region which I presume is related to the degree of compensation of the Deacon cell. No discussion of this feature is provided, nor are we sure how to interpret the result given the uncertainty about exactly what is being shown.
Line 466: “This suggests that longer integrations are required for GLOB16 …”: It was previously stated that the analysis of all cases was for the first cycle (Line 150). Why is that only GLOB16 requires longer integration to be compared?
Figures 13-14 and accompanying discussion: This is a long discussion of the GLOB16 results alone with no explicit comparison across resolutions. It seems unnecessary if the purpose of the paper is investigating resolution dependence rather than an assessment of GLOB16 alone.
Line 560: Treguier 2012 and Robert 2016 refs missing
Citation: https://doi.org/10.5194/egusphere-2023-469-RC1 -
AC1: 'Reply on RC1', Doroteaciro Iovino, 14 Aug 2023
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-469/egusphere-2023-469-AC1-supplement.pdf
-
AC1: 'Reply on RC1', Doroteaciro Iovino, 14 Aug 2023
-
RC2: 'Comment on egusphere-2023-469', Anonymous Referee #2, 19 May 2023
This manuscript provides a high-level assessment of the performance of the CMCC GLOB16 1/16° global ocean and sea ice simulation relative to two related simulations at 1° and 0.25° (ORCA1 and ORCA025) and range of observationally estimated values. The text is clearly written and logically organised, and the figures are appropriate and well-presented. While the manuscript provides few new insights, it gives a good overview of the main strengths and weaknesses of GLOB16 which will be of use to users of that model and as a point of comparison for other modelling efforts internationally. I would like to see it published after major revision to include more details of interest to the ocean modelling community, and I've provided detailed suggestions in the hope that this will help.
While the comparisons to observation are well-chosen and cover many of the most important assessment criteria for models of this sort, there are some significant omissions:
- Several references are made to sea ice processes and differences between the two sea ice models as explanations for differing ocean features, but no sea ice results are presented to back up these speculations. Comparing sea ice results (such as climatological maps of concentration and time series of ice volume, area and extent) with observations and between LIM2 and CICE would be very helpful to aid interpretation of the ocean biases and understand the differences between these models.
- There could also be more comparison of the variability at different resolutions relative to observations, e.g. maps of sea level standard deviation, to highlight the impact of increased resolution.
- No information on model computational performance is provided, e.g. the relative core-hours per simulated year at each resolution. This would be useful for practitioners in deciding whether the improved solution fidelity at high resolution is worth trading off against a shorter simulation duration within finite computational and walltime budgets. Other technical details (e.g. number of computational cores, parallelisation efficiency, etc) would also be helpful.
The depth of analysis could also be improved. Many parts of the text simply give a verbal description of what the plots show. This does not provide much value to the reader, and in some places the descriptions are also incorrect. Additional physical insights and interpretations would be very helpful.
An assessment of the impact of increased resolution in GLOB16 is hampered by many important differences between this model and ORCA1 and ORCA025 (e.g. a different sea ice model, twice as many vertical levels, many different parameterisations). This is unfortunate but perhaps beyond the scope of this paper to rectify.
Re. Code and Data Availability - can the configuration parameter files for GLOB16, ORCA1 and ORCA025 be provided? And links to source code for LIM2 and CICE4?
There are many small typos and errors, which I have listed in the last section below.
Numbers in my detailed comments below are line numbers.
Comments on content:56: Mention that this multi-resolution approach is similar to that taken at other modelling centers, eg Storkey et al 2018 https://doi.org/10.5194/gmd-11-3187-2018, Adcroft et al 2019 http://dx.doi.org/10.1029/2019MS001726, Kiss et al 2020 https://www.geosci-model-dev.net/13/401/2020/
84: if the model has been "extensively upgraded", then Iovino et al. 2016 is not very useful as a reference. Please provide a list of the important changes that have been made since Iovino et al. 2016
93: give the equation of state, and say what the prognostic variables are (e.g. conservative or potential temperature)
105: "While the best approach to identify the impact of grid resolution should be to change only resolution and associated physics in the suit of models, this was not the case in similar previous studies (Chassignet et al., 2020, Kiss et al., 2020, Li et al., 2020)." - while there were unavoidable differences in parameterisation due to the differing ability to resolve processes at different resolutions, Kiss et al. 2020 made significant efforts to harmonise the configurations across resolution. It sounds like an effort in that direction would be possible here and would more cleanly highlight the effects of improving resolution. Is that beyond the scope of this project?
Table 1: as also pointed out by Alexander Shchepetkin, "barotropic sub-step [sec]" should be "barotropic sub-steps". It would also be worth noting that this was a configuration error (the barotropic timestep is an order of magnitude smaller than needed for CFL stability) which would adversely affect the computational cost, but not the numerical solutions.
186: does the differing surface vertical resolution play a role in this SST difference?
190: "Kiss et al. (2020) where the 1/10° ocean surface ... with the largest bias from observations" no, obs in Kiss et al 2020 fig 3b is an anomaly offset by 18°, so this plot only compares trend, not bias
157: specify whether the salt restoring is constrained to have zero total flux. If not, how significant is the salt flux for the drift in total ocean salt mass?
228: "The SSS drift is offset by the surface salinity restoring that is incorporated into the codes to enforce salt conservation in the model ocean (in Sect. 2)." - do you mean "constrain SSS drift" rather than "enforce salt conservation"? Conserving total ocean salt mass would require balancing any net flux into sea ice and nonzero net restoring salt flux.
