Raindrop size distribution characteristics of pre-monsoon precipitation observed over eastern India

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Journal of Atmospheric and Solar-Terrestrial Physics Pub Date : 2024-07-20 DOI:10.1016/j.jastp.2024.106315
Anuj Shrivastava , Balaji Kumar Seela , Bhishma Tyagi , Pay-Liam Lin
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Abstract

The knowledge of raindrop size distribution (DSD) is crucial for understanding the microphysical processes involved with the precipitation. Different empirical relationships established with DSD parameters, like radar reflectivity– rainfall rate (ZR) relationships and shape–slope (μɅ) relationships, can progress the rainfall estimation algorithms and cloud modeling simulations. In the present study, long-term (2018–2021) measurements of a Laser Precipitation Monitor (LPM) disdrometer installed at the National Institute of Technology, Rourkela, India is used to investigate the DSD characteristics of pre-monsoon (March–May) rainfall. Along with the disdrometer data, auxiliary parameters like convective available potential energy (CAPE), total column water vapor (TCWV), vertical profiles of temperature and relative humidity from reanalysis data sets of ECMWF (European Centre for Medium-Range Weather Forecasts) fifth-generation reanalysis (ERA5) are also used in this study. Based on standardized rainfall anomaly, the pre-monsoon precipitation days are classified into strong, moderate, and weak rainy days, and they contributed to 58.69%, 32.7%, and 8.61% of total rainfall, respectively. The average DSD indicated noteworthy variations among strong, moderate, and weak rainy days with maximum (minimum) concentration of raindrops in strong (weak) rainy days. The mean value of rain rate (R), normalized intercept parameter (Nw), and mass-weighted mean diameter (Dm) is maximum during days of strong rainfall. Strong rainy days showed high-value CAPE, TCWV and vertical profile of relative humidity. The majority of R is contributed by moderate-sized raindrops with a significant difference in the Z–R and μ–Λ relationships among three types of rainy days.

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在印度东部观测到的季风前降水的雨滴大小分布特征
雨滴粒径分布(DSD)知识对于了解降水的微物理过程至关重要。利用 DSD 参数建立的不同经验关系,如雷达反射率-降雨率(-)关系和形状-坡度(-)关系,可促进降雨估算算法和云建模模拟的发展。本研究利用安装在印度鲁尔凯拉国立技术学院的激光降水监测仪(LPM)测距仪的长期(2018-2021 年)测量数据,研究季风前(3 月至 5 月)降雨的 DSD 特性。除了测距仪数据外,本研究还使用了来自 ECMWF(欧洲中期天气预报中心)第五代再分析数据集(ERA5)的对流可用势能(CAPE)、总水汽柱(TCWV)、温度和相对湿度垂直剖面等辅助参数。根据标准化降雨异常,季风前期降水日被分为强降雨日、中雨日和弱雨日,它们分别占总降雨量的 58.69%、32.7% 和 8.61%。平均日降水量显示,强、中、弱雨日之间存在显著差异,强(弱)雨日的雨滴浓度最大(最小)。雨率()、归一化截距参数()和质量加权平均直径()的平均值在强降雨日最大。强降雨日的 CAPE 值、TCWV 值和相对湿度垂直剖面值都很高。大部分降雨是由中等大小的雨滴造成的,三种降雨日的降雨量和降雨量之间的关系存在显著差异。
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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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