Background wind effect on propagation of nonmigrating diurnal tides in the middle atmosphere

IF 1.9 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Journal of Atmospheric and Solar-Terrestrial Physics Pub Date : 1997-03-01 DOI:10.1016/S1364-6826(96)00012-0
E.M.P. Ekanayake , T. Aso , S. Miyahara
{"title":"Background wind effect on propagation of nonmigrating diurnal tides in the middle atmosphere","authors":"E.M.P. Ekanayake ,&nbsp;T. Aso ,&nbsp;S. Miyahara","doi":"10.1016/S1364-6826(96)00012-0","DOIUrl":null,"url":null,"abstract":"<div><p>The propagation characteristics of the nonmigrating diurnal tides are investigated numerically using a 2-dimensional (latitude-height) steady state model for a realistic atmosphere characterized by background mean zonal winds, meridional temperature gradients, mechanical and thermal dissipation, and tropospheric forcing obtained from a General Circulation Model. The mechanical and thermal dissipation is parameterized through eddy viscosity and conductivity, respectively, in addition to the molecular viscosity and conductivity.</p><p>It is found that the westward (eastward) propagating diurnal nonmigrating tides possess significant amplitudes compared to those of the migrating tide at upper mesospheric and lower thermospheric heights in the hemisphere where the westerlies (easterlies) are dominant. Hence, it is shown that the Doppler effect due to the presence of background mean zonal winds makes it possible for the diurnal nonmigrating tides of higher zonal wave numbers (both westward and eastward) to propagate up into the middle to high latitude regions of both hemispheres.</p></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":"59 4","pages":"Pages 401-429"},"PeriodicalIF":1.9000,"publicationDate":"1997-03-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/S1364-6826(96)00012-0","citationCount":"65","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Atmospheric and Solar-Terrestrial Physics","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S1364682696000120","RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
引用次数: 65

Abstract

The propagation characteristics of the nonmigrating diurnal tides are investigated numerically using a 2-dimensional (latitude-height) steady state model for a realistic atmosphere characterized by background mean zonal winds, meridional temperature gradients, mechanical and thermal dissipation, and tropospheric forcing obtained from a General Circulation Model. The mechanical and thermal dissipation is parameterized through eddy viscosity and conductivity, respectively, in addition to the molecular viscosity and conductivity.

It is found that the westward (eastward) propagating diurnal nonmigrating tides possess significant amplitudes compared to those of the migrating tide at upper mesospheric and lower thermospheric heights in the hemisphere where the westerlies (easterlies) are dominant. Hence, it is shown that the Doppler effect due to the presence of background mean zonal winds makes it possible for the diurnal nonmigrating tides of higher zonal wave numbers (both westward and eastward) to propagate up into the middle to high latitude regions of both hemispheres.

查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
背景风对中层大气非迁移日潮传播的影响
本文采用二维(纬度-高度)稳态模式对真实大气的非迁移日潮的传播特性进行了数值研究,该模式的特征包括背景平均纬向风、经向温度梯度、机械和热耗散以及一般环流模式的对流层强迫。除了分子粘度和电导率外,机械耗散和热耗散分别通过涡流粘度和电导率参数化。在西风带(东风)为主的半球,向西(向东)传播的日非迁移潮比中层上层和低层的迁移潮具有显著的振幅。因此,研究表明,由于背景平均纬向风的存在,多普勒效应使得高纬向波数(西向和东向)的日非迁移潮汐向上传播到两个半球的中纬度和高纬度地区成为可能。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 去求助
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.
期刊最新文献
Editorial Board Corrigendum to ‘Optimized fuzzy logic algorithm for classifying meteorological and non-meteorological echoes in CINRAD/SA data in Poyang lake region’ [J. Atmos. Sol. Terr. Phys., Volume 278, 2026, 106708] Degradation behavior of perovskite solar cells under high-intensity and multi band illumination conditions A simulation study on the key cloud microphysical processes in an extreme warm-sector heavy rainfall over the south China mountains Artificial Neural Network (ANN) modeling for CO2 concentration prediction in geothermal fields
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:604180095
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1