229: "The restoring of SSS drives its quasi-stationary evolution, the salt exchange between ocean and sea-ice due to ice formation and melting, is the only source of salt for the ocean." - so is there zero net salt restoring flux?254: drift may also be due to biased forcing (as mentioned later in this paragraph), or adjustment from an unbalanced initial condition
257: or initial condition... though less likely for surface bias
Fig 4: if this bias was plotted relative to the WOA initial condition it would remove any effect from initial condition bias relative to ERSSTv5
Figs 5,6: Summer differences are very hard to discern. It would be better to plot winter in both hemispheres in fig 5 and summer in both hemispheres in fig 6, with different color scale.
Figs 5,6: extend latitude range further south to show Ross and Weddell convection
Fig 5,6: add citation for (a) to captionFig 7 adds little beyond what is in 5&6, other than an additional obs dataset - could be supplementary material.
Fig 7: cite obs datasets in caption279: "The observed MLD is diagnosed through a density threshold criterion as the depth over which the potential density increases by 0.03 kg m-3 from the reference value of surface potential density taken at 10m depth; resulting values are mapped on a monthly basis at 1°x1° spatial resolution (de Boyer Montégut et al., 2004). The same density threshold method is applied to model output as recommended by Griffies et al. (2016) to compute the MLD in OMIP models." - This is not the same method because Griffies et al 2016 specify using the top model level as a reference, not 10m. Treguier et al 2023 state CMCC use the top model level, not 10m. Or was MLD recalculated to use 10m (ie different from the Griffies et al method)? If not, this difference may contribute to the bias, as Treguier et al discuss. Please clarify what was done and its bearing on comparison with obs.
297: also mention MLD bias at 0°E in mid-north Greenland Sea: several hundred metres too shallow
367: could also comment on the differences in the Zapiola anticyclone at different resolution - seem similar to what was seen by Kiss et al 2020.
384: "In an eddy-rich regime, the ocean model is less diffusive/viscous" is back to front: At high res, diffusivity/viscosity can be reduced while maintaining numerical stability; this allows WBCs to be realistically narrow and inertial, and the resolution of the internal Rossby radius allows baroclinic instability and an eddying flow
384: "less diffusive/viscous leading to an improvement in the strength and position of WBCs" - could relate this to narrowing the Munk (Laplacian) or Haidvogel et al 1992 (biharmonic) viscous WBC scales (A_lap/beta)^(1/3) and (A_bih/beta)^(1/5). Perhaps these scale values could also be useful in table 1:
ORCA1: Munk: (1e4/2e-11)^1/3~80km
ORCA025: Haidvogel: (1.8e11/2e-11)^1/5~25km
GLOB16: Haidvogel: (0.5e10/2e-11)^1/5~12km
Haidvogel et al 1992 ref: http://dx.doi.org/10.1175/1520-0485(1992)022%3C0882:BCSIAQ%3E2.0.CO;2434: "The Antarctic coastal current is also clearly represented, it flows westward along the Antarctic coast and meets the eastward-flowing ACC at the Drake Passage, emerging as the Malvinas current." - isn't the Malvinas fed by the Antarctic circumpolar current, not the Antarctic coastal current?
465: More discussion of the overturning south of 30°S would be good, e.g. in comparison with Farneti et al 2015. What depth does 1036.8kg/m^3 correspond to in GLOB16 in this region? Why is this subpolar cell mostly disconnected from the abyssal export cell in GLOB16 and ORCA1? It seems more connected to the surface cell at ~50S, 1036kg/m^3 than the abyss. The circulation below 1037kg/m^3 looks quite different from Kiss et al 2020 fig 7 and many of the models in Farneti et al 2015 fig 17 (and ORCA1 looks very different from the 1° CMCC model Farneti et al show) - can you point this out and speculate as to why? Also in ORCA1 a much larger fraction of the southern ocean upwelling is recirculated south of 35S in an intense clockwise cell rather than joining the NADW cell, and this overturning cell is stronger than at higher resolution - why?
589: is it feasible to do a RAPID-like calculation with your model data to verify this?
Further details needed:86: specify the latitude at which the tripolar cap starts
87: is this a Mercator grid? If so, say so. e.g. replace "increases poleward as cosine" -> "meridional spacing decreases poleward as the cosine"
105, 121: state the ice grid used - is it the same as the ocean model? If not, what interpolation methods are used?
105, 121: state what fields are coupled between the ocean and sea ice in each direction
111: specify what is meant by the "in-house sea ice module"? is it CICEv4.1 (line 116)? But that's not in-house.
118: specify maximum ocean depth in the 3 models
120: "such as" - be specific. What else was used? e.g. Redi?
121: give GM parameter values
122: "multi-category" - specify how many
Table 1: suggest to also specify
- ice model dynamic and thermodynamic timesteps
- ocean-ice coupling timestep
- whether downslope transport or mixing schemes were used at low res
- whether Rayleigh was drag used in any straits at low resolution133: specify JRA55-do version (1.4?)
136: specify the interpolation methods that were used from JRA55-do to the model grid in each model
141: is relative wind also used for stress calculation on ice?
145: "at the ocean surface in GLOB16" - is this literally in the top 0.8m, with no distribution to depth at all?
160: "the sea ice models used in our two systems employ different bulk salinity affecting the salt release from the sea ice to the ocean" - specify these values - how different are they? can the effect on stratification and circulation be quantified or at least estimated?
Fig 1,2 captions: specify averaging period (are annual means plotted?)
