Improving radar-based rainfall nowcasting by a nearest-neighbour approach – Part 1: Storm characteristics
<p>The nowcast of rainfall storms at fine temporal and spatial resolutions is quite challenging due to the unpredictable nature of rainfall at such scales. Typically, rainfall storms are recognized by weather radar and extrapolated in the future by the Lagrangian persistence. However, storm ev...
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Format: | Article |
Language: | English |
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Copernicus Publications
2022-03-01
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Series: | Hydrology and Earth System Sciences |
Online Access: | https://hess.copernicus.org/articles/26/1631/2022/hess-26-1631-2022.pdf |
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author | B. Shehu U. Haberlandt |
author_facet | B. Shehu U. Haberlandt |
author_sort | B. Shehu |
collection | DOAJ |
description | <p>The nowcast of rainfall storms at fine temporal and spatial resolutions is
quite challenging due to the unpredictable nature of rainfall at such
scales. Typically, rainfall storms are recognized by weather radar and extrapolated in the future by the Lagrangian persistence. However, storm
evolution is much more dynamic and complex than the Lagrangian persistence,
leading to short forecast horizons, especially for convective events. Thus, the aim of this paper is to investigate the improvement that past similar
storms can introduce to the object-oriented radar-based nowcast. Here we propose a nearest-neighbour approach that measures first the similarity
between the “to-be-nowcasted” storm and past observed storms and later uses the behaviour of the past most similar storms to issue either a single
nowcast (by averaging the 4 most similar storm responses) or an ensemble nowcast (by considering the 30 most similar storm responses). Three questions are tackled here. (i) What features should be used to describe storms in
order to check for similarity? (ii) How should similarity between past storms be measured? (iii) Is this similarity useful for object-oriented nowcast? For
this purpose, individual storms from 110 events in the period 2000–2018
recognized within the Hanover Radar Range (<span class="inline-formula"><i>R</i>∼115</span> km<span class="inline-formula"><sup>2</sup></span>), Germany, are used as a basis for investigation. A “leave-one-event-out”
cross-validation is employed to test the nearest-neighbour approach for the prediction of the area, mean intensity, the <span class="inline-formula"><i>x</i></span> and <span class="inline-formula"><i>y</i></span> velocity components, and
the total lifetime of the to-be-nowcasted storm for lead times from <span class="inline-formula">+</span> 5 min up to <span class="inline-formula">+</span> 3 h. Prior to the application, two importance analysis methods (Pearson correlation and partial information correlation) are
employed to identify the most important predictors. The results indicate
that most of the storms behave similarly, and the knowledge obtained from such similar past storms helps to capture better the storm dissipation and
improves the nowcast compared to the Lagrangian persistence, especially for convective events (storms shorter than 3 h) and longer lead times (from
1 to 3 h). The main advantage of the nearest-neighbour approach is seen when applied in a probabilistic way (with the 30 closest neighbours as
ensembles) rather than in a deterministic way (averaging the response from the four closest neighbours). The probabilistic approach seems promising, especially
for convective storms, and it can be further improved by either increasing the sample size, employing more suitable methods for the
predictor identification, or selecting physical predictors.</p> |
first_indexed | 2024-12-13T19:54:21Z |
format | Article |
id | doaj.art-b5b8ae1f8fd2433c9cac53ed008b258d |
institution | Directory Open Access Journal |
issn | 1027-5606 1607-7938 |
language | English |
last_indexed | 2024-12-13T19:54:21Z |
publishDate | 2022-03-01 |
publisher | Copernicus Publications |
record_format | Article |
series | Hydrology and Earth System Sciences |
spelling | doaj.art-b5b8ae1f8fd2433c9cac53ed008b258d2022-12-21T23:33:21ZengCopernicus PublicationsHydrology and Earth System Sciences1027-56061607-79382022-03-01261631165810.5194/hess-26-1631-2022Improving radar-based rainfall nowcasting by a nearest-neighbour approach – Part 1: Storm characteristicsB. ShehuU. Haberlandt<p>The nowcast of rainfall storms at fine temporal and spatial resolutions is quite challenging due to the unpredictable nature of rainfall at such scales. Typically, rainfall storms are recognized by weather radar and extrapolated in the future by the Lagrangian persistence. However, storm evolution is much more dynamic and complex than the Lagrangian persistence, leading to short forecast horizons, especially for convective events. Thus, the aim of this paper is to investigate the improvement that past similar storms can introduce to the object-oriented radar-based nowcast. Here we propose a nearest-neighbour approach that measures first the similarity between the “to-be-nowcasted” storm and past observed storms and later uses the behaviour of the past most similar storms to issue either a single nowcast (by averaging the 4 most similar storm responses) or an ensemble nowcast (by considering the 30 most similar storm responses). Three questions are tackled here. (i) What features should be used to describe storms in order to check for similarity? (ii) How should similarity between past storms be measured? (iii) Is this similarity useful for object-oriented nowcast? For this purpose, individual storms from 110 events in the period 2000–2018 recognized within the Hanover Radar Range (<span class="inline-formula"><i>R</i>∼115</span> km<span class="inline-formula"><sup>2</sup></span>), Germany, are used as a basis for investigation. A “leave-one-event-out” cross-validation is employed to test the nearest-neighbour approach for the prediction of the area, mean intensity, the <span class="inline-formula"><i>x</i></span> and <span class="inline-formula"><i>y</i></span> velocity components, and the total lifetime of the to-be-nowcasted storm for lead times from <span class="inline-formula">+</span> 5 min up to <span class="inline-formula">+</span> 3 h. Prior to the application, two importance analysis methods (Pearson correlation and partial information correlation) are employed to identify the most important predictors. The results indicate that most of the storms behave similarly, and the knowledge obtained from such similar past storms helps to capture better the storm dissipation and improves the nowcast compared to the Lagrangian persistence, especially for convective events (storms shorter than 3 h) and longer lead times (from 1 to 3 h). The main advantage of the nearest-neighbour approach is seen when applied in a probabilistic way (with the 30 closest neighbours as ensembles) rather than in a deterministic way (averaging the response from the four closest neighbours). The probabilistic approach seems promising, especially for convective storms, and it can be further improved by either increasing the sample size, employing more suitable methods for the predictor identification, or selecting physical predictors.</p>https://hess.copernicus.org/articles/26/1631/2022/hess-26-1631-2022.pdf |
spellingShingle | B. Shehu U. Haberlandt Improving radar-based rainfall nowcasting by a nearest-neighbour approach – Part 1: Storm characteristics Hydrology and Earth System Sciences |
title | Improving radar-based rainfall nowcasting by a nearest-neighbour approach – Part 1: Storm characteristics |
title_full | Improving radar-based rainfall nowcasting by a nearest-neighbour approach – Part 1: Storm characteristics |
title_fullStr | Improving radar-based rainfall nowcasting by a nearest-neighbour approach – Part 1: Storm characteristics |
title_full_unstemmed | Improving radar-based rainfall nowcasting by a nearest-neighbour approach – Part 1: Storm characteristics |
title_short | Improving radar-based rainfall nowcasting by a nearest-neighbour approach – Part 1: Storm characteristics |
title_sort | improving radar based rainfall nowcasting by a nearest neighbour approach part 1 storm characteristics |
url | https://hess.copernicus.org/articles/26/1631/2022/hess-26-1631-2022.pdf |
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