北印度洋热带气旋热势与气旋强度的关系

B. Jangir, D. Swain, T. U. Udaya Bhaskar
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引用次数: 5

摘要

海洋热含量(OHC)在调节热带气旋(TC)强度方面发挥着重要作用。TC热势(TCHP)是热含量的估计值,因此被认为是TC发生和增强的有用指标。在本研究中,我们通过统计比较TCHP和气旋强度(CI),分析了TCHP在北印度洋(NIO) tc增强中的作用。利用印度国家海洋信息服务中心的全球海洋资料同化系统(GODAS)模式的chp资料和印度气象局的气旋最佳路径资料,对2005-2012年共27个TCs(孟加拉湾20个,阿拉伯海7个)进行了分析。在分析的27个气旋中,海湾(阿拉伯海)58%(86%)的气旋与CI和TCHP呈负相关,42%(14%)的气旋与TCHP呈正相关。总体上,超过60%的NIO气旋CI与TCHP呈负相关。TCHP领先CI 24小时和48小时的负百分比进一步增加。国家遥感中心的卫星TCHP数据和联合台风变暖中心的TCHP最佳轨迹数据也显示出类似的趋势。因此,我们认为除了海面温度之外,chp本身不一定是NIO中tc增强和传播的唯一重要海洋参数。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Relation between tropical cyclone heat potential and cyclone intensity in the North Indian Ocean
Ocean Heat Content (OHC) plays a significant role in modulating the intensity of Tropical Cyclones (TC) in terms of the oceanic energy available to TCs. TC Heat Potential (TCHP), an estimate of OHC, is thus known to be a useful indicator of TC genesis and intensification. In the present study, we analyze the role of TCHP in intensification of TCs in the North Indian Ocean (NIO) through statistical comparisons between TCHP and Cyclone Intensities (CI). A total of 27 TCs (20 in the Bay of Bengal, and 7 in the Arabian Sea) during the period 2005–2012 have been analyzed using TCHP data from Global Ocean Data Assimilation System (GODAS) model of Indian National Center for Ocean Information Services and cyclone best track data from India Meteorological Department. Out of the 27 cyclones analyzed, 58% (86%) in the Bay (Arabian Sea) have negative correlation and 42% (14%) cyclones have positive correlation between CI and TCHP. On the whole, more than 60% cyclones in the NIO show negative correlations between CI and TCHP. The negative percentage further increases for TCHP leading CI by 24 and 48 hours. Similar trend is also seen with satellite derived TCHP data obtained from National Remote Sensing Center and TC best track data from Joint Typhoon Warming Centre. Hence, it is postulated that TCHP alone need not be the only significant oceanographic parameter, apart from sea surface temperature, responsible for intensification and propagation of TCs in the NIO.
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