Small errors, typos, suggestions for clearer phrasing, etc:7: "This paper describes the GLOB16 global ..." so GLOB16 is defined prior to first use on line 13
13: access -> assess
13: mesoscale activities -> resolving mesoscale processes
21: effort -> efforts
29: trade-off among -> trade-offs between
33: Both model configurations do not resolve -> Neither resolution resolves
L6: require -> requiring
38: access to which -> assess to what
51: is -> are
58: (low-, nominally 1° horizontal grid spacing), eddy-permitting (medium-, nominally 0.25°) to eddy-rich (high-, 0.0625°) resolutions -> (low-resolution, nominally 1° horizontal grid spacing), eddy-permitting (medium-resolution, nominally 0.25°) to eddy-rich (high-resolution, 0.0625°)
73: activities -> processes
84: , -> , and
88: - the -> . The
90: Outline -> An outline
93: momentums -> momentum
103: C grid -> a C grid
105: suit -> suite
107: computation cost of GLOB16 -> computational cost of the GLOB16
117: refinement of meridional grid to 1/3° -> meridional refinement to 1/3°
123: delete "Note that the two sea ice models LIM and CICE employ different bulk salinity, affecting the salt release from the sea ice into the ocean." - repeated in line 160
141: JRA55 -> JRA55-do
148: GLOB16 grid -> The GLOB16 grid
154: "in coupled runs" is unclear. I suggest "in ORCA1 and ORCA025" (assuming this is what was meant)
167: that warms -> warming
169: staying anyway -> but staying
170: specify whether the 0.1°C cooling is over 1 cycle or 6
175: over -> out of
187: 2c -> 1b
189: what found -> what was found
fig 1: swap b & c in caption
205: largely -> greatly
212: resolutions -> resolution
229: evolution, the -> evolution, and the
244: in 2018 -> by 2018 ?
258: activities -> activity
259: GLOB16 bias -> GLOB16
261: define "WBC" acronym on first use
262: differences are also in -> improvements are also seen in
265: regions -> regions than ORCA1 and ORCA025
268: experiments with a -> experiments due to a
275: insert last sentence of this paragraph here as the 2nd sentence
288: The mixed -> The winter mixed
290: Ross and Weddell convection is cut off in figs 5,6
298: remove "slightly" - this is quite a big difference
301 high-latitude -> northern high-latitude
305: horizontal -> zonal?
306: remove "caveats"
314: NH Sept MLD not interpretable with this colormap
329, table 1: were downslope transport or mixing schemes used at low res?
350: the observation one -> the spread of observations
360: (Fig. 8), zoomed in the key dynamical regions (Fig. 9 and 10), -> (Fig. 8), and zoomed in to the key dynamical regions (Fig. 9 and 10). The
404: passed -> past
404: follows closely -> closely follows
407: to OSCAR -> to the OSCAR
408: remove "in amplitude"
408: The decaying eastward along the Kuroshio extension and magnitude match the observed one -> The GLOB16 Kuroshio extension magnitude and its eastward decay match observations
409: the 170°E longitude -> 170°E
410: toward 145°E, to rapidly decay westwards. -> until 145°E, but decays too rapidly further east.
Fig 9: fix panel numbering (a-d happens twice)
464, 474, 475, fig 11: stated transports are double what is shown in fig 11 - is the text incorrect or is the contour interval 2 Sv, not 1 Sv as stated in the caption for fig 11?
480: "~2 Sv in density space (~ 6 Sv below 3000 m in depth space)." Are these back to front? Looks like about 6 Sv in fig 11 (or 12 Sv if the contour interval is 2 Sv)
467: "A portion" - quantify this
468: we do present -> we present
473: 55°N -> 65°N?
Fig 11: plot contours beyond current range (both positive and negative) - seem to be missing some in the far south, unless the extrema are very flat. Also state in caption how colour is related to overturning direction
497: till -> until
Fig 12 caption: Swap "dashed" and "solid" and state that ORCA1 is also plotted.
512: two decades -> decade ?
513: can't see low in 2009 in either obs record in Fig 13. "observed in 2009 and 2010" -> "observed at 26.5°N in 2005, 2010, 2011 and 2013"?
518, 528, fig 13: why not plot the other 2 models as well?
Fig 13 caption: state that the time scale is compressed prior to 2000.
539: 15°N -> 18°N?
540, 541: swap 10 - 20°N and 20-30°N (or is fig14a key wrong?)
542: MHT peaks around 24°N -> MHT peaks around 24°N but is not well constrained given the error bars
542-589: MHT -> AMHT
548: remove "The strongest heat transport is found in the eddy-rich ocean." - repeated below
550: GLOB16 tracks the ECMWF estimates and compares well with TF08 -> GLOB16 tracks the ECMWF estimates and compares well with TF08 except north of 40°N
552: Hirschi et al. 2019 -> Hirschi et al. 2020 ?
556: 18°N -> 15°N ?
565: slightly exceeds the total MHT between the equator and 15°N -> slightly exceeds the total MHT between the equator and 15°N and south of 20°S
568: gyre one increases to level off -> gyre component increases to level off at total AMHT
574: remove "not shown for ORCA025 575 and ORCA1" - this difference is visible in fig 14a.
578: misrepresent -> misrepresents
579: 2010, 2011, 2013 and 2017 minima -> 2010, 2011, 2013, 2017 and 2019 minima ?
Fig 14b: why not include the other 2 models?
608: negative -> positive
617, table 1: was Rayleigh drag used in the straits at low resolution?
