Height of warm core in very severe cyclonic storms Phailin: INSAT-3D perspective

S. Rani, V. S. Prasad, E. Rajagopal, S. Basu
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引用次数: 3

Abstract

Warm core is the characteristic that distinguishes tropical cyclones from its extra tropical counter parts, where the center of the cyclone is warmer than its environment. Two of the most common variables used to characterize the warm core are its strength and height. The strength is given by the magnitude of maximum perturbation temperature and the height is the level where the maximum perturbation temperature occurs. INSAT-3D, India's advanced weather satellite, is the first geostationary sounder over India and the surrounding Oceanic regions. INSAT-3D has 18 channel sounder with a resolution of 10 km to profile the atmospheric temperature and humidity. Brightness Temperatures (Tbs) from INSAT-3D sounder channels are used to analyze the warm core structure of Tropical cyclone Phailin (8–14 October 2013) over the North Indian Ocean. Only when the system becomes very severe cyclonic system, when the eye of the cyclone is clearer (fully cloud free), the sounder channel Tbs showed multiple maxima, with strong primary maximum in the middle level (600–500 mb) and the secondary maximum in the upper level (300–250 mb), unlike the conventional belief suggested warm core existence at 250 mb. Due to the high resolution of (10 km) INSAT-3D sounder channels, compared to the Micro wave channels (AMSU-A of 50 km resolution), the warm core structure below 10 km of the atmosphere is well resolved.
非常强烈气旋风暴的暖核高度:INSAT-3D透视
暖核是将热带气旋与其他热带气旋区分开来的特征,热带气旋的中心比其周围的环境更温暖。用来表征暖地核的两个最常见的变量是它的强度和高度。强度由最高扰动温度的大小给出,高度是最高扰动温度发生的水平。印度的先进气象卫星INSAT-3D是印度及其周边大洋地区的首个地球同步探测仪。INSAT-3D有18通道的测深仪,分辨率为10公里,可以探测大气温度和湿度。利用INSAT-3D探测通道的亮度温度(Tbs)对2013年10月8-14日热带气旋“菲林”在北印度洋上空的暖核结构进行了分析。只有当系统变成非常严重的气旋系统时,当气旋眼更加清晰(完全无云)时,声道Tbs才会出现多个极大值,其中强烈的初级极大值在中层(600-500 mb),次级极大值在上层(300-250 mb),而不是传统认为的250 mb存在暖核。由于(10 km) INSAT-3D声道的高分辨率,与50 km分辨率的微波声道(AMSU-A)相比,在大气层10千米以下的暖核结构得到了很好的解析。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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