Articles | Volume 17, issue 4
https://doi.org/10.5194/gmd-17-1689-2024
© Author(s) 2024. This work is distributed under the Creative Commons Attribution 4.0 License.
Flux coupling approach on an exchange grid for the IOW Earth System Model (version 1.04.00) of the Baltic Sea region
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- Final revised paper (published on 26 Feb 2024)
- Preprint (discussion started on 01 Sep 2023)
- Supplement to the preprint
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Status: closed
Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor
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RC1: 'Comment on gmd-2023-166', Anonymous Referee #1, 11 Sep 2023
- AC1: 'Reply on RC1', Sven Karsten, 21 Nov 2023
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RC2: 'Comment on gmd-2023-166', Anonymous Referee #2, 20 Sep 2023
- AC2: 'Reply on RC2', Sven Karsten, 21 Nov 2023
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AR – Author's response | RR – Referee report | ED – Editor decision | EF – Editorial file upload
AR by Sven Karsten on behalf of the Authors (21 Nov 2023)
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ED: Publish subject to minor revisions (review by editor) (08 Dec 2023) by Sophie Valcke
AR by Sven Karsten on behalf of the Authors (18 Dec 2023)
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ED: Publish subject to technical corrections (03 Jan 2024) by Sophie Valcke
AR by Sven Karsten on behalf of the Authors (03 Jan 2024)
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This article provides a fairly comprehensive description of the exchange grid method used in a regional ocean-atmosphere model of the Baltic Sea region.
The exchange grid developed at GFDL is a relatively old one. But it is not widely used. And it is very little described in the literature, and in that sense the description and fairly complete analysis in this article is very welcome, with an interest that extends beyond the Baltic modellers. The analyse of the different exchange grids is interesting. The article is well suited to the scope of GMD in the model description paper category.
The flux calculator allows to take into account heterogeneity in a model grid box. It still make strong assumptions on what is homogeneous :
1/ In this coupling scheme, there is the assumption that even above surfaces of variable temperature, the atmosphere is homogeneous, on the scale of a model grid box, from the first level of the model to the top. This is a very strong assumption, and in fact a priori false. You only have to look at the clouds above a free water-sea ice front to that at least the planetary boundary layer may have very different vertical structure within one atmosphere grid box.
2/ The transfer coefficients ch and cm are sent by the atmosphere (Fig. 4). They are not calculated by the flux calculator. It is quite possible in reality to have stable air above the ice and unstable air above the open water. This yield very different transfert coefficients above the two surfaces. This should lead to very different flux compare to what the flux calculator computes. Note that if the calculations of these coefficients involve iterations in the atmosphere, this can indeed be complicated to compute them in the flux calculator.
This two limitations should be explained to the reader, with if possible some descriptions of the potential impact, and technical constraints that explained the chosen algorithm.
Major concerns.
I didn't really succeeded to catch the time pattern of exchanges. Fig. 5 is supposed to address this issue, but it doesn't explain how exchanges are synchronised with models time stepping, and the frontiers of the time steps. We need a time sketch showing when the different components (models and flux calculator) are working, when they are waiting, etc ...
In Fig. 2, Fig. 3 and Fig.4, an ocean grid cell is either ice free or fully ice covered. But line 145 reads that fluxes are computed for free ocean and each ice category. Do you consider partially ice covered ocean grid boxes, with several ice categories ? Is so, please show ice fraction and ice categories (by thickness classes ?) in the figures, and give more details in the text about the flux computation over different surfaces.
Radiation is not computed by the flux calculator. But each ocean grid cell may have different albedos, especially if there is sea ice. Do all ocean grid cells receive the same short wave flux ? Or do you use the albedos of each cell and surface type (water, ice) to redistribute the solar flux ? With no redistribution, the flux can be very unrealistic (for instance very low solar flux toward ocean when the ice fraction is large, very high solar flux on ice when ice fraction is low). Please details that, and address the potential impact of your procedure.
Minor concerns
Line 59 "by (Balaji et al. 2006)" -> "by Balaji et al. (2006)"
Line 174, 183, 188. The atmospheric wind speed is used in the bulk formulae. In Fig. 5, exchanged variables include Uair, Vair, U10m, V10m. What is the difference, and what variables are used in which flux computation ?
Line 189 : "It is noteworthy, that the horizontal velocity components of the ocean’s water body are negligible compared to the atmospheric ones and are thus omitted". That's true if the model does not resolve the tides. Is it the case ?
Line 200 : "Moreover, the presented formulas might be updated to more elaborate schemes using more sophisticated theories e.g. a TKE-based ansatz for the calculation of transfer coefficients (Doms et al., 2011)." As the transfert coefficients are computed in the atmosphere, and not in the flux calculator, it seems not feasible to implement a TKE formulation in the flux calculator.
Line 219 : time steps are 600s and 150s for the oceanic and atmospheric model, respectively. For the atmosphere I suppose that this is the 'physics' time step, and advection is called more frequently ? A question important for the coupling is the time step of the computation of solar radiation. Is it called at the same pace than the coupling ? Or with a longer time step ?