Articles | Volume 18, issue 24
https://doi.org/10.5194/amt-18-7603-2025
© Author(s) 2025. This work is distributed under the Creative Commons Attribution 4.0 License.
A method for characterizing the spatial organization of deep convective cores in deep convective systems' cloud shield using idealized elementary convective structure decomposition
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- Final revised paper (published on 15 Dec 2025)
- Supplement to the final revised paper
- Preprint (discussion started on 19 Jun 2025)
- Supplement to the preprint
Interactive discussion
Status: closed
Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor
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RC1: 'Comment on egusphere-2025-2247', Anonymous Referee #1, 21 Jul 2025
- AC1: 'Reply on RC1', Louis Netz, 02 Oct 2025
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RC2: 'Comment on egusphere-2025-2247', Anonymous Referee #2, 28 Jul 2025
- AC2: 'Reply on RC2', Louis Netz, 02 Oct 2025
Peer review completion
AR – Author's response | RR – Referee report | ED – Editor decision | EF – Editorial file upload
AR by Louis Netz on behalf of the Authors (03 Oct 2025)
Author's response
Author's tracked changes
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ED: Referee Nomination & Report Request started (06 Oct 2025) by Andrew Sayer
RR by Anonymous Referee #2 (04 Nov 2025)
ED: Reconsider after major revisions (05 Nov 2025) by Andrew Sayer
AR by Louis Netz on behalf of the Authors (24 Nov 2025)
Author's response
Author's tracked changes
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ED: Publish as is (25 Nov 2025) by Andrew Sayer
AR by Louis Netz on behalf of the Authors (27 Nov 2025)
Review: A method for characterizing the spatial organization of deep convective cores in deep convective systems’ cloud shield
This paper introduces a novel method to classify and study the spatial organization and geometry of convective systems as well as their distribution of convective cores. Four key metrics are introduced based on infrared brightness temperatures in geostationary satellite observations and outgoing longwave radiation in km-scale numerical simulations (with a delta x of 3km) of idealized cloud scenes. The metrics give a more holistic description of convective organization, including the size and relative fraction of convective cores as well as their spatial arrangement and randomness. The metrics are discussed well in the context of already existing metrics for convective organization and the authors make an argument that convective organization cannot be well described when relying on one single parameter instead of combining different aspects of the spatial structure. Overall, the paper is well-structured, well-written and is a valuable contribution to allow for a more sophisticated analysis of convective processes. While I do not think that any additional analyses are needed, I think there are still a few parts in the paper that need clarifications, in particular because the main point of the paper is to introduce a new technique that should be straightforward to reproduce. I recommend the paper for minor revisions.
General comments
Physical processes
Acknowledging that this paper focuses on the introduction and development of a new method, it is not expected that the conclusions center around new findings about convective organization. However, I think the paper would benefit from explaining how the introduced metrics and the classes that are based upon these four metrics, could be used to identify certain processes. Right now, the differences in the distributions (e.g. in Fig. 13-14) are not really discussed in the context of which underlying weather systems and processes would produce the different signatures in convective organization. In addition, it would be useful to name a few examples of how this method can be applied in weather and climate research.
Decomposition into elementary structure
It appears to me that the decomposition into the elementary structures that is based on the square-like nature of the convective core has implications for the characteristic length L. Can you explain in more detail if this assumption is a limitation for the range of L values that you get?
Differences between observations and model simulations
In the very beginning of the paper, the definition of “convective” vs. “stratiform” is introduced for models and observations. I am wondering how much of the differences that you find between the datasets actually go back to how you define “convective” in the model dataset. It makes sense to base this definition on physical processes such as updrafts, but I am afraid that, as you mention yourself, this would lead to significantly different regions than the purely radar-based signature in the satellite observations. In addition to that, I think that the paper would benefit from a more thorough discussion of differences between models and observations, as an example for how to apply the introduced method (i.,e. that it can help to validate models that partly resolve convective processes).
Figure labels
The font size in all figures need to be increased. In some figures, such as, Fig. 3, the labels are barely readable.
Detailed comments
L,. 134 ff: When introducing the radar collocations, could you clarify which variables you are working with - is it only the retrieved rain rates or other retrieved quantities? Do you leverage the radar reflectivity values at all?
Fig. 4: Is the core size given in the number of pixels?
Fig. 5: Add in the figure caption that this is for the satellite data. Are those the composites over all tracked DCSs?
Fig. 11: The difference in the maximal area between the satellite data and the model simulation appears to be quite significant. Is this a consequence of the effective resolution of the datasets, and does this indicate that the model physics cannot reproduce the large cloud shields that we can observe? In addition, the duration of the DCs seems similar, which is interesting because the spatial and temporal scales should also be linked or not? I think it would be useful to discuss this point in more detail.
L. 546: If I understood it correctly, K-means clustering is used to produce the four classes in Fig. 13 and these classes are based on the multivariate coherence of the four metrics. It is, however, not explained in detail how the PDFs of each metric relate to the respective class (from random to organized). For instance, Fig. 13 a) shows quite distinct distributions for F between class 0 and 1 although these are the classes closer related to each other. I do not expect to go into the details of all possible combinations of the four metrics, but it would be decent to describe a little bit more how convective systems with substantially different distributions for F and P can still be more alike each other when they are similar in terms of L and S.