Governing factors of the unprecedented extreme rainfall over Rameswaram Island

IF 2.2 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Meenakshi S, S. Sridharan
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引用次数: 0

Abstract

On 20-21 November 2024, extreme precipitation, the first of its kind to occur in the past 125 years, resulted in severe flooding across the southern coastal region of Tamil Nadu in particular over Rameswaram. The dynamic and thermodynamic conditions in the atmosphere that precede this extreme precipitation event are examined using reanalysis datasets of ERA5, brightness temperature, and Sea Surface Temperature. The analysis reveals deep convective clouds, a large amount of precipitable water, elevated specific humidity, and wind convergence in the lower troposphere at Rameswaram. The positive sea surface temperature (SST) anomaly of 2°C in the Bay of Bengal could lead to significant evaporation. Intense moisture is transported from the Bay of Bengal by easterly winds, and the westward-propagating tropical easterly waves facilitate the advection of positive PV anomalies towards Rameswaram. The presence of a cyclonic circulation progressing towards the southwest coast of the Indian Peninsula is evident in the moisture flux divergence. Convection was supported and sustained by enhanced upward vertical velocity between 850 and 200 hPa. Moreover, the positive potential vorticity (PV) tower extending from 850 hPa to 200 hPa, points to the development of dynamic instability. Vertical and horizontal PV dipoles, signatures of deep convection and instability, are also identified over Rameswaram during heavy rain. The time-height evolution of the divergence, vertical velocity (ω), and PV anomaly, along with the mid-level vortex, suggests that the 'top-down' dynamics can be responsible for the torrential downpour over Rameswaram.
Rameswaram岛史无前例的极端降雨的控制因素
2024年11月20日至21日,极端降水在过去125年来首次出现,导致泰米尔纳德邦南部沿海地区,特别是拉姆斯瓦拉姆地区发生严重洪灾。利用ERA5、亮度温度和海面温度的再分析数据集,研究了这次极端降水事件发生前的大气动力和热力学条件。分析显示Rameswaram对流层低层有较深的对流云、大量的可降水量、较高的比湿度和风辐合。孟加拉湾海温正异常(2°C)可能导致显著的蒸发。强烈的水汽由东风从孟加拉湾输送而来,向西传播的热带东风波促进正向PV异常向Rameswaram平流。在水汽通量辐散中,明显存在向印度半岛西南海岸推进的气旋环流。850 ~ 200 hPa之间的垂直上升速度增强支持和维持对流。正位涡(PV)塔从850 hPa延伸至200 hPa,预示着动力不稳定的发展。在暴雨期间,Rameswaram上空的垂直和水平PV偶极子,深层对流和不稳定的特征也被识别出来。辐散度、垂直速度(ω)、PV异常以及中层涡旋的时高演变表明,“自上而下”的动力可能是造成Rameswaram地区暴雨的原因。
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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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