Analysis of Dual Polarization Characteristics of Turbulent Structure from Hail Supercell Storms
Convective storms transmit momentum through turbulence， so it is important to understand the echo characteristics of turbulence structure in severe convective storms.Focusing on the velocity spectrum width above 5 m·s -1， the turbulent intensity of two strong hailstorm supercells with different inte...
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Science Press, PR China
2023-02-01
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| Series: | Gaoyuan qixiang |
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| Online Access: | http://www.gyqx.ac.cn/EN/10.7522/j.issn.1000-0534.2022.00027 |
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| author | Juxiu WU Ming WEI Xiuguang DIAO Jiawen PAN |
| author_facet | Juxiu WU Ming WEI Xiuguang DIAO Jiawen PAN |
| author_sort | Juxiu WU |
| collection | DOAJ |
| description | Convective storms transmit momentum through turbulence， so it is important to understand the echo characteristics of turbulence structure in severe convective storms.Focusing on the velocity spectrum width above 5 m·s
-1， the turbulent intensity of two strong hailstorm supercells with different intensity of mesocyclones are analyzed， and the relationship between airflow structure and turbulence enhancement are revealed.The results show that： （1） The strong hail supercell has moderate or above intensity turbulence in the strong updraft region， and the supercell triggered by the gust front also shows moderate intensity spectrum width in the inflow path， indicating the possibility of moderate intensity turbulence.（2） In general， the strongest turbulence occurs in the region with the largest velocity shear intensity.The maximum spectrum width of the supercell with moderate intensity mesocyclone is about 10 ms
-1， with differential reflectivity factor （
ZDR） within 1dB， echo intensity exceeding 35 dBZ， and larger differential phase shift rate （
KDP）.The strong turbulence region of the supercell with strong mesocyclone is mainly located at the intersection of positive and negative velocities at the top of
ZDR column， and the spectral width near the mesocyclone can reach 16.5 m·s
-1， and the side near the strong echo core contains more supercooled water， with about 0.96 of correlation coefficient （CC） and large
KDP.While， the echo intensity on the other side is slightly lower， with CC low to 0.85， where graupel particles and large raindrops brought by updraft exist.These regions of strong turbulence indicate the path of momentum transmission.（3） The upper part of the supercell storm has the strongest turbulence， both updrafts and downdrafts are strong， but the turbulence is stronger near the downdrafts that probably related to horizontal shear of the wind， where the highest spectrum width for strong mesocyclone is 17.5 m·s
-1， and
ZDR is higher than that in the updraft and
KDP is negative， but
KDP is about 0 （°）·km
-1 and
ZDR is about 0 dB in the updrafts， however， spectrum width of the storm with moderate mesocyclone increases slightly.Strong mesocyclone supercell has stronger turbulence enhancement， and these discussions provide a reference for understanding the turbulence structure and momentum transmission of severe storms by dual-polarization radar observation. |
| format | Article |
| id | doaj-art-7f5d4356b9bc4df3bdac003d6ddaa7a9 |
| institution | OA Journals |
| issn | 1000-0534 |
| language | zho |
| publishDate | 2023-02-01 |
| publisher | Science Press, PR China |
| record_format | Article |
| series | Gaoyuan qixiang |
