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Model studies of time-dependent ducting for high-frequency gravity waves and associated airglow responses in the upper atmosphere.

机译:高空大气中高频重力波的时间相关管道模型及相关气辉响应的模型研究。

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摘要

This doctoral dissertation has mainly concentrated on modeling studies of shorter period acoustic-gravity waves propagating in the upper atmosphere. Several cases have been investigated in the literature, which are focusing on the propagation characteristics of highfrequency gravity wave packets. The dissertation consists of five main divisions of which each has its own significance to be addressed, and these five chapters are also bridged in order with each other to present a theme about gravity wave ducting dynamics, energetics, and airglows.;The first chapter is served as an introduction of the general topic about atmospheric acoustic-gravity waves. Some of the historical backgrounds are provided as an interesting refreshment and also as a motivation reasoning this scientific research for decades. A new 2-D, time-dependent, and nonlinear model is introduced in the second chapter (the AGE-TIP model, acronymically named atmospheric gravity waves for the Earth plus tides and planetary waves). The model is developed during this entire doctoral study and has carried out almost all research results in this dissertation.;The third chapter is a model application for shorter period gravity waves ducted in a thermally stratified atmosphere. In spite of mean winds the thermal ducting occurs because ducted waves are fairly common occurrences in airglow observations. One-dimensional Fourier analysis is applied to identify the ducted wave modes that reside within multiple thermal ducts. Besides, the vertical energy flux and the wave kinetic energy density are derived as wave diagnostic variables to better understand the time-resolved vertical transport of wave energy in the presence of multiple thermal ductings.;The fourth chapter is also a model application for shorter period gravity waves, but it instead addresses the propagation of high-frequency gravity waves in the presence of mean background wind shears. The wind structure acts as a significant directional filter to the wave spectra and hence causes noticeable azimuthal variations at higher altitudes. In addition to the spectral analysis applied previously the wave action has been used to interpret the energy coupling between the waves and the mean flow among some atmospheric regions, where the waves are suspected to extract energy from the mean flow at some altitudes and release it to other altitudes.;The fifth chapter is a concrete and substantial step connecting theoretical studies and realistic observations through nonlinearly coupling wave dynamic model with airglow chemical reactions. Simulated O (1S) (557.7 nm) airglow images are provided so that they can be compared with observational airglow images. These simulated airglow brightness variations response accordingly with minor species density fluctuations, which are due to propagating and ducting nonlinear gravity waves within related airglow layers. The thermal and wind structures plus the seasonal and geographical variabilities could significantly influence the observed airglow images. By control modeling studies the simulations can be used to collate with concurrent observed data, so that the incoherencies among them could be very useful to discover unknown physical processes behind the observed wave scenes.
机译:该博士论文主要集中于在高层大气中传播的短期声重力波的建模研究。在文献中已经研究了几种情况,它们集中在高频重力波包的传播特性上。论文由五个主要部分组成,每个部分都有其自身的重要意义,并且这五个章节也相互衔接,以提出一个关于重力波导管动力学,能量学和气辉的主题。作为有关大气声重力波的一般主题的介绍。提供了一些历史背景,作为有趣的更新,并且也是数十年来进行这项科学研究的动机。在第二章中介绍了一个新的二维,时变和非线性模型(AGE-TIP模型,简称为地球重力,潮汐和行星波的大气重力波)。该模型是在整个博士研究过程中开发的,并完成了本论文的几乎所有研究成果。第三章是热分层大气中短周期引力波的模型应用。尽管风向平均,但发生热导管是因为在气辉观测中导管波是相当普遍的现象。一维傅里叶分析用于识别驻留在多个热导管中的导管波模式。此外,将垂直能量通量和波浪动能密度作为波浪诊断变量,以更好地理解存在多个热导管的情况下波浪能量在时间上的垂直传输。第四章也是短期内的模型应用重力波,但是它解决了在平均背景风切变的情况下高频重力波的传播。风的结构对波谱起着重要的方向性过滤器的作用,因此在较高的高度会引起明显的方位角变化。除了以前应用的频谱分析外,波浪作用还被用来解释波浪与某些大气区域之间的平均流之间的能量耦合,其中怀疑波浪在某些高度从平均流中提取能量并将其释放给第五章是一个具体而实质性的步骤,它通过波浪动力学模型与气辉化学反应的非线性耦合将理论研究和现实观察联系起来。提供了模拟的O(1S)(557.7 nm)气辉图像,以便可以将它们与观察到的气辉图像进行比较。这些模拟的气辉亮度变化相应地具有较小的物种密度波动,这是由于在相关的气辉层内传播和输送非线性重力波所致。热力和风的结构加上季节和地理的变化会极大地影响观测到的气辉图像。通过控制建模研究,可以将模拟与并发的观测数据进行核对,从而使它们之间的不相干性对于发现观测到的波场背后的未知物理过程非常有用。

著录项

  • 作者

    Yu, Yonghui.;

  • 作者单位

    University of Central Florida.;

  • 授予单位 University of Central Florida.;
  • 学科 Atmospheric Sciences.
  • 学位 Ph.D.
  • 年度 2007
  • 页码 138 p.
  • 总页数 138
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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