Remote measurement of cloud microphysics and its influence in predicting high impact weather events

Paul Shukla Bipasha, John Jinya
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Abstract

Understanding the cloud microphysical processes and precise retrieval of parameters governing the same are crucial for weather and climate prediction. Advanced remote sensing sensors and techniques offer an opportunity for monitoring micro-level developments in cloud structure. . Using the observations from a visible and near-infrared lidar onboard CALIPSO satellite (part of A-train) , the spatial variation of cloud structure has been studied over the Tropical monsoon region . It is found that there is large variability in the cloud microphysical parameters manifesting in distinct precipitation regimes. In particular, the severe storms over this region are driven by processes which range from the synoptic to the microphysical scale. Using INSAT-3D data, retrieval of cloud microphysical parameters like effective radius (CER) and optical depth (COD) were carried out for tropical cyclone Phailine. It was observed that there is a general increase of CER in a top–down direction, characterizing the progressively increasing number and size of precipitation hydrometeors while approaching the cloud base. The distribution of CER relative to cloud top temperature for growing convective clouds has been investigated to reveal the evolution of the particles composing the clouds. It is seen that the relatively high concentration of large particles in the downdraft zone is closely related to the precipitation efficiency of the system. Similar study was also carried using MODIS observations for cyclones over Indian Ocean (2010-2013), in which we find that that the mean effective radius is 24 microns with standard deviation 4.56, mean optical depth is 21 with standard deviation 13.98, mean cloud fraction is 0.92 with standard deviation 0.13 and mainly ice phase is dominant. Thus the remote observations of microstructure of convective storms provide very crucial information about the maintenance and potential devastation likely to be associated with it. With the synergistic observations from A-Train , geostationary and futuristic imaging spectroscopic sensors, a multi-dimensional, and multi-scalar exploration of cloud systems is anticipated leading to accurate prediction of high impact weather events.
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云微物理的远程测量及其在预测高影响天气事件中的影响
了解云的微物理过程和精确检索控制这些过程的参数对天气和气候预测至关重要。先进的遥感传感器和技术为监测云结构的微观发展提供了机会。利用CALIPSO卫星(a -train的一部分)的可见光和近红外激光雷达观测资料,研究了热带季风区云结构的空间变化。研究发现,在不同的降水条件下,云微物理参数有很大的变异性。特别是,该地区的强风暴是由天气尺度到微物理尺度的过程驱动的。利用INSAT-3D数据反演了热带气旋“菲琳”的有效半径(CER)和光学深度(COD)等云微物理参数。观测到,CER总体呈自上而下的增加趋势,表现为降水水成物的数量和大小在接近云底时逐渐增加。研究了成长中的对流云的CER相对于云顶温度的分布,以揭示构成云的粒子的演变。可见,下沉气流区较大颗粒浓度的高低与系统的降水效率密切相关。2010-2013年印度洋气旋的MODIS观测结果表明,平均有效半径为24 μ m,标准差为4.56,平均光学深度为21,标准差为13.98,平均云分率为0.92,标准差为0.13,以冰相为主。因此,对对流风暴微观结构的远程观测提供了与之相关的维持和潜在破坏的非常重要的信息。借助a - train、地球静止和未来成像光谱传感器的协同观测,预计将对云系统进行多维、多标量的探索,从而准确预测高影响天气事件。
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