与珠江三角洲极端小时降水有关的γ-中尺度涡旋特征观测分析

Observational analysis of the characteristics of meso-γ-scale vortexes associated with the extreme hourly precipitation in the Pearl River Delta region.

  • 摘要: 本研究建立了一套基于多普勒天气雷达观测资料的γ-中尺度涡旋(Meso-γ-scale Vortex;MV)客观识别算法,针对珠江三角洲地区稠密地面气象站五年暖季共237个极端小时降水(EXHP;>75mm )记录,统计分析与之有关的MV特征和环境大气动、热力参数,并选取EXHP站次最多的三次事件,展示MV与瞬时雨强、强回波的时空配置。主要发现:41.8%的EXHP记录有MV伴随;共57个MV,约84%属于弱切变(旋转速度<12 m/s)、12%为弱中气旋、4%为中等中气旋强度;MV平均持续时长约39分钟,平均核心厚度为699米,MV时长与核心厚度的相关系数为0.67。相对于美国伴随MV的EXHP,珠三角地区EXHP的环境0-3 km风暴相对螺旋度(SRH)和0-1km垂直风切变(VWS)较弱,但是,相对于珠三角地区无旋EXHP,有旋EXHP的环境具有显著较高的0-1km VWS和0-3km SRH,这为形成中涡旋提供了较好的环境动力条件,而有旋EXHP也倾向于发生在具有更充足的水汽和更高的对流有效位能的环境中,这为强降水对流系统提供了环境层结不稳定和水汽条件。EXHP站次最多的三次事件中,产生EXHP的对流系统形态差异大(分别呈现β-中尺度不规则形状、γ-中尺度准团状、β-中尺度准带状),MV常常位于对流系统内部强回波区域,许多MV在最强的回波核附近,有些MV紧邻强回波呈现弓形的部分;持续时间长、旋转相对较强的MV与极端强的6-min累积雨量(≥10 mm/6-min)的时空相关度很高,可能发生低层旋转与强降水的正反馈作用;在受到热带风暴影响的一次事件中,出现了三个MV相继在几乎相同的地点出现、并沿着几乎相同的路径移动的MV后建过程。

     

    Abstract: In this study, an objective algorithm to identify meso-γ-scale vortexes (MVs) using observations from a Doppler weather radar is built. Then, for the 237 Extreme Hourly Precipitation (EXHP; > 75 mm) records observed at the densely distributed surface weather stations in the Pearl River Delta (PRD) during five warm seasons, the associated MVs’ properties and environmental dynamic and thermodynamic parameters are statistically analyzed. Further, the three events with the most abundant EXHP records are analyzed to illustrate the spatiotemporal distributions of the MV, instantaneous rain rate, and strong radar echo. Major findings are as follows. About 41.8% of the EXHP records are accompanied with MVs. Of the total 57 MVs, about 84% are of weak shear intensity (rotational speed <12 m/s), 12% of weak mesocyclone intensity, and 4% of moderate mesocyclone intensity. The MVs have an average duration of about 39 minutes and an average core thickness of 699 meters, with the correlation coefficient of 0.67 between the duration and core thickness. Relative to the EXHP events with MVs in the United States, those in the PRD have smaller 0—3 km storm relative helicity (SRH) and 0—1 km vertical wind shear (VWS). However, compared to the EXHP without MVs in the PRD, the EXHP with MVs has significantly higher 0—1 km VWS and 0—3 km SRH, which provides better environmental dynamic conditions for the formation of MVs. Meanwhile, the EXHP with MV tend to occur in an environment with larger moisture amounts and higher convective available potential energy, which provides environmental instability and moisture conditions for strong convective systems.. In the three events with the largest (top 3) number of EXHP records, the EXHP-producing convective storms are featured with substantially different morphologies, i.e., a meso-β-scale irregular shape, a meso-γ-scale quasi-circular shape, and a meso-β-scale quasi-banded shape, respectively. The MVs are often located inside the strong radar reflectivity region, many of which are near the strongest echo core and some of which are next to the bow-shaped part of the strong echo. Those MVs that last longer and of relatively stronger rotation are highly correlated with the extreme 6-min rainfall accumulation (≥10 mm) in space and time, suggesting that the positive feedback between low-level rotation and short-term rain rate may be functioning. In the event influenced by a tropical storm, there was an MV back-building process in which three MVs appeared at almost the same location in succession and moved along roughly the same path.

     

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