首页 | 本学科首页   官方微博 | 高级检索  
     检索      

“莫兰蒂”台风致灾大风的结构特征及成因
引用本文:陈德花,张玲,张伟,赵玉春,蒋永成,郑辉.“莫兰蒂”台风致灾大风的结构特征及成因[J].大气科学学报,2018,41(5):692-701.
作者姓名:陈德花  张玲  张伟  赵玉春  蒋永成  郑辉
作者单位:厦门市气象局 海峡气象开放实验室, 福建 厦门 361012;厦门市气象局 海峡气象开放实验室, 福建 厦门 361012;厦门市气象局 海峡气象开放实验室, 福建 厦门 361012;厦门市气象局 海峡气象开放实验室, 福建 厦门 361012;厦门市气象局 海峡气象开放实验室, 福建 厦门 361012;厦门市气象局 海峡气象开放实验室, 福建 厦门 361012
基金项目:国家自然科学基金资助项目(41705045);福建省自然科学基金资助项目(2016J01182);厦门市科学技术局科技惠民项目(3502Z20164083);中国气象局预报员专项(CMAYBY2017-036);福建省气象局开放基金项目(2016K02);福建省强降水机理研究创新团队;厦门市气象局海洋精细化预报创新团队
摘    要:利用多种观测资料分析1614号"莫兰蒂"台风致灾大风的风场结构特征及成因。结果表明:"莫兰蒂"登陆前台风环流内的局地强风呈阶段性波动特征,局地强风相对台风方位角的变化随着台风靠近先顺转后逆转;基于台风风压关系的分析表明"莫兰蒂"强度估计与实测吻合;台风登陆后受地形摩擦影响,台风左侧的风速大于右侧;数值模拟分析表明在影响局地强风过程的主要物理因子中,风矢量的水平平流和气压梯度项的影响最重要;"莫兰蒂"台风的强风区呈现明显的中尺度特征,较高动量的空气垂直输送和动量下传作用导致眼壁周围风力增强。

关 键 词:“莫兰蒂”台风  致灾大风  风压关系  数值模拟
收稿时间:2018/2/3 0:00:00
修稿时间:2018/4/21 0:00:00

Structure characteristics and cause analysis of catastrophic wind caused by super typhoon Meranti
CHEN Dehu,ZHANG Ling,ZHANG Wei,ZHAO Yuchun,JIANG Yongcheng and ZHENG Hui.Structure characteristics and cause analysis of catastrophic wind caused by super typhoon Meranti[J].大气科学学报,2018,41(5):692-701.
Authors:CHEN Dehu  ZHANG Ling  ZHANG Wei  ZHAO Yuchun  JIANG Yongcheng and ZHENG Hui
Institution:Laboratory of Straits Meteorology, Xiamen Meteorological Bureau, Xiamen 361012, China;Laboratory of Straits Meteorology, Xiamen Meteorological Bureau, Xiamen 361012, China;Laboratory of Straits Meteorology, Xiamen Meteorological Bureau, Xiamen 361012, China;Laboratory of Straits Meteorology, Xiamen Meteorological Bureau, Xiamen 361012, China;Laboratory of Straits Meteorology, Xiamen Meteorological Bureau, Xiamen 361012, China;Laboratory of Straits Meteorology, Xiamen Meteorological Bureau, Xiamen 361012, China
Abstract:Based on the observed data and simulated results, this paper studies the structure characteristics and cause of catastrophic wind caused by super typhoon Meranti(typhoon "1614"). It is the strongest typhoon affecting Xiamen since typhoon "5903", and its impact radius is relatively small. Before landing, the local strong wind in typhoon circulation is characterized by periodic fluctuation. The azimuth change of the local strong wind relative to the typhoon first turns clockwise, then turns counterclockwise with the typhoon approaching. Simulated strength of typhoon Meranti based on the wind-pressure relation is in good agreement with the observed result. After landing, typhoon Meranti is affected by terrain friction, which makes the wind speed on the left side of typhoon stronger than that on the right side. Numerical simulation analysis shows that the horizontal advection of wind vector and the pressure gradient term are the main physical factors causing the local catastrophic wind. The strong wind area of typhoon Meranti shows obvious meso-scale characteristics. Wind around the eye wall is strengthened by the vertical air transportation with higher momentum and the momentum downward propagation effect.
Keywords:typhoon Meranti  catastrophic wind  wind-pressure relation  numerical simulation
本文献已被 CNKI 等数据库收录!
点击此处可从《大气科学学报》浏览原始摘要信息
点击此处可从《大气科学学报》下载免费的PDF全文
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号