the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
A multi-instrument fuzzy logic boundary-layer top detection algorithm
Abstract. Understanding the boundary-layer height and its dynamics is crucial for a wide array of applications spanning various fields. Accurate identification of the boundary-layer top contributes to improved air quality predictions, pollutant transport assessments, and enhanced numerical weather prediction through parameterization and assimilation techniques. Despite its significance, defining and observing the boundary-layer top remains challenging. Existing methods of estimating the boundary-layer height encompass radiosonde-based methods, radar-based retrievals, and more. As emerging boundary-layer observation platforms emerge, it is useful to reevaluate the efficacy of existing boundary-layer top detection methods and explore new ones.
This study introduces a fuzzy-logic algorithm that leverages the synergy of multiple remote-sensing boundary-layer profiling instruments. By harnessing the distinct advantages of each sensing platform, the proposed method enables accurate boundary-layer height estimation both during daytime and nocturnal conditions. The algorithm is benchmarked against radiosonde-derived boundary-layer top estimates obtained from balloon launches across diverse locations in Wisconsin, Oklahoma, and Louisiana during summer and fall. The findings reveal notable similarities between the results produced by the proposed fuzzy-logic algorithm and traditional radiosonde-based approaches. However, this study delves into the nuanced differences in their behavior, providing insightful analyses about the underlying causes of the observed discrepancies. The fuzzy-logic boundary-layer top detection algorithm, called BLISS-FL, is released publicly fostering collaboration and advancement within the research community.
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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.
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Preprint
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The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
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- Final revised paper
Journal article(s) based on this preprint
Interactive discussion
Status: closed
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CC1: 'Radar question - Comment on egusphere-2023-2050', Vagner Castro, 14 Dec 2023
Dear Author,
Your study mentions using radar data. Would you mind sharing some specific details about the system, like the type and the operating frequency?
Thanks,
Vagner
Citation: https://doi.org/10.5194/egusphere-2023-2050-CC1 -
CC2: 'Reply on CC1', Jacob Carlin, 15 Dec 2023
Thank you for your comment. The current study does not make direct use of any radar data. However, as discussed in section 3.3, part of the CLAMPS dataset used for validation was collected during a study comparing CLAMPS BL depth estimates using the proposed algorithm and radar Bragg-scatter-based estimates. In that case, we used data from the polarimetric WSR—88D radars that comprise the NEXRAD network in the United States, which operate in the S band between 2.7 and 3.0 GHz (e.g., https://nap.nationalacademies.org/read/10394/chapter/11). The results of that comparison are forthcoming in a follow-up study.Â
Citation: https://doi.org/10.5194/egusphere-2023-2050-CC2
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CC2: 'Reply on CC1', Jacob Carlin, 15 Dec 2023
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RC1: 'Comment on egusphere-2023-2050', Anonymous Referee #1, 05 Jan 2024
This paper presents the results of using a fuzzy logic algorithm with a combination of doppler lidar, radiance inferometer and microwave radiometer, with validation done by comparisons with radiosonde data. I feel the paper needs a major revision as the presentation is confusing and the results are not very clear. I realize that there are lots of different cases to present, and many options in the radiosonde comparisons, but in the end, it's not obvious as to how these retrievals might ultimately be used. But I think a rewrite could make it much easier to extract this information. My specific comments are:
1. Both the and abstract should state more clearly what observations are being used for the retrieval and validation (see the first sentence above).Â2. Line 110: do you mean the first generation step in B18, or is this changed in the current algorithm?
3. Line 126:Â Why are buoyant processes important during the night? This seems counter intuitive as buoyancy should grow during the daytime.
4. Line 131:Â So you mean that the B18 algorithm was not successful in estimating overnight BL height?
5. Section 3:Â Do radiosonde observations measure thermodynamic BLH rather than the ML height? If so, is it really a good comparison?
6. Line 402:Â It is fine not to recommend a preferred radiosonde PBLH algorithm, but it would be really helpful to see a plot likeÂ
7. Figure 3 is really helpful to see the evolution of the PBLH estimate during the course of a day. It would be even better if you could plot the radiosonde estimates of PBLH on top of this. There is lots of discussion of how the algorithm does at different times of the day, but much of this could be clarified with a comparison like this.
8. The summary section (5) doesn't really have any concrete conclusions. As you say, it's hard to make a fair comparison since a 100 m difference means something very different depending on the time of day. But plotting the height estimates in comparison to radiosondes as a function of time would really help with this.Â
9. Figure 7: It's not clear what you mean by dark and light colors.
10. Table 3 appears to be the primary result of this work. Would it help to include a percent difference along with the absolute difference?
