Revealing Key Dynamical Mechanisms of a Severe Supercell Within a QLCS Using Rapid Update 4DVar Assimilation of C-Band Phased Array Weather Radar Data

IF 3.8 2区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES
Ruiting Liu, Jingya Wu, Mingxuan Chen, Rui Qin, Xian Xiao, Siteng Li, Lu Yang, Jianli Ma, Hongbo Zhang, Hao Huang, Lina Zhang
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Abstract

We investigate the evolution of a supercell storm within a quasi-linear convective system (QLCS) that occurred in the Beijing area on 12 June 2022. Using high spatiotemporal resolution observations from a C-band phased array radar (PAR), assimilated into a four-dimensional variational data assimilation system, we primarily analyze dynamical processes contributing to the development of the supercell storm and its associated mesocyclone. Our study shows that just before the convective cell is triggered, a significant convergence zone develops to the west of the terrain, forming several meso-γ vortices near the surface. During the merger of the convective cell and the QLCS from upper to lower levels, a strong downdraft generated by the QLCS enhances low-level horizontal convergence, further producing a stretching effect on the vortices within the storm and significantly increasing vertical vorticity. With the formation of the mesocyclone in the mature stage of supercell storm, the height of the rotational center rises to 4.5 km, and the maximum rotational velocity reaches 20 m/s. Our results indicate that the surface convergence lines and the meso-γ vortices along them strengthen low-level convergence and generate strong updrafts, triggering the initial storm. These intense updrafts transform horizontal vorticity into vertical vorticity and transport it upward. Additionally, the process of convective merging leads to strengthen low-level horizontal convergence, which forcibly stretches the mesovortex, enhancing vertical vorticity and allowing the convective storm to develop in a strong, organized manner and form the supercell storm.

Abstract Image

利用c波段相控阵天气雷达数据快速更新4DVar同化揭示QLCS中严重超级单体的关键动力机制
我们研究了2022年6月12日发生在北京地区的准线性对流系统(QLCS)中的超级单体风暴的演变过程。利用c波段相控阵雷达(PAR)的高时空分辨率观测资料,将其同化为四维变分资料同化系统,分析了超级单体风暴及其相关中气旋发展的动力过程。我们的研究表明,就在对流单体被触发之前,一个显著的辐合区在地形西部发展,在地表附近形成了几个中γ涡旋。在对流单体与QLCS自上而下合并过程中,QLCS产生的强下沉气流增强了低层水平辐合,进一步对风暴内部涡旋产生拉伸效应,垂直涡度显著增加。随着超级单体风暴成熟阶段中气旋的形成,旋转中心高度上升到4.5 km,最大旋转速度达到20 m/s。结果表明,地面辐合线及其上的中γ涡旋加强了低空辐合,并产生了强烈的上升气流,触发了最初的风暴。这些强烈的上升气流将水平涡度转化为垂直涡度并向上输送。此外,对流合并过程导致低层水平辐合增强,强拉伸中涡旋,使垂直涡度增强,使对流风暴强而有组织地发展,形成超级单体风暴。
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来源期刊
Journal of Geophysical Research: Atmospheres
Journal of Geophysical Research: Atmospheres Earth and Planetary Sciences-Geophysics
CiteScore
7.30
自引率
11.40%
发文量
684
期刊介绍: JGR: Atmospheres publishes articles that advance and improve understanding of atmospheric properties and processes, including the interaction of the atmosphere with other components of the Earth system.
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