{"title":"Comparative analysis of thermal structure in the activities of Southwest China vortexes","authors":"Yongren Chen , Yueqing Li","doi":"10.1016/j.jastp.2026.106746","DOIUrl":null,"url":null,"abstract":"<div><div>The Southwest China vortex (SWCV) is an important weather system that affects warm-season rainfall in China, but forecasting its path of activity remains difficult. In this study, we chose six historical cases to analyze the thermodynamic differences between the less-moving pattern (LMP) and the moving pattern (MP) of SWCV activity, the principal results were as follows. (1) Regardless of whether the SWCV moved, an approximate “dipole pattern” of cold–warm advection was evident in the vortex circulation. Generally, dry–cold advection was found in the northeasterly airflow of the SWCV circulation, and wet–warm advection occurred in the southwesterly airflow. (2) In the LMP, the range of dry–cold advection was smaller than that of wet–warm advection in the horizontal direction. In the MP, the range of dry–cold advection at the rear of the SWCV along the direction of motion expanded and promoted movement of the SWCV. In the vertical direction, the front of the SWCV was always characterized by wet–warm advection, and the rear was characterized by dry–cold advection under eastward movement of the MP, but such a feature was not obvious in the LMP. To a certain extent, the approximate dipole pattern of cold–warm advection in the horizontal direction facilitates the maintenance of a complete cyclonic circulation, but it also supports SWCV movement when the dry–cold advection expands and becomes deeper in the vertical direction. Based on these findings, we tried to define a thermodynamic index for determining SWCV movement.</div></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":"280 ","pages":"Article 106746"},"PeriodicalIF":2.2000,"publicationDate":"2026-03-01","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/S1364682626000301","RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"2026/2/5 0:00:00","PubModel":"Epub","JCR":"Q3","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
The Southwest China vortex (SWCV) is an important weather system that affects warm-season rainfall in China, but forecasting its path of activity remains difficult. In this study, we chose six historical cases to analyze the thermodynamic differences between the less-moving pattern (LMP) and the moving pattern (MP) of SWCV activity, the principal results were as follows. (1) Regardless of whether the SWCV moved, an approximate “dipole pattern” of cold–warm advection was evident in the vortex circulation. Generally, dry–cold advection was found in the northeasterly airflow of the SWCV circulation, and wet–warm advection occurred in the southwesterly airflow. (2) In the LMP, the range of dry–cold advection was smaller than that of wet–warm advection in the horizontal direction. In the MP, the range of dry–cold advection at the rear of the SWCV along the direction of motion expanded and promoted movement of the SWCV. In the vertical direction, the front of the SWCV was always characterized by wet–warm advection, and the rear was characterized by dry–cold advection under eastward movement of the MP, but such a feature was not obvious in the LMP. To a certain extent, the approximate dipole pattern of cold–warm advection in the horizontal direction facilitates the maintenance of a complete cyclonic circulation, but it also supports SWCV movement when the dry–cold advection expands and becomes deeper in the vertical direction. Based on these findings, we tried to define a thermodynamic index for determining SWCV movement.
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.