629: plot Donohue et al value in fig 15c
631: below the most recent estimates (Xu et al., 2020) -> below the most recent estimates (Xu et al., 2020) and some eddy-rich models (Kiss et al., 2020)
Fig 15 caption: (b) the Indonesian Throughflow -> (b) the southward Indonesian Throughflow
Fig 15 caption: Cite sources for obs in a & b671: provide -> provides
679: Indian to the Pacific -> Pacific to Indian
683: (weaker than observed values) -> (weaker than observed values and some other eddy-rich models)
Citation: https://doi.org/10.5194/egusphere-2023-469-RC2 -
AC2: 'Reply on RC2', Doroteaciro Iovino, 14 Aug 2023
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-469/egusphere-2023-469-AC2-supplement.pdf
-
AC2: 'Reply on RC2', Doroteaciro Iovino, 14 Aug 2023
Interactive discussion
Status: closed
-
CC1: 'Comment on egusphere-2023-469', Alexander Shchepetkin, 23 Mar 2023
It looks like here is some typo or confusion in Table 1 on pagge 4, line130:
Barotropic sub-steop [sec] 30 64 120
these numbers does not look right.
At first, they are probably in reverse order, as 1 degree model should allow larger (not smaller step).
Secondly, assuming maximum barotropic wave speed of 240 m/sec = sqrt(g*h) = sqrt(9.8 * 6000), it takes approximately 400 seconds to cover 100km, which corresponds to 1 grid box of 1-degree model at Equator. I high latittudes the grid box is smaller (in km), so it will take less than 400 sec, and from this point of view 120sec barotropic ime step looks reasonable, thought a bit conservative, I would try 200 sec or so. But i also depends on numerical time stepping algorithm in barotropic mode.
Refining resolution by a factor of 4 twice, 1degree --> 1/4 --> 1/16, requires reducing barotropic step by he same factor (this does not necessarily works for barolinic step - the model tend to develop larger velocitties as the resolution goes finer, but for he barotropic i is pretty straightforward). So ne figures in this row of the table should be proportional to 1:0.25::0.0625, say 200 50 12.5.
It is highly unlikely that you an run your model at 0.0625 degree resoluion wih barotropic step of not only 120, but also 32 seconds: making the same estimate as above, it takes 25 seconds to cross 1 grid box of 1/16-degree model near Equator, half this time at 60-degrees Norh, or in Acctic (whatever the curvilinear grid is used tthere). Assuming generalized forward-backward shcheme of ROMS (also used in modern versions of NEMO), its maximum allowed Courant number is 0.87. this bring you o he estimate of 10 ... 12 second barotropic time step.
Citation: https://doi.org/10.5194/egusphere-2023-469-CC1 -
CC2: 'Reply on CC1', Doroteaciro Iovino, 05 Apr 2023
Thank you for the comment and for spotting the error in table 1.
Numbers are actually correct, but they do not represent the barotropic sub-step in second (as written in the table), but the number of iterations of barotropic mode during one time step used for the three dimensional prognostic variables. So the barotropic time step correcly decreases with finer resolution.
line130 in Table 1 will be corrected as we revise the manuscript.
Citation: https://doi.org/10.5194/egusphere-2023-469-CC2 -
CC3: 'Reply on CC2', Alexander Shchepetkin, 05 Apr 2023
Still something is wrong here. At the first approximation, the ratio of baroclinic-to-barotropic time step size is determined by the ration of phase speeds of barotropic and first baroclinic mode, and therefore should not depend on resolution.
Looking into more detail, barotropic time step size is striclly restricted by phase speed of external mode, sqrt(g*h), as any other factor (advection velocity, Coriolis term) are much less restrictive. So, given the same depth, barotropic step is strictly proportional to horizontal grid size.
For the baroclinic it is a bit more nonlinear: generally propagation of the first baroclinic mode is the fastest process, however, if horizontal grid is too coarse, the time step should still resolve inertial oscillations, so time step cannot be set too large, even if an estimate based on baroclinic mode speed allows. Thypically this happens when time step is larger than 1 hour. For fine resolution models inertial oscillations are not restrictive (time step is too small any way), but other factors kick in: advection velocity because of more active currents, and eventually vertical advection. So maximum allowed time step needs to be a bit smaller than based solely on first baroclinic mode.
Assuming that numbers 30, 64, 120 in your table are the ratios of baroclinic/barotropic time steps, your barotropic steps are
3600/30=120 sec for 1-degree model, which is reasonable.
1200/64=18.75 sec for 0.25-degree, which is not so reasonable, too small, as it takes approximately 100 seconds for barotropic signal propagating as speed of 250 m/sec [=sqrt(9.81*6000)] to cover distance of one grid box; and
200/120 = 1.666 sec for 0.0625-degre model, which is EXTREMELY WASTEFUL, because now it takes about 25 seconds to cover one grid box, and now your Courant number for barotropic mode is 15 times smaller than it should be.
Citation: https://doi.org/10.5194/egusphere-2023-469-CC3 -
CC4: 'Reply on CC3', Doroteaciro Iovino, 15 May 2023
This is correct. The barotropic time step used in the high-resolution run is small. The ratio baroclinic/barotropic time steps of 120 was chosen for the GLOB16 configuration based on larger time steps that we were unable to achieve at run time for the OMIP2 simulation. Unfortunately we did not modify it. Likely, this choice does affect the computational model performance, not the results.
