Articles | Volume 18, issue 3
https://doi.org/10.5194/gmd-18-621-2025
© Author(s) 2025. This work is distributed under the Creative Commons Attribution 4.0 License.
Accurate space-based NOx emission estimates with the flux divergence approach require fine-scale model information on local oxidation chemistry and profile shapes
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- Final revised paper (published on 05 Feb 2025)
- Preprint (discussion started on 23 Aug 2024)
Interactive discussion
Status: closed
Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor
| : Report abuse
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RC1: 'Comment on egusphere-2024-2225', Gerrit Kuhlmann, 23 Sep 2024
- AC2: 'Reply on RC1', Felipe Cifuentes, 22 Nov 2024
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RC2: 'Comment on egusphere-2024-2225', Anonymous Referee #2, 09 Oct 2024
- AC1: 'Reply on RC2', Felipe Cifuentes, 22 Nov 2024
Peer review completion
AR – Author's response | RR – Referee report | ED – Editor decision | EF – Editorial file upload
AR by Felipe Cifuentes on behalf of the Authors (27 Nov 2024)
Author's response
Author's tracked changes
Manuscript
ED: Referee Nomination & Report Request started (28 Nov 2024) by Volker Grewe
RR by Anonymous Referee #2 (02 Dec 2024)
RR by Gerrit Kuhlmann (06 Dec 2024)
ED: Publish as is (06 Dec 2024) by Volker Grewe
AR by Felipe Cifuentes on behalf of the Authors (13 Dec 2024)
General comments
The authors present a comprehensive analysis of the flux divergence method (FDA) using model fields created with the LOTOS-EUROS model for the Netherlands. The paper provides new insights in the accuracy of the FDA model. The paper is written well and the structure is clear. The methods are outlined well and clear with a few open questions:
Specific comments
L65ff: The differentiation between "plume dispersion models" and "mass conservation" is oversimplified here. The assumption of mass conservation is also used for methods that are applied to single sources (e.g. cross-sectional flux, Gaussian plume inversion and integrated mass enhancement). The statement "no need to run a computationally expensive CTM" contradicts the main conclusion of the study that CTM simulations are needed (last sentence in the abstract).
L75f: There have been some studies that have analyzed the FDA accuracy using model data: e.g. Goldberg at. 2022 and Hakkarainen et al. 2022.
L109f: You could mention here, why updating the a priori profile only partially corrects the bias.
L137: Please clarify if emissions were released at the surface or vertical profiles were used. If emissions were released at the surface, it is likely that all NOx remains in the PBL. However, vertical profiles can release NOx into the free troposphere (in particular for low PBL), which has implications on the performance of using PBL columns only.
L161ff: Koene et al. 2024 show that divergence should be computed over the smallest region possible to avoid noise negatively affecting the divergence calculation (recommendation 5). A forth-order difference is therefore likely less ideal. You probably do not see the impact here, as you do not include noise in your NO2 fields. However, I think it would be good to note that for application to noisy satellite images, a lower-order operator might be better.
L173ff: While NOX concentrations are stable around TROPOMI overpass, increasing turbulent mixing can still badly break the steady-state assumption inside plumes resulting in biased divergence fields.
L180ff: Since the NO2 enhancement will always have a vertical extent, the effective wind speed should be computed using the concentration profile of the NO2 enhancement. Half the PBL height is a good approximation of the mean wind speed inside the PBL assuming well-mixed NO2 concentrations, which isn't a bad assumption for cities or a few kilometers downstream of stack source (e.g. Krol et al. 2024).
L187f: The wind divergence will remain zero for a total column (assuming incompressible air), but not for partial column (e.g., PBL column), because air can leave or enter at the top of the partial column. In theory, it is possible to compute a two-dimensional wind, but this would require that you know both the NO2 and wind profile (Koene et al. 2024). Thus, errors in the wind are caused by using (a) only a partial NO2 column and (b) the wind field at a single (spatial varying) altitude.