Citation: https://doi.org/10.5194/egusphere-2023-2050-RC1 -
AC1: 'Reply to RC1', Elizabeth Smith, 07 Feb 2024
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2050/egusphere-2023-2050-AC1-supplement.pdf
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AC1: 'Reply to RC1', Elizabeth Smith, 07 Feb 2024
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RC2: 'Comment on egusphere-2023-2050', Anonymous Referee #2, 06 Jan 2024
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AC2: 'Reply to RC2', Elizabeth Smith, 07 Feb 2024
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2050/egusphere-2023-2050-AC2-supplement.pdf
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AC2: 'Reply to RC2', Elizabeth Smith, 07 Feb 2024
Interactive discussion
Status: closed
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CC1: 'Radar question - Comment on egusphere-2023-2050', Vagner Castro, 14 Dec 2023
Dear Author,
Your study mentions using radar data. Would you mind sharing some specific details about the system, like the type and the operating frequency?
Thanks,
Vagner
Citation: https://doi.org/10.5194/egusphere-2023-2050-CC1 -
CC2: 'Reply on CC1', Jacob Carlin, 15 Dec 2023
Thank you for your comment. The current study does not make direct use of any radar data. However, as discussed in section 3.3, part of the CLAMPS dataset used for validation was collected during a study comparing CLAMPS BL depth estimates using the proposed algorithm and radar Bragg-scatter-based estimates. In that case, we used data from the polarimetric WSR—88D radars that comprise the NEXRAD network in the United States, which operate in the S band between 2.7 and 3.0 GHz (e.g., https://nap.nationalacademies.org/read/10394/chapter/11). The results of that comparison are forthcoming in a follow-up study.Â
Citation: https://doi.org/10.5194/egusphere-2023-2050-CC2
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CC2: 'Reply on CC1', Jacob Carlin, 15 Dec 2023
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RC1: 'Comment on egusphere-2023-2050', Anonymous Referee #1, 05 Jan 2024
This paper presents the results of using a fuzzy logic algorithm with a combination of doppler lidar, radiance inferometer and microwave radiometer, with validation done by comparisons with radiosonde data. I feel the paper needs a major revision as the presentation is confusing and the results are not very clear. I realize that there are lots of different cases to present, and many options in the radiosonde comparisons, but in the end, it's not obvious as to how these retrievals might ultimately be used. But I think a rewrite could make it much easier to extract this information. My specific comments are:
1. Both the and abstract should state more clearly what observations are being used for the retrieval and validation (see the first sentence above).Â2. Line 110: do you mean the first generation step in B18, or is this changed in the current algorithm?
3. Line 126:Â Why are buoyant processes important during the night? This seems counter intuitive as buoyancy should grow during the daytime.
4. Line 131:Â So you mean that the B18 algorithm was not successful in estimating overnight BL height?
5. Section 3:Â Do radiosonde observations measure thermodynamic BLH rather than the ML height? If so, is it really a good comparison?
6. Line 402:Â It is fine not to recommend a preferred radiosonde PBLH algorithm, but it would be really helpful to see a plot likeÂ
7. Figure 3 is really helpful to see the evolution of the PBLH estimate during the course of a day. It would be even better if you could plot the radiosonde estimates of PBLH on top of this. There is lots of discussion of how the algorithm does at different times of the day, but much of this could be clarified with a comparison like this.
8. The summary section (5) doesn't really have any concrete conclusions. As you say, it's hard to make a fair comparison since a 100 m difference means something very different depending on the time of day. But plotting the height estimates in comparison to radiosondes as a function of time would really help with this.Â
9. Figure 7: It's not clear what you mean by dark and light colors.
10. Table 3 appears to be the primary result of this work. Would it help to include a percent difference along with the absolute difference?
Citation: https://doi.org/10.5194/egusphere-2023-2050-RC1 -
AC1: 'Reply to RC1', Elizabeth Smith, 07 Feb 2024
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2050/egusphere-2023-2050-AC1-supplement.pdf
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AC1: 'Reply to RC1', Elizabeth Smith, 07 Feb 2024
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RC2: 'Comment on egusphere-2023-2050', Anonymous Referee #2, 06 Jan 2024
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AC2: 'Reply to RC2', Elizabeth Smith, 07 Feb 2024
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2050/egusphere-2023-2050-AC2-supplement.pdf
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AC2: 'Reply to RC2', Elizabeth Smith, 07 Feb 2024
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Elizabeth N. Smith
Jacob T. Carlin
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(10816 KB) - Metadata XML