{"title":"A Study of the Effects of the Ice-Microphysics, Surface Friction, and Surface Heat Flux on Tropical Cyclone Formation§","authors":"M. Yamasaki","doi":"10.2174/1874282301307010110","DOIUrl":null,"url":null,"abstract":"This paper describes results from numerical experiments which have been performed to understand the effects of the ice microphysics, surface friction, and surface heat flux on tropical cyclone (TC) formation. This study uses the author's non-hydrostatic model that intends to resolve cumulus convection. However, the horizontal grid size is taken to be somewhat large; 2 km in an area of 600 km x 600 km. A non-uniform coarse grid is used in the surrounding area with 4,000-km square. Several buoyancy perturbations arranged in the west-east direction, and a weak vortex with the maximum wind speed of 5 m s -1 are given at the initial time of the numerical time integrations. It is confirmed from two numerical experiments with and without ice microphysics that the development of a vortex is slower, and TC formation is delayed, in the presence of ice microphysics. It is also confirmed that a vortex can develop even without surface friction. It is shown that a strong vortex with the maximum wind speed of 20~25 m s -1 can be obtained. As expected, however, no eye forms, and further development does not occur. That is, it is confirmed that surface friction is indispensable to eye formation and a very strong TC having an eye. As for the third concern of this study, it is shown that a vortex with the maximum wind speed of about 5 m s -1 does not develop in the absence of the surface heat flux. That is, the surface heat flux plays an important role even in a weak vortex. Important backgrounds and understandings that are concerned with these results are described, based on studies on TCs in the past 50 years.","PeriodicalId":122982,"journal":{"name":"The Open Atmospheric Science Journal","volume":"798 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2013-12-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"The Open Atmospheric Science Journal","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.2174/1874282301307010110","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 1
Abstract
This paper describes results from numerical experiments which have been performed to understand the effects of the ice microphysics, surface friction, and surface heat flux on tropical cyclone (TC) formation. This study uses the author's non-hydrostatic model that intends to resolve cumulus convection. However, the horizontal grid size is taken to be somewhat large; 2 km in an area of 600 km x 600 km. A non-uniform coarse grid is used in the surrounding area with 4,000-km square. Several buoyancy perturbations arranged in the west-east direction, and a weak vortex with the maximum wind speed of 5 m s -1 are given at the initial time of the numerical time integrations. It is confirmed from two numerical experiments with and without ice microphysics that the development of a vortex is slower, and TC formation is delayed, in the presence of ice microphysics. It is also confirmed that a vortex can develop even without surface friction. It is shown that a strong vortex with the maximum wind speed of 20~25 m s -1 can be obtained. As expected, however, no eye forms, and further development does not occur. That is, it is confirmed that surface friction is indispensable to eye formation and a very strong TC having an eye. As for the third concern of this study, it is shown that a vortex with the maximum wind speed of about 5 m s -1 does not develop in the absence of the surface heat flux. That is, the surface heat flux plays an important role even in a weak vortex. Important backgrounds and understandings that are concerned with these results are described, based on studies on TCs in the past 50 years.
本文描述了为了解冰微物理、表面摩擦和表面热通量对热带气旋(TC)形成的影响而进行的数值实验结果。本研究采用作者的非流体静力模型来解析积云对流。然而,水平网格尺寸被认为有点大;2公里在600公里× 600公里的面积。周边面积4000平方公里,采用非均匀粗网格。在数值时间积分的初始时刻,有几个在东西方向排列的浮力扰动和一个最大风速为5 m s -1的弱涡旋。有冰微物理和没有冰微物理的两个数值实验证实,在冰微物理存在的情况下,涡的发展速度较慢,TC的形成延迟。也证实了即使没有表面摩擦也能形成涡。结果表明,在此条件下可形成最大风速为20~25 m s -1的强涡。然而,正如预期的那样,没有眼睛形成,进一步的发展也没有发生。也就是说,表面摩擦对于眼睛的形成是不可缺少的,一个非常强大的TC有一只眼睛。对于本研究的第三个问题,表明在没有地表热通量的情况下,最大风速约为5 m s -1的涡旋不会形成。即即使在弱涡旋中,地表热通量也起着重要的作用。本文根据近50年来对tc的研究,阐述了与这些结果有关的重要背景和认识。