L222f: The paragraph should acknowledge recent studies that have used different NOx partitioning factors: "Often a constant NOx:NO2 ratio is assumed to infer the NO emissions from space-based NO observations. Many studies (e.g., Beirle et al., 2011, Beirle et al., 2019, de Foy and Schauer, 2022, Merlaud et al., 2020, Shaiganfar et al., 2017, Ionov et al., 2022, Potts et al., 2022, Hakkarainen et al., 2021) use the steady-state noontime molar concentration ratio under typical urban conditions of 1.32 based on Seinfeld and Pandis (2006). Recently, model-based concentration ratios have also been calculated using simulations from Copernicus Atmospheric Monitoring Service (CAMS, Lorente et al., 2019, Rey-Pommier et al., 2022) and Comprehensive Air Quality Model with Extensions (CAMx, Goldberg et al., 2022). Beirle et al. (2021) calculated NOx:NO2 ratios according to the photo-stationary steady state. In general, these studies show small deviations from the value 1.32 (e.g., 1.16–1.83), but acknowledge that values near the point sources are likely to be higher. CHIMERE model simulations (Shaiganfar et al., 2017) further indicate that in large circles around Paris, the partitioning ratios are smaller during summer (1.32) than in winter (1.51), due to the higher ozone mixing ratios in summer. In contrast to model-based analyses, the Dutch aircraft measurements of in-plume NOx/NO2 ratios from power stations (e.g., Janssen, 1988, Vilà-Guerau de Arellano et al., 1990, Bange et al., 1991, Hanrahan, 1999) often showed values higher than 10 near the source and values between 2 and 10 up to 15 km from the source." (Hakkarainen et al. 2024).
L245: I am also not aware of any studies that subtracted the background from NO2 observations. The background has also been subtracted from CO2 columns by Hakkarainen et al. (2022). Koene et al. (2024) show that removing the background eliminates the steady-state assumption for the background component.
L304ff: You earlier state that using a second-order difference instead of fourth-order difference had only a minor impact on your results. This contradicts your statement here that the fourth-order difference cause (strong) spatial smearing.
Therefore, the smearing likely has a different explanation: I would expect some smoothing from LOTOS-EUROS depending on the model dispersion settings, as the effective model resolution is typically coarser than grid resolution of 2 km. It is also possible that LOTUS-EUROS is not mass conserving at strong point sources.
L335ff: Is using the PBL column still feasible, if strong point sources release in the free troposphere in particular for low PBLs? Was this include in the model simulations?
L384f: As noted above, many recent studies used values other than 1.32.
L401f: The impact of the divergence-free winds is likely small, because you subtract the background from the NO2 column. Koene et al (2024) show that omitting the wind divergence term is useful if the background is not removed from the column.
L416f/L440ff: Do you use only PBL columns in this case study? I would expect that in the morning the PBL is very low, which would "leak" some NO2 in the free troposphere and thus result in an underestimation of the emissions.
L486: An underestimation of the emissions by 18% is still larger than 11% from the synthetic data. Can you provide a brief a discussion for the reasons? Is the bias due to overestimated emissions in simulation or caused by the FDA method?
L530f: Most studies use ERA-5 wind fields instead high-resolution simulations. Do you expect an impact on estimated emissions using ERA-5 fields?
L553: What are the implications for Sentinel-5 with an overpass time of 9:30 LT?
Technical corrections
L6: Summer -> summer
L98: DOAS -> Differential Optical Absorption Spectroscopy (DOAS)
Figure 3: Mention that the figure is for ID06.
Table 3: Please add units.
Figure A6: Colorscale is not ideal.
References
Goldberg et al., https://doi.org/10.5194/acp-22-10875-2022, 2022.
Hakkarainen et al., https://doi.org/10.3389/frsen.2022.878731, 2022.
Koene et al., https://doi.org/10.1029/2023JD039904, 2024.
Krol et al., https://doi.org/10.5194/acp-24-8243-2024, 2024.
Hakkarainen et al., https://doi.org/10.1016/j.apr.2024.102171, 2024.