Inter-seasonal variation of rainfall microphysics as observed over New Delhi, India

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Journal of Atmospheric and Solar-Terrestrial Physics Pub Date : 2024-08-22 DOI:10.1016/j.jastp.2024.106333
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Abstract

This study analyzes the raindrop size distribution (RSD) characteristics over New Delhi by dividing the year into three seasons: PreM (March–May), monsoon (June–September), and PostM (October–February). Data from a Joss-Waldvogel Disdrometer, installed at IITM New Delhi, Rajendra Nagar, was used for three years (2021–2023). The observed raindrop spectra were fitted with three-parameter Gamma functions to obtain the RSD. ERA-5 and satellite data were also employed to establish atmospheric and cloud properties for the three seasons. The RSD for the monsoon season shows the highest concentration of midsize (1–3 mm diameter) drops and the highest mean rain rate. PostM has the least concentration of midsize and large (diameter >3 mm) drops. General statistics of rain integral parameters reveal high variability in rain rate (R) and mass-weighted mean diameter (Dm) values during the monsoon season. The mu-lambda scatter plots show considerable differences among the three seasons, indicating slightly distinct rainfall mechanisms in the three seasons. Z-R relations of the form Z = aRb were derived, with the highest coefficient (a) values observed for the PreM precipitation. The exponent (b) is found to be greater than unity in all three seasons. Rainfall was stratified based on rain rate. RSD gets broader with increasing R. Large drops are not found appreciably in the spectrum for R < 20 mm/h. A notable disparity between convective and stratiform RSD is evident. The values of rain integral parameters show considerable differences between the convective and stratiform regimes. A higher fraction of large drops is found for the stratiform rainfall in the PreM season compared to the other two seasons. CAPE, water vapor, surface temperature, and surface winds were higher during PreM and monsoon months compared to PostM. The distribution of differential temperature (δT) indicates that clouds with significant depth are found in PreM and monsoon seasons but are often lacking during PostM.

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在印度新德里上空观测到的降雨微物理的季节间变化
本研究将一年分为三个季节,分析了新德里上空的雨滴大小分布 (RSD) 特征:季前(3 月至 5 月)、季风(6 月至 9 月)和季后(10 月至 2 月)。数据来自安装在 Rajendra Nagar 新德里国际理工学院的 Joss-Waldvogel 测距仪,时间为三年(2021-2023 年)。观测到的雨滴光谱用三参数伽马函数拟合,以获得 RSD。ERA-5和卫星数据也用于确定三个季节的大气和云层属性。季风季节的 RSD 显示中型(直径 1-3 毫米)雨滴的浓度最高,平均降雨率也最高。后季风季的中型和大型(直径 3 毫米)雨滴最少。雨量积分参数的一般统计显示,季风季节的雨量(R)和质量加权平均直径(Dm)值变化很大。亩-λ散点图显示三个季节之间存在很大差异,表明三个季节的降雨机制略有不同。得出了 Z = aRb 形式的 Z-R 关系,其中预雨季降水的系数(a)值最高。三个季节的指数(b)均大于 1。根据降雨率对降雨进行了分层。在 R < 20 mm/h 的频谱中没有发现明显的大滴。对流和分层 RSD 之间存在明显差异。雨积分参数值在对流和平流状态下显示出相当大的差异。与其他两个季节相比,PreM 季节的层状降雨中大滴的比例更高。与后季风季节相比,前季风季节和季风季节的 CAPE、水汽、地表温度和地表风都更高。温差分布(δT)表明,在气象预报季节和季风季节会出现深度较大的云层,但在气象预报季节后往往缺乏云层。
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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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