利用卫星观测伊朗东南部热带气旋的结构

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Elham Ghasemifar , Somayeh Naserpour , Zahra Sonboli
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引用次数: 0

摘要

伊朗东南部易受源自北印度洋的热带气旋引发的山洪暴发的影响。在 2007 年至 2022 年的 5 月底至 9 月期间,共有 11 个气旋袭击了这一地区。虽然这些气旋的理论依据在文献中都有详细记载,但它们在降雨率、降雨类型、暖雨、云量和气溶胶分布等方面的物理结构还没有文献记载。本研究利用雷达(热带降雨测量任务(TRMM)、全球降水测量(GPM)和云卫星)、激光雷达(云-气溶胶激光雷达和红外探路卫星(CALIPSO))和光学(Aqua)卫星数据以及ERA5再分析数据集研究了11个气旋的结构。结果表明,最大的水汽输送和上升运动位于东南象限。因此,最大总雨量、层状雨量和对流雨量都落在这一象限。雨率的分布与暴雨顶部高度的分布一致。东南象限的暖雨最少,其次是东北象限。此外,东南象限也是对流云出现频率最高的象限。气溶胶光学深度的最大值位于南部象限,尤其是西南部,并在 5 千米范围内保持一致,之后最大值向西北部移动。所得结果可为水文和风险管理行业的决策者提供帮助。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Structure of tropical cyclones in the southeast Iran using satellite observations

The southeast Iran is exposed to flash floods from tropical cyclones originating in the North Indian Ocean. During late May–September of the period 2007–2022, 11 cyclones hit this region. Although the theoretical basis of these cyclones is well documented in the literature, their physical structure in terms of rain rate, rain type, warm rain, cloudiness, and aerosol distribution is not yet documented. In this study, the structure of 11 cyclones was investigated by the radar (Tropical Rainfall Measuring Mission (TRMM), Global Precipitation Measurement (GPM) and CloudSat), lidar (Cloud-Aerosol Lidar and Infrared Pathfinder Satellite (CALIPSO)), and optic (Aqua) satellite data and ERA5 reanalysis datasets. The results show that the maximum moisture transport and upward motion are located in the southeast quadrant. As a result, the maximum total rain rate, the stratiform and the convective rain rate fall in this quadrant. The distribution of the rain rate is consistent with the distribution of the storm top height. The southeast quadrant followed by the northeast receives the least warm rain. Moreover, the southeast quadrant also recorded the highest frequency of convective clouds. The maximum aerosol optical depth is located in the southern quadrants, particularly in the southwest and is consistent up to 5 km, after which the maximum shifts to the northwest. The obtained results can help decision makers within the hydrological and risk management industries.

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来源期刊
Journal of Atmospheric and Solar-Terrestrial Physics
Journal of Atmospheric and Solar-Terrestrial Physics 地学-地球化学与地球物理
CiteScore
4.10
自引率
5.30%
发文量
95
审稿时长
6 months
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.
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