Citation: https://doi.org/10.5194/egusphere-2023-469-CC4
-
CC4: 'Reply on CC3', Doroteaciro Iovino, 15 May 2023
-
CC3: 'Reply on CC2', Alexander Shchepetkin, 05 Apr 2023
-
CC2: 'Reply on CC1', Doroteaciro Iovino, 05 Apr 2023
-
RC1: 'Comment on egusphere-2023-469', Anonymous Referee #1, 01 May 2023
The present manuscript presents a high level overview of the differences and similarities between three configurations of the CMCC ocean model in forced simulations. The comparisons are limited to the simulated state - no of process level explanations of the differences are provided. Further, while the emphasis is on the impact of horizontal resolution, there are a large number of other differences in the models being compared: vertical resolution, topography, the sea ice component model and the sea ice initialization, the salinity restoring timescale, the way that runoff forcing is applied, along with the more typical adjustments to viscous and diffusive parameterizations. So, while the authors have put in a considerable amount of effort in compiling model metrics, the resulting manuscript is rather unsatisfying. We have little new insight into how and why the explicit representation versus parameterization of the mesoscale impacts the simulated ocean state. As a documentation of what was done the manuscript may be adequate with some additional work to correct imprecise descriptions, but I do not envision the manuscript having much of an impact beyond those who might wish to use the CMCC models and it is unlikely to advance the field. Additionally, the manuscript suffers from being poorly prepared with many missing references and poor language constructions.
Detailed Comments:
Line 26 “enforces our ability in understanding ”: poor wording, perhaps is a prerequisite to develop our understanding
Line 29-30: ensemble size is a mother strong trade-off in both prediction and climate modeling.
Line 31 “start grid spacing”: rather, typical grid spacing. No standard (a specification) exists.
Line 33 “miss key processes”: it is not necessarily the case that key processes are missed. They may be parameterized.
Line 36 “Despite”: While simulations at this resolution …
Line 38: “access to which” : to assess to what extent
Line 60 “resolution dependent”: as discussed at top this is not a convergence study in the sense of numerical analysis. Many other aspects of the simulation besides horizontal resolution are change.
Line 68: Manral et al 2013 ref missing
Line 104: suggest starting new paragraph with sentence beginning “While the best …”
Line 154 “in coupled runs”: all the runs described herein are forced not coupled?
Line 189: do not correspond to what _was_ found in
Line 203-204: I do not understand this distinction. The difference from the initial state taken from observations is the model bias?
Line 210: Lellouche et al 2021 ref missing
Table 2: is the standard deviation stated the inter annual standard deviation of the global mean SST or the mean standard deviation of the global spatial deviation of SST?
Line 254: I don’t understand the difference between “model physics”, which I generally take to be parameterizations and “unresolved processes” which require parameterization?
Line 260: Most of the SST biases are reduced”: This is not visually that obvious. State the rms error of annual mean SST at each resolution.
Section 3.3.2 and Figures 5-6: This discussion would be much improved by showing panels with the summer MLD (JJA for NH and JFM for SH) as a single plot and winter MLD (vice versa) as a single plot with the color scale appropriate to each season. The discussion of similarities in summer or lower latitude features is completely obscured by the full annual range color scale. This is also a very long section with little insight beyond that they are different. To what extent can we attribute differences to changes in preconditioning of water masses due to differences in large scale flow versus changes in the restartification power of mixed layer eddies in each case? Does the ORCA1 model include a parameterization (e.g. Fox-Kemper e al) of submesoscale mixed laser restratification included in its GM parameterization?
Line 338-342 discussion of higher order statistics in Johnson and Lyman 2022: What is the relevance to this study none of these statistics are evaluated in the paper
Line 349: Johnson and Lyman 2022 ref missing
Line 350: again, the use of the full dynamic range in the axis scale makes it difficult to compare the quality of the simulation of shallower mixed layers. The relative error could be just as large as for deeper M.
Line 374 “representations is underrepresented”: nonsensical phrase
Line 377: “unable to represent flow instabilities …”: yes, but the figure is showing mean low speed, not EKE
Line 385: “dependent on model numerics”: how so? Don’t all of the models use the same numerical methods to solve the equations of motion?
Line 386: “impact of mesoscale dynamics”: This has not been shown. It could simply be the impact of viscous boundary layer dynamics or topography which also differ across configurations
Line 404 “passed”: past
Line 421 “Figure 10 shows role of mesoscale eddy field …” : again, the figure shows the mean flow and no analysis of eddy-mean flow interaction is provided.
Section 3.3.2 (sigma overturning): A more precise definition of how the stream function was calculated at each resolution is required. Was it computed from Eulerian mean (monthly, annual, climatological?) velocity and density fields? Was the GM eddy-induced velocity included in the ORCA1 result? The authors should write down the integral with averaging operators in the appropriate places for clarity. This is important in trying to understand whether differences seen are related to “bolus velocity”, diapycnal processes or surface forcing. The reference to Andrews and McIntyre suggest that we should be interpreting something about eddy induced transport, but the discussion is unclear. One of the major differences is the structure of the strong clockwise cell in the ACC region which I presume is related to the degree of compensation of the Deacon cell. No discussion of this feature is provided, nor are we sure how to interpret the result given the uncertainty about exactly what is being shown.
Line 466: “This suggests that longer integrations are required for GLOB16 …”: It was previously stated that the analysis of all cases was for the first cycle (Line 150). Why is that only GLOB16 requires longer integration to be compared?
Figures 13-14 and accompanying discussion: This is a long discussion of the GLOB16 results alone with no explicit comparison across resolutions. It seems unnecessary if the purpose of the paper is investigating resolution dependence rather than an assessment of GLOB16 alone.
