The Role of WISHE in the Rapid Intensification of Super Typhoon Hinnamnor (2022)

IF 3.8 2区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES
Hui Wang, Dajun Zhao, Hongxiong Xu, Qian Wang, Jia Liang, Tzu-Hsiung Yen
{"title":"The Role of WISHE in the Rapid Intensification of Super Typhoon Hinnamnor (2022)","authors":"Hui Wang,&nbsp;Dajun Zhao,&nbsp;Hongxiong Xu,&nbsp;Qian Wang,&nbsp;Jia Liang,&nbsp;Tzu-Hsiung Yen","doi":"10.1029/2024JD041864","DOIUrl":null,"url":null,"abstract":"<p>In this study, the role of the wind-induced surface heat exchange (WISHE) in rapid intensification (RI) is investigated in a numerical model. During the development of Hinnamnor, its energy growth rate (EGR) continuously increases as RI progresses. After Hinnamnor reaches its maximum intensity, although its EGR weakens a little, it remains relatively large. If it had not been for the influence of the external environment (such as the tropical depression), its maximum intensity would have been far greater than the actual maximum intensity (140 knots). As the WISHE effect progressively weakens, the number of convective bursts (CBs) gradually diminishes. This, in turn, gives rise to a corresponding weakening of the warm core and a subsequent delay in the start time of the axisymmetrization of the inner core, thereby affecting the intensification rate of the vortex and the final maximum intensity. Consequently, the start time of RI is also correspondingly postponed. Differing from the maximum potential intensity theory, when the EGR approaches zero, a TC does not immediately reach its maximum intensity. Instead, it attains its peak intensity approximately 12 hr later. During this additional 12 hr period, the number of CBs continues to increase, the warm core keeps on strengthening and the inner core continues its progress toward axisymmetric until the end of the RI process. This indicates that the dynamical and thermodynamical processes are also of great importance during the RI stage.</p>","PeriodicalId":15986,"journal":{"name":"Journal of Geophysical Research: Atmospheres","volume":"130 1","pages":""},"PeriodicalIF":3.8000,"publicationDate":"2024-12-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Geophysical Research: Atmospheres","FirstCategoryId":"89","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1029/2024JD041864","RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"METEOROLOGY & ATMOSPHERIC SCIENCES","Score":null,"Total":0}
引用次数: 0

Abstract

In this study, the role of the wind-induced surface heat exchange (WISHE) in rapid intensification (RI) is investigated in a numerical model. During the development of Hinnamnor, its energy growth rate (EGR) continuously increases as RI progresses. After Hinnamnor reaches its maximum intensity, although its EGR weakens a little, it remains relatively large. If it had not been for the influence of the external environment (such as the tropical depression), its maximum intensity would have been far greater than the actual maximum intensity (140 knots). As the WISHE effect progressively weakens, the number of convective bursts (CBs) gradually diminishes. This, in turn, gives rise to a corresponding weakening of the warm core and a subsequent delay in the start time of the axisymmetrization of the inner core, thereby affecting the intensification rate of the vortex and the final maximum intensity. Consequently, the start time of RI is also correspondingly postponed. Differing from the maximum potential intensity theory, when the EGR approaches zero, a TC does not immediately reach its maximum intensity. Instead, it attains its peak intensity approximately 12 hr later. During this additional 12 hr period, the number of CBs continues to increase, the warm core keeps on strengthening and the inner core continues its progress toward axisymmetric until the end of the RI process. This indicates that the dynamical and thermodynamical processes are also of great importance during the RI stage.

求助全文
约1分钟内获得全文 求助全文
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.
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信