| spelling | doaj-art-7f5d4356b9bc4df3bdac003d6ddaa7a92025-08-20T02:11:17ZzhoScience Press, PR ChinaGaoyuan qixiang1000-05342023-02-0142113914910.7522/j.issn.1000-0534.2022.000271000-0534（2023）01-0139-11Analysis of Dual Polarization Characteristics of Turbulent Structure from Hail Supercell StormsJuxiu WU0Ming WEI1Xiuguang DIAO2Jiawen PAN3Key Laboratory for Meteorological Disaster Prevention and Mitigation of Shandong， Atmospheric Sounding Technology Support Center， Shandong Meteorological Burea， Jinan 250031， Shandong， ChinaCollaborative Innovation Center on Forecast and Evaluation of Meteorological Disasters， NUIST， Nanjing 210044， Jiangsu， ChinaShandong Meteorological Bureau， Jinan 250031， Shandong， ChinaXiamen Key Laboratory of Straits Meteorology， Xiamen Meteorological Bureau， Xiamen 361012， Fujian， China.Convective storms transmit momentum through turbulence， so it is important to understand the echo characteristics of turbulence structure in severe convective storms.Focusing on the velocity spectrum width above 5 m·s -1， the turbulent intensity of two strong hailstorm supercells with different intensity of mesocyclones are analyzed， and the relationship between airflow structure and turbulence enhancement are revealed.The results show that： （1） The strong hail supercell has moderate or above intensity turbulence in the strong updraft region， and the supercell triggered by the gust front also shows moderate intensity spectrum width in the inflow path， indicating the possibility of moderate intensity turbulence.（2） In general， the strongest turbulence occurs in the region with the largest velocity shear intensity.The maximum spectrum width of the supercell with moderate intensity mesocyclone is about 10 ms -1， with differential reflectivity factor （ ZDR） within 1dB， echo intensity exceeding 35 dBZ， and larger differential phase shift rate （ KDP）.The strong turbulence region of the supercell with strong mesocyclone is mainly located at the intersection of positive and negative velocities at the top of ZDR column， and the spectral width near the mesocyclone can reach 16.5 m·s -1， and the side near the strong echo core contains more supercooled water， with about 0.96 of correlation coefficient （CC） and large KDP.While， the echo intensity on the other side is slightly lower， with CC low to 0.85， where graupel particles and large raindrops brought by updraft exist.These regions of strong turbulence indicate the path of momentum transmission.（3） The upper part of the supercell storm has the strongest turbulence， both updrafts and downdrafts are strong， but the turbulence is stronger near the downdrafts that probably related to horizontal shear of the wind， where the highest spectrum width for strong mesocyclone is 17.5 m·s -1， and ZDR is higher than that in the updraft and KDP is negative， but KDP is about 0 （°）·km -1 and ZDR is about 0 dB in the updrafts， however， spectrum width of the storm with moderate mesocyclone increases slightly.Strong mesocyclone supercell has stronger turbulence enhancement， and these discussions provide a reference for understanding the turbulence structure and momentum transmission of severe storms by dual-polarization radar observation.http://www.gyqx.ac.cn/EN/10.7522/j.issn.1000-0534.2022.00027supercell stormspectrum widthturbulencedual polarization characteristics |
| spellingShingle | Juxiu WU Ming WEI Xiuguang DIAO Jiawen PAN Analysis of Dual Polarization Characteristics of Turbulent Structure from Hail Supercell Storms Gaoyuan qixiang supercell storm spectrum width turbulence dual polarization characteristics |
| title | Analysis of Dual Polarization Characteristics of Turbulent Structure from Hail Supercell Storms |
| title_full | Analysis of Dual Polarization Characteristics of Turbulent Structure from Hail Supercell Storms |
| title_fullStr | Analysis of Dual Polarization Characteristics of Turbulent Structure from Hail Supercell Storms |
| title_full_unstemmed | Analysis of Dual Polarization Characteristics of Turbulent Structure from Hail Supercell Storms |
| title_short | Analysis of Dual Polarization Characteristics of Turbulent Structure from Hail Supercell Storms |
| title_sort | analysis of dual polarization characteristics of turbulent structure from hail supercell storms |
| topic | supercell storm spectrum width turbulence dual polarization characteristics |
| url | http://www.gyqx.ac.cn/EN/10.7522/j.issn.1000-0534.2022.00027 |
| work_keys_str_mv | AT juxiuwu analysisofdualpolarizationcharacteristicsofturbulentstructurefromhailsupercellstorms AT mingwei analysisofdualpolarizationcharacteristicsofturbulentstructurefromhailsupercellstorms AT xiuguangdiao analysisofdualpolarizationcharacteristicsofturbulentstructurefromhailsupercellstorms AT jiawenpan analysisofdualpolarizationcharacteristicsofturbulentstructurefromhailsupercellstorms |