Line 560: Treguier 2012 and Robert 2016 refs missing
Citation: https://doi.org/10.5194/egusphere-2023-469-RC1 -
AC1: 'Reply on RC1', Doroteaciro Iovino, 14 Aug 2023
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-469/egusphere-2023-469-AC1-supplement.pdf
-
AC1: 'Reply on RC1', Doroteaciro Iovino, 14 Aug 2023
-
RC2: 'Comment on egusphere-2023-469', Anonymous Referee #2, 19 May 2023
This manuscript provides a high-level assessment of the performance of the CMCC GLOB16 1/16° global ocean and sea ice simulation relative to two related simulations at 1° and 0.25° (ORCA1 and ORCA025) and range of observationally estimated values. The text is clearly written and logically organised, and the figures are appropriate and well-presented. While the manuscript provides few new insights, it gives a good overview of the main strengths and weaknesses of GLOB16 which will be of use to users of that model and as a point of comparison for other modelling efforts internationally. I would like to see it published after major revision to include more details of interest to the ocean modelling community, and I've provided detailed suggestions in the hope that this will help.
While the comparisons to observation are well-chosen and cover many of the most important assessment criteria for models of this sort, there are some significant omissions:
- Several references are made to sea ice processes and differences between the two sea ice models as explanations for differing ocean features, but no sea ice results are presented to back up these speculations. Comparing sea ice results (such as climatological maps of concentration and time series of ice volume, area and extent) with observations and between LIM2 and CICE would be very helpful to aid interpretation of the ocean biases and understand the differences between these models.
- There could also be more comparison of the variability at different resolutions relative to observations, e.g. maps of sea level standard deviation, to highlight the impact of increased resolution.
- No information on model computational performance is provided, e.g. the relative core-hours per simulated year at each resolution. This would be useful for practitioners in deciding whether the improved solution fidelity at high resolution is worth trading off against a shorter simulation duration within finite computational and walltime budgets. Other technical details (e.g. number of computational cores, parallelisation efficiency, etc) would also be helpful.
The depth of analysis could also be improved. Many parts of the text simply give a verbal description of what the plots show. This does not provide much value to the reader, and in some places the descriptions are also incorrect. Additional physical insights and interpretations would be very helpful.
An assessment of the impact of increased resolution in GLOB16 is hampered by many important differences between this model and ORCA1 and ORCA025 (e.g. a different sea ice model, twice as many vertical levels, many different parameterisations). This is unfortunate but perhaps beyond the scope of this paper to rectify.
Re. Code and Data Availability - can the configuration parameter files for GLOB16, ORCA1 and ORCA025 be provided? And links to source code for LIM2 and CICE4?
There are many small typos and errors, which I have listed in the last section below.
Numbers in my detailed comments below are line numbers.
Comments on content:56: Mention that this multi-resolution approach is similar to that taken at other modelling centers, eg Storkey et al 2018 https://doi.org/10.5194/gmd-11-3187-2018, Adcroft et al 2019 http://dx.doi.org/10.1029/2019MS001726, Kiss et al 2020 https://www.geosci-model-dev.net/13/401/2020/
84: if the model has been "extensively upgraded", then Iovino et al. 2016 is not very useful as a reference. Please provide a list of the important changes that have been made since Iovino et al. 2016
93: give the equation of state, and say what the prognostic variables are (e.g. conservative or potential temperature)
105: "While the best approach to identify the impact of grid resolution should be to change only resolution and associated physics in the suit of models, this was not the case in similar previous studies (Chassignet et al., 2020, Kiss et al., 2020, Li et al., 2020)." - while there were unavoidable differences in parameterisation due to the differing ability to resolve processes at different resolutions, Kiss et al. 2020 made significant efforts to harmonise the configurations across resolution. It sounds like an effort in that direction would be possible here and would more cleanly highlight the effects of improving resolution. Is that beyond the scope of this project?
Table 1: as also pointed out by Alexander Shchepetkin, "barotropic sub-step [sec]" should be "barotropic sub-steps". It would also be worth noting that this was a configuration error (the barotropic timestep is an order of magnitude smaller than needed for CFL stability) which would adversely affect the computational cost, but not the numerical solutions.
186: does the differing surface vertical resolution play a role in this SST difference?
190: "Kiss et al. (2020) where the 1/10° ocean surface ... with the largest bias from observations" no, obs in Kiss et al 2020 fig 3b is an anomaly offset by 18°, so this plot only compares trend, not bias
157: specify whether the salt restoring is constrained to have zero total flux. If not, how significant is the salt flux for the drift in total ocean salt mass?
228: "The SSS drift is offset by the surface salinity restoring that is incorporated into the codes to enforce salt conservation in the model ocean (in Sect. 2)." - do you mean "constrain SSS drift" rather than "enforce salt conservation"? Conserving total ocean salt mass would require balancing any net flux into sea ice and nonzero net restoring salt flux.
229: "The restoring of SSS drives its quasi-stationary evolution, the salt exchange between ocean and sea-ice due to ice formation and melting, is the only source of salt for the ocean." - so is there zero net salt restoring flux?254: drift may also be due to biased forcing (as mentioned later in this paragraph), or adjustment from an unbalanced initial condition
257: or initial condition... though less likely for surface bias
Fig 4: if this bias was plotted relative to the WOA initial condition it would remove any effect from initial condition bias relative to ERSSTv5
Figs 5,6: Summer differences are very hard to discern. It would be better to plot winter in both hemispheres in fig 5 and summer in both hemispheres in fig 6, with different color scale.
Figs 5,6: extend latitude range further south to show Ross and Weddell convection
Fig 5,6: add citation for (a) to captionFig 7 adds little beyond what is in 5&6, other than an additional obs dataset - could be supplementary material.
Fig 7: cite obs datasets in caption279: "The observed MLD is diagnosed through a density threshold criterion as the depth over which the potential density increases by 0.03 kg m-3 from the reference value of surface potential density taken at 10m depth; resulting values are mapped on a monthly basis at 1°x1° spatial resolution (de Boyer Montégut et al., 2004). The same density threshold method is applied to model output as recommended by Griffies et al. (2016) to compute the MLD in OMIP models." - This is not the same method because Griffies et al 2016 specify using the top model level as a reference, not 10m. Treguier et al 2023 state CMCC use the top model level, not 10m. Or was MLD recalculated to use 10m (ie different from the Griffies et al method)? If not, this difference may contribute to the bias, as Treguier et al discuss. Please clarify what was done and its bearing on comparison with obs.
