Contrasting features of rainfall microphysics as observed over the coastal and orographic region of western ghat in the inter-seasonal time-scale

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Journal of Atmospheric and Solar-Terrestrial Physics Pub Date : 2024-03-29 DOI:10.1016/j.jastp.2024.106221
Kaustav Chakravarty , Rohit P. Patil , Gargi Rakshit , G. Pandithurai
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Abstract

The paper aims to highlight the contrasting inter-seasonal variability of raindrop size distribution (DSD) as observed over Mumbai (representing a coastal city) and Mahabaleshwar (representing an orographic station in the Western Ghat mountain range) of Indian peninsula for a continuous period of four years (2018–2022). Upon examining the microphysical features of precipitation patterns, it is observed that raindrops with diameter of 3 mm and above dominate the rainfall in Mahabaleshwar during the pre-monsoon period, while the same with diameter of 1.5 mm and above dominate Mumbai's rainfall during the monsoon months. Additionally, the study finds a strong diurnal variation in rainfall occurrences during the pre-monsoon period for both the stations, while such variation is absent during the monsoon period. The analysis suggests that the Convective Available Potential Energy (CAPE) plays a significant role in these divergent diurnal patterns. Furthermore, the paper explores the relationship between mass-weighted mean diameter (Dm) - rain rate (R) values and shape (μ) versus slope (Λ) parameters as obtained from the two stations during the inter-seasonal phases of the monsoon. The results indicate that, during the pre-monsoon period, higher rain intensities (>16 mm/h) correspond to a dominant Dm value in Mahabaleshwar's rainfall. Conversely, during the monsoon months, higher Dm values are noticeable in Mumbai's rainfall. Thus by connecting with all the analysis done through this paper, it can be said that convective rainfall dominates the pre-monsoon period over orographic station, with convectivity becoming evident at rain rates greater than 16 mm/h. On the other hand, during the monsoon period, local thermodynamic conditions and higher moisture availability trigger the formation of deep convective clouds over coastal areas, thereby resulting for more convective rainfall in the coastal city compared to the orographic station.

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在西加特沿海和高原地区观测到的降雨微物理在跨季节时间尺度上的对比特征
本文旨在强调在印度半岛的孟买(代表沿海城市)和马哈巴莱什瓦尔(代表西高特山脉的一个地貌站)连续四年(2018-2022 年)观测到的雨滴大小分布(DSD)的季节间变化对比。在对降水模式的微物理特征进行研究后发现,直径为 3 毫米及以上的雨滴在马哈巴莱什瓦尔季风前期的降雨中占主导地位,而直径为 1.5 毫米及以上的雨滴则在孟买季风月份的降雨中占主导地位。此外,研究还发现,在季风前期,两个站点的降雨量都有很强的昼夜变化,而在季风期则没有这种变化。分析表明,对流可用势能(CAPE)在这些不同的昼夜模式中发挥了重要作用。此外,本文还探讨了季风季节间阶段从两个站点获得的质量加权平均直径(Dm)-降雨率(R)值和形状(μ)与斜率(Λ)参数之间的关系。结果表明,在季风前期,较高的降雨强度(>16 毫米/小时)对应于马哈巴莱什瓦尔降雨的主要 Dm 值。相反,在季风月份,孟买降雨的 Dm 值较高。因此,结合本文所做的所有分析,可以说对流降雨在季风前期的地貌站中占主导地位,当降雨率大于 16 毫米/小时时,对流降雨变得明显。另一方面,在季风期,当地的热力学条件和较高的水汽供应量会在沿海地区形成深层对流云,从而导致沿海城市的对流降雨量多于地形站。
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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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