{"title":"行星边界层方案对理想热带气旋最大潜在强度的影响","authors":"Chen Chen , Jiangnan Li","doi":"10.1016/j.jastp.2025.106603","DOIUrl":null,"url":null,"abstract":"<div><div>Tropical cyclones (TCs)' development relies on boundary layer processes. With climate change increasing extreme TCs, predicting their intensity under different planetary boundary layer (PBL) schemes is crucial. This study utilizes idealized TC experiments at cloud-resolving resolution within the Weather Research and Forecasting (WRF) model, employing PBL schemes of low-order or high-order closure, and local or nonlocal types, to investigate the impacts of these schemes on TC's maximum potential intensity (MPI).</div><div>The findings indicate that the MPI is remarkably sensitive to the choice of PBL schemes, with disparities in simulated MPI reaching up to 67 hPa. While schemes with different closure methods often compute turbulent diffusion coefficients differently, some, like YSU and MYNN3, simulate similar MPI due to shared low boundary layer heights (PBLH) and efficient latent heat utilization. Conversely, schemes with similar diffusion coefficient definitions, such as MYNN3 and BouLac, can produce differing MPI due to variations in mixing mechanisms.</div><div>Analysis of strong versus weak TC simulations reveals that strong TCs have lower boundary layer heights and turbulent diffusion coefficient peaks further from the surface, leading to greater near-surface gradient wind imbalance and stronger radial inflow. Weak TCs, on the other hand, have higher boundary layer heights and peaks closer to the surface, resulting in weaker inflow. Stronger inflow in strong TCs promotes moisture convergence in the core region, enhancing inner-core diabatic heating and forming a pronounced upper-level warm core, which accelerates TC intensification. The study highlights how PBL schemes significantly affect TC MPI by linking dynamic and thermodynamic processes.</div></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":"274 ","pages":"Article 106603"},"PeriodicalIF":1.9000,"publicationDate":"2025-08-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"The impacts of planetary boundary layer schemes on maximum potential intensity of idealized tropical cyclone\",\"authors\":\"Chen Chen , Jiangnan Li\",\"doi\":\"10.1016/j.jastp.2025.106603\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div>Tropical cyclones (TCs)' development relies on boundary layer processes. With climate change increasing extreme TCs, predicting their intensity under different planetary boundary layer (PBL) schemes is crucial. This study utilizes idealized TC experiments at cloud-resolving resolution within the Weather Research and Forecasting (WRF) model, employing PBL schemes of low-order or high-order closure, and local or nonlocal types, to investigate the impacts of these schemes on TC's maximum potential intensity (MPI).</div><div>The findings indicate that the MPI is remarkably sensitive to the choice of PBL schemes, with disparities in simulated MPI reaching up to 67 hPa. While schemes with different closure methods often compute turbulent diffusion coefficients differently, some, like YSU and MYNN3, simulate similar MPI due to shared low boundary layer heights (PBLH) and efficient latent heat utilization. Conversely, schemes with similar diffusion coefficient definitions, such as MYNN3 and BouLac, can produce differing MPI due to variations in mixing mechanisms.</div><div>Analysis of strong versus weak TC simulations reveals that strong TCs have lower boundary layer heights and turbulent diffusion coefficient peaks further from the surface, leading to greater near-surface gradient wind imbalance and stronger radial inflow. Weak TCs, on the other hand, have higher boundary layer heights and peaks closer to the surface, resulting in weaker inflow. Stronger inflow in strong TCs promotes moisture convergence in the core region, enhancing inner-core diabatic heating and forming a pronounced upper-level warm core, which accelerates TC intensification. The study highlights how PBL schemes significantly affect TC MPI by linking dynamic and thermodynamic processes.</div></div>\",\"PeriodicalId\":15096,\"journal\":{\"name\":\"Journal of Atmospheric and Solar-Terrestrial Physics\",\"volume\":\"274 \",\"pages\":\"Article 106603\"},\"PeriodicalIF\":1.9000,\"publicationDate\":\"2025-08-05\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of Atmospheric and Solar-Terrestrial Physics\",\"FirstCategoryId\":\"89\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S1364682625001877\",\"RegionNum\":4,\"RegionCategory\":\"地球科学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"GEOCHEMISTRY & GEOPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Atmospheric and Solar-Terrestrial Physics","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S1364682625001877","RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
The impacts of planetary boundary layer schemes on maximum potential intensity of idealized tropical cyclone
Tropical cyclones (TCs)' development relies on boundary layer processes. With climate change increasing extreme TCs, predicting their intensity under different planetary boundary layer (PBL) schemes is crucial. This study utilizes idealized TC experiments at cloud-resolving resolution within the Weather Research and Forecasting (WRF) model, employing PBL schemes of low-order or high-order closure, and local or nonlocal types, to investigate the impacts of these schemes on TC's maximum potential intensity (MPI).
The findings indicate that the MPI is remarkably sensitive to the choice of PBL schemes, with disparities in simulated MPI reaching up to 67 hPa. While schemes with different closure methods often compute turbulent diffusion coefficients differently, some, like YSU and MYNN3, simulate similar MPI due to shared low boundary layer heights (PBLH) and efficient latent heat utilization. Conversely, schemes with similar diffusion coefficient definitions, such as MYNN3 and BouLac, can produce differing MPI due to variations in mixing mechanisms.
Analysis of strong versus weak TC simulations reveals that strong TCs have lower boundary layer heights and turbulent diffusion coefficient peaks further from the surface, leading to greater near-surface gradient wind imbalance and stronger radial inflow. Weak TCs, on the other hand, have higher boundary layer heights and peaks closer to the surface, resulting in weaker inflow. Stronger inflow in strong TCs promotes moisture convergence in the core region, enhancing inner-core diabatic heating and forming a pronounced upper-level warm core, which accelerates TC intensification. The study highlights how PBL schemes significantly affect TC MPI by linking dynamic and thermodynamic processes.
期刊介绍:
The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them.
The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions.
Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.