297: also mention MLD bias at 0°E in mid-north Greenland Sea: several hundred metres too shallow
367: could also comment on the differences in the Zapiola anticyclone at different resolution - seem similar to what was seen by Kiss et al 2020.
384: "In an eddy-rich regime, the ocean model is less diffusive/viscous" is back to front: At high res, diffusivity/viscosity can be reduced while maintaining numerical stability; this allows WBCs to be realistically narrow and inertial, and the resolution of the internal Rossby radius allows baroclinic instability and an eddying flow
384: "less diffusive/viscous leading to an improvement in the strength and position of WBCs" - could relate this to narrowing the Munk (Laplacian) or Haidvogel et al 1992 (biharmonic) viscous WBC scales (A_lap/beta)^(1/3) and (A_bih/beta)^(1/5). Perhaps these scale values could also be useful in table 1:
ORCA1: Munk: (1e4/2e-11)^1/3~80km
ORCA025: Haidvogel: (1.8e11/2e-11)^1/5~25km
GLOB16: Haidvogel: (0.5e10/2e-11)^1/5~12km
Haidvogel et al 1992 ref: http://dx.doi.org/10.1175/1520-0485(1992)022%3C0882:BCSIAQ%3E2.0.CO;2434: "The Antarctic coastal current is also clearly represented, it flows westward along the Antarctic coast and meets the eastward-flowing ACC at the Drake Passage, emerging as the Malvinas current." - isn't the Malvinas fed by the Antarctic circumpolar current, not the Antarctic coastal current?
465: More discussion of the overturning south of 30°S would be good, e.g. in comparison with Farneti et al 2015. What depth does 1036.8kg/m^3 correspond to in GLOB16 in this region? Why is this subpolar cell mostly disconnected from the abyssal export cell in GLOB16 and ORCA1? It seems more connected to the surface cell at ~50S, 1036kg/m^3 than the abyss. The circulation below 1037kg/m^3 looks quite different from Kiss et al 2020 fig 7 and many of the models in Farneti et al 2015 fig 17 (and ORCA1 looks very different from the 1° CMCC model Farneti et al show) - can you point this out and speculate as to why? Also in ORCA1 a much larger fraction of the southern ocean upwelling is recirculated south of 35S in an intense clockwise cell rather than joining the NADW cell, and this overturning cell is stronger than at higher resolution - why?
589: is it feasible to do a RAPID-like calculation with your model data to verify this?
Further details needed:86: specify the latitude at which the tripolar cap starts
87: is this a Mercator grid? If so, say so. e.g. replace "increases poleward as cosine" -> "meridional spacing decreases poleward as the cosine"
105, 121: state the ice grid used - is it the same as the ocean model? If not, what interpolation methods are used?
105, 121: state what fields are coupled between the ocean and sea ice in each direction
111: specify what is meant by the "in-house sea ice module"? is it CICEv4.1 (line 116)? But that's not in-house.
118: specify maximum ocean depth in the 3 models
120: "such as" - be specific. What else was used? e.g. Redi?
121: give GM parameter values
122: "multi-category" - specify how many
Table 1: suggest to also specify
- ice model dynamic and thermodynamic timesteps
- ocean-ice coupling timestep
- whether downslope transport or mixing schemes were used at low res
- whether Rayleigh was drag used in any straits at low resolution133: specify JRA55-do version (1.4?)
136: specify the interpolation methods that were used from JRA55-do to the model grid in each model
141: is relative wind also used for stress calculation on ice?
145: "at the ocean surface in GLOB16" - is this literally in the top 0.8m, with no distribution to depth at all?
160: "the sea ice models used in our two systems employ different bulk salinity affecting the salt release from the sea ice to the ocean" - specify these values - how different are they? can the effect on stratification and circulation be quantified or at least estimated?
Fig 1,2 captions: specify averaging period (are annual means plotted?)
Small errors, typos, suggestions for clearer phrasing, etc:7: "This paper describes the GLOB16 global ..." so GLOB16 is defined prior to first use on line 13
13: access -> assess
13: mesoscale activities -> resolving mesoscale processes
21: effort -> efforts
29: trade-off among -> trade-offs between
33: Both model configurations do not resolve -> Neither resolution resolves
L6: require -> requiring
38: access to which -> assess to what
51: is -> are
58: (low-, nominally 1° horizontal grid spacing), eddy-permitting (medium-, nominally 0.25°) to eddy-rich (high-, 0.0625°) resolutions -> (low-resolution, nominally 1° horizontal grid spacing), eddy-permitting (medium-resolution, nominally 0.25°) to eddy-rich (high-resolution, 0.0625°)
73: activities -> processes
84: , -> , and
88: - the -> . The
90: Outline -> An outline
93: momentums -> momentum
103: C grid -> a C grid
105: suit -> suite
107: computation cost of GLOB16 -> computational cost of the GLOB16
117: refinement of meridional grid to 1/3° -> meridional refinement to 1/3°
123: delete "Note that the two sea ice models LIM and CICE employ different bulk salinity, affecting the salt release from the sea ice into the ocean." - repeated in line 160
141: JRA55 -> JRA55-do
148: GLOB16 grid -> The GLOB16 grid
154: "in coupled runs" is unclear. I suggest "in ORCA1 and ORCA025" (assuming this is what was meant)
167: that warms -> warming
169: staying anyway -> but staying
170: specify whether the 0.1°C cooling is over 1 cycle or 6
175: over -> out of
187: 2c -> 1b
189: what found -> what was found
fig 1: swap b & c in caption
205: largely -> greatly
212: resolutions -> resolution
229: evolution, the -> evolution, and the
244: in 2018 -> by 2018 ?
