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Exploration of the mystery of polar wave dynamics with lidar/radar observations and general circulation models & development of new wave analysis methods.

机译:利用激光雷达/雷达观测和一般环流模型探索极波动力学的奥秘,并开发新的波分析方法。

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摘要

The Space-atmosphere interaction region (SAIR) between ~50 and 200 km is one of the key factors enabling our Earth to harbor life. Its fundamental processes are believed to be universal and applicable to the atmospheres of Earth-like planets throughout our galaxy. However, the SAIR remains one of the least observed and understood regions. This thesis aims to advance the observations and characterizations of atmospheric waves that are fundamental to shaping the SAIR, especially exploring the mystery of persistent inertia-gravity waves, discovered by our Fe Boltzmann lidar measurements of temperatures at McMurdo (77.8°S, 166.7°E), Antarctica.;This thesis discovers a new wave phenomenon in the Antarctic middle and upper atmosphere, namely the persistent inertia-gravity waves with periods of 3--10 h. This group of large-amplitude waves dominates the temperature perturbations from the stratosphere to the lower thermosphere (about 30--115 km). They occur so frequently as to appear endless and uninterrupted, impacting the composition, chemistry and thermodynamics of the SAIR. This thesis reports the first simultaneous lidar/radar observations of inertia-gravity waves in Antarctica. Utilizing the lidar data in June from 2011 to 2015, this thesis characterizes the persistent gravity wave properties for the first time. These waves exhibit a uniform dominant vertical wavelength of 20--30 km across periods of 3.5--10 h and vertical phase speeds of 0.8--2 m/s. They possess more than half of the spectral energy for ~93% of the time. An analysis of the 65-h lidar data on 28--30 June 2014 demonstrates multiple wave packets spanning as long as 60 h. Further analysis of May and July data confirms the persistency and dominancy of these waves but reveal a month-to-month variability.;This thesis develops a system of wave analysis methods, including extracting gravity waves from ~30--155 km in the neutral atmosphere for the first time. Our methodologies also include the temporal hodograph methods for simultaneous lidar/radar data; improved 1-D Morlet wavelet transform methods; rigorous pre-whitening and post-coloring spectral analysis techniques; and automated 2-D Morlet wavelet analysis and synthesis methods. Successful application of these methodologies provides new insights into gravity waves, their sources and impacts on the whole atmosphere and space.
机译:大约50至200公里之间的空间-大气相互作用区域(SAIR)是使我们的地球拥有生命的关键因素之一。它的基本过程被认为是普遍的,并且适用于整个银河系中类似地球的行星的大气层。但是,SAIR仍然是最少被观察和了解的区域之一。本论文旨在推进对形成SAIR至关重要的大气波的观测和表征,特别是探索我们的Fe Boltzmann激光雷达对麦克默多(77.8°S,166.7°E本文在南极中高层大气中发现了一种新的波浪现象,即持续时间为3--10 h的持续惯性重力波。这组大振幅波主导了从平流层到较低热层(约30--115 km)的温度扰动。它们如此频繁地出现,以至于看起来无休止且不间断,从而影响了SAIR的组成,化学和热力学。本论文首次报道了南极惯性重力波同时进行的激光雷达/雷达观测。本文利用2011年至2015年6月的激光雷达数据,首次描述了持续重力波的性质。这些波在3.5--10 h的时间内表现出20--30 km的统一主垂直波长,垂直相位速度为0.8--2 m / s。在约93%的时间内,它们拥有超过一半的光谱能量。 2014年6月28日至30日对65小时激光雷达数据的分析显示,多个波包的时间长达60小时。对5月和7月数据的进一步分析证实了这些波的持久性和优势性,但揭示了逐月的变化性;本论文开发了一种波分析方法系统,包括从中性线〜30--155 km处提取重力波。第一次的气氛。我们的方法还包括用于同时进行激光雷达/雷达数据的时间全息法;改进的一维Morlet小波变换方法;严格的前白化和后上色光谱分析技术;以及自动二维Morlet小波分析和合成方法。这些方法的成功应用为引力波,其来源以及对整个大气和空间的影响提供了新的见解。

著录项

  • 作者

    Chen, Cao.;

  • 作者单位

    University of Colorado at Boulder.;

  • 授予单位 University of Colorado at Boulder.;
  • 学科 Aerospace engineering.
  • 学位 Ph.D.
  • 年度 2016
  • 页码 212 p.
  • 总页数 212
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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