On the Optimal Initial Inner-Core Size for Tropical Cyclone Intensification: An Idealized Numerical Study

IF 6.5 2区 地球科学 Q1 METEOROLOGY & ATMOSPHERIC SCIENCES Advances in Atmospheric Sciences Pub Date : 2024-09-07 DOI:10.1007/s00376-024-3296-6
Rong Fei, Yuqing Wang
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Abstract

Recent observational and numerical studies have revealed the dependence of the intensification rate on the inner-core size of tropical cyclones (TCs). In this study, with the initial inner-core size (i.e., the radius of maximum wind—RMW) varied from 20–180 km in idealized simulations using two different numerical models, we found a nonmonotonic dependence of the lifetime maximum intensification rate (LMIR) on the inner-core size. Namely, there is an optimal inner-core size for the LMIR of a TC. Tangential wind budget analysis shows that, compared to large TCs, small TCs have large inward flux of absolute vorticity due to large absolute vorticity inside the RMW. However, small TCs also suffer from strong lateral diffusion across the eyewall, which partly offsets the positive contribution from large inward flux of absolute vorticity. These two competing processes ultimately lead to the TC with an intermediate initial inner-core size having the largest LMIR. Results from sensitivity experiments show that the optimal size varies in the range of 40–120 km and increases with higher sea surface temperature, lower latitude, larger horizontal mixing length, and weaker initial TC intensity. The 40–120 km RMW corresponds to the inner-core size most commonly found for intensifying TCs in observations, suggesting the natural selection of initial TC size for intensification. This study highlights the importance of accurate representation of TC inner-core size to TC intensity forecasts by numerical weather prediction models.

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关于热带气旋加强的最佳初始内核大小:理想化数值研究
最近的观测和数值研究揭示了热带气旋(TC)的加强率与内核大小的关系。在这项研究中,我们使用两种不同的数值模式进行理想化模拟,初始内核大小(即最大风半径)在 20-180 公里之间变化,结果发现终生最大增强率(LMIR)与内核大小存在非单调依赖关系。也就是说,热气旋的最大增强率存在一个最佳内核尺寸。切向风预算分析表明,与大型 TC 相比,小型 TC 由于 RMW 内部的绝对涡度较大,因此绝对涡度内流较大。然而,小型热气旋也受到眼球横向扩散的影响,这部分抵消了绝对涡度大量内流的正贡献。这两个相互竞争的过程最终导致具有中等初始内核尺寸的热气旋具有最大的 LMIR。敏感性实验结果表明,最佳尺寸在 40-120 公里范围内变化,并随海面温度升高、纬度降低、水平混合长度增大和初始 TC 强度减弱而增大。40-120 km RMW 与观测资料中最常见的增强型热气旋的内核大小一致,这表明初始热气旋大小是自然选择的。这项研究强调了数值天气预报模式准确表示热气旋内核尺寸对热气旋强度预报的重要性。
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来源期刊
Advances in Atmospheric Sciences
Advances in Atmospheric Sciences 地学-气象与大气科学
CiteScore
9.30
自引率
5.20%
发文量
154
审稿时长
6 months
期刊介绍: Advances in Atmospheric Sciences, launched in 1984, aims to rapidly publish original scientific papers on the dynamics, physics and chemistry of the atmosphere and ocean. It covers the latest achievements and developments in the atmospheric sciences, including marine meteorology and meteorology-associated geophysics, as well as the theoretical and practical aspects of these disciplines. Papers on weather systems, numerical weather prediction, climate dynamics and variability, satellite meteorology, remote sensing, air chemistry and the boundary layer, clouds and weather modification, can be found in the journal. Papers describing the application of new mathematics or new instruments are also collected here.
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