258: activities -> activity
259: GLOB16 bias -> GLOB16
261: define "WBC" acronym on first use
262: differences are also in -> improvements are also seen in
265: regions -> regions than ORCA1 and ORCA025
268: experiments with a -> experiments due to a
275: insert last sentence of this paragraph here as the 2nd sentence
288: The mixed -> The winter mixed
290: Ross and Weddell convection is cut off in figs 5,6
298: remove "slightly" - this is quite a big difference
301 high-latitude -> northern high-latitude
305: horizontal -> zonal?
306: remove "caveats"
314: NH Sept MLD not interpretable with this colormap
329, table 1: were downslope transport or mixing schemes used at low res?
350: the observation one -> the spread of observations
360: (Fig. 8), zoomed in the key dynamical regions (Fig. 9 and 10), -> (Fig. 8), and zoomed in to the key dynamical regions (Fig. 9 and 10). The
404: passed -> past
404: follows closely -> closely follows
407: to OSCAR -> to the OSCAR
408: remove "in amplitude"
408: The decaying eastward along the Kuroshio extension and magnitude match the observed one -> The GLOB16 Kuroshio extension magnitude and its eastward decay match observations
409: the 170°E longitude -> 170°E
410: toward 145°E, to rapidly decay westwards. -> until 145°E, but decays too rapidly further east.
Fig 9: fix panel numbering (a-d happens twice)
464, 474, 475, fig 11: stated transports are double what is shown in fig 11 - is the text incorrect or is the contour interval 2 Sv, not 1 Sv as stated in the caption for fig 11?
480: "~2 Sv in density space (~ 6 Sv below 3000 m in depth space)." Are these back to front? Looks like about 6 Sv in fig 11 (or 12 Sv if the contour interval is 2 Sv)
467: "A portion" - quantify this
468: we do present -> we present
473: 55°N -> 65°N?
Fig 11: plot contours beyond current range (both positive and negative) - seem to be missing some in the far south, unless the extrema are very flat. Also state in caption how colour is related to overturning direction
497: till -> until
Fig 12 caption: Swap "dashed" and "solid" and state that ORCA1 is also plotted.
512: two decades -> decade ?
513: can't see low in 2009 in either obs record in Fig 13. "observed in 2009 and 2010" -> "observed at 26.5°N in 2005, 2010, 2011 and 2013"?
518, 528, fig 13: why not plot the other 2 models as well?
Fig 13 caption: state that the time scale is compressed prior to 2000.
539: 15°N -> 18°N?
540, 541: swap 10 - 20°N and 20-30°N (or is fig14a key wrong?)
542: MHT peaks around 24°N -> MHT peaks around 24°N but is not well constrained given the error bars
542-589: MHT -> AMHT
548: remove "The strongest heat transport is found in the eddy-rich ocean." - repeated below
550: GLOB16 tracks the ECMWF estimates and compares well with TF08 -> GLOB16 tracks the ECMWF estimates and compares well with TF08 except north of 40°N
552: Hirschi et al. 2019 -> Hirschi et al. 2020 ?
556: 18°N -> 15°N ?
565: slightly exceeds the total MHT between the equator and 15°N -> slightly exceeds the total MHT between the equator and 15°N and south of 20°S
568: gyre one increases to level off -> gyre component increases to level off at total AMHT
574: remove "not shown for ORCA025 575 and ORCA1" - this difference is visible in fig 14a.
578: misrepresent -> misrepresents
579: 2010, 2011, 2013 and 2017 minima -> 2010, 2011, 2013, 2017 and 2019 minima ?
Fig 14b: why not include the other 2 models?
608: negative -> positive
617, table 1: was Rayleigh drag used in the straits at low resolution?
629: plot Donohue et al value in fig 15c
631: below the most recent estimates (Xu et al., 2020) -> below the most recent estimates (Xu et al., 2020) and some eddy-rich models (Kiss et al., 2020)
Fig 15 caption: (b) the Indonesian Throughflow -> (b) the southward Indonesian Throughflow
Fig 15 caption: Cite sources for obs in a & b671: provide -> provides
679: Indian to the Pacific -> Pacific to Indian
683: (weaker than observed values) -> (weaker than observed values and some other eddy-rich models)
Citation: https://doi.org/10.5194/egusphere-2023-469-RC2 -
AC2: 'Reply on RC2', Doroteaciro Iovino, 14 Aug 2023
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-469/egusphere-2023-469-AC2-supplement.pdf
-
AC2: 'Reply on RC2', Doroteaciro Iovino, 14 Aug 2023
Peer review completion
Journal article(s) based on this preprint
Viewed
| HTML | XML | Total | BibTeX | EndNote | |
|---|---|---|---|---|---|
| 383 | 165 | 22 | 570 | 11 | 6 |
- HTML: 383
- PDF: 165
- XML: 22
- Total: 570
- BibTeX: 11
- EndNote: 6
Viewed (geographical distribution)
| Country | # | Views | % |
|---|
| Total: | 0 |
| HTML: | 0 |
| PDF: | 0 |
| XML: | 0 |
- 1
Cited
Doroteaciro Iovino
Pier Giuseppe Fogli
Simona Masina
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(7773 KB) - Metadata XML