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Effects of background winds and temperature on bores, strong wind shears and concentric gravity waves in the mesopause region.

机译:背景风和温度对更年期区域的钻孔,强风切变和同心重力波的影响。

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摘要

Using data from the CSU sodium lidar and Kyoto University OH airglow imager at Fort Collins, CO, this thesis provides a comprehensive, though qualitative, understanding for three different yet related observed fluid-dynamical phenomena in the mesopause region.;The first project involves the convection-excited gravity waves observed in the OH airglow layer at 87 km. Case study on May 11, 2004 is discussed in detail along with statistical studies and a ray-tracing modeling. A single convection source matches the center of the concentric gravity waves. The horizontal wavelengths and periods of these gravity waves were measured as functions of both radius and time. The weak mean background wind between the lower and middle atmosphere determines the penetration of the gravity waves into higher altitude.;The second project involves mesospheric bores observed by the same OH imager. The observation on October 9, 2007 suggests that when a large-amplitude gravity wave is trapped in a thermal duct, its wave front could steepen and forms bore-like structure in the mesopause. In turn, the large gravity wave and its bore may significantly impact the background. Statistical study reveals the possible link between the jet/front system in the lower atmosphere and the large-scale gravity waves and associated bores in the mesopause region.;The third project involves the relationship between large wind shear generation and sustainment and convective/dynamic stabilities measured by the sodium lidar at the altitude of 80--105 km during 2002--2005. The correlation between wind shear, S, and Brunt-Vaisala frequency, N suggests that the maximum sustainable wind shear is determined by the necessary condition for dynamic instability of Richardson number, leading to the result that the maximal wind shear occurs at altitudes of lower thermosphere where the atmosphere is convectively very stable. The dominate source for sustainable large windshears appears to be the semidiurnal tidal-period perturbations with shorter vertical wavelengths and greater amplitude.
机译:利用CSU钠激光雷达数据和位于科罗拉多州柯林斯堡的京都大学OH气辉成像仪的数据,本论文对中绝经区三种不同但相关的流体动力学现象提供了全面但定性的理解。对流激发的重力波在OH气辉层的87 km处观测到。我们将详细讨论2004年5月11日的案例研究,以及统计研究和光线跟踪建模。单个对流源与同心重力波的中心匹配。测量这些重力波的水平波长和周期是半径和时间的函数。低层和中层大气之间的弱平均背景风决定了重力波向高空的渗透。第二个项目涉及同一OH成像仪观测到的中层孔。 2007年10月9日的观测结果表明,当大振幅重力波被困在热导管中时,其波前可能变陡并在中绝经期形成孔状结构。反过来,大的重力波及其孔径可能会严重影响背景。统计研究揭示了低层大气中的射流/前部系统与更年期区域中的大重力波和相关孔之间的可能联系。第三项研究涉及大风切变的产生与维持与对流/动力稳定性之间的关系。在2002--2005年期间由钠激光雷达在80--105 km的高度进行测量。风切变S和布鲁特-维萨拉频率N之间的相关性表明,最大可持续风切变由Richardson数动态不稳定性的必要条件决定,从而导致最大风切变发生在低热圈高度对流非常稳定的地方可持续的大风切变的主要来源似乎是半日潮汐扰动,其垂直波长较短,振幅较大。

著录项

  • 作者

    Yue, Jia.;

  • 作者单位

    Colorado State University.;

  • 授予单位 Colorado State University.;
  • 学科 Engineering Electronics and Electrical.;Atmospheric Sciences.
  • 学位 Ph.D.
  • 年度 2009
  • 页码 151 p.
  • 总页数 151
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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