首页> 外文学位 >STUDY OF ACOUSTIC-GRAVITY WAVE SPECTRA IN THE ATMOSPHERE USING MESOSPHERE-STRATOSPHERE- TROPOSPHERE RADAR (PROPAGATION, UNIVERSAL SPECTRUM).
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STUDY OF ACOUSTIC-GRAVITY WAVE SPECTRA IN THE ATMOSPHERE USING MESOSPHERE-STRATOSPHERE- TROPOSPHERE RADAR (PROPAGATION, UNIVERSAL SPECTRUM).

机译:用中层-平层-对流层雷达(传播,通用光谱)研究大气中的声重力波谱。

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摘要

Current research indicates that acoustic-gravity waves can greatly influence the large-scale dynamics of the middle atmosphere. The morphology and structure of the atmospheric processes which cause this phenomenon can be better understood by the study of acoustic-gravity wave spectra. In order to use the meso-scale wind fluctuation data measured by MST radars to investigate such spectra, it is necessary to apply the relation between the observed wind fluctuation spectrum and the wave spectrum. The correct relationship is quantitatively derived in this study, based on acoustic-gravity wave theory and radar observation principle. Theoretical spectra are computed for a vertically and azimuthally symmetric wave model and also for a more general asymmetric model. Examples are given to show how the theoretical results can be used to interpret the one-dimensional observational data as well as to derive parameters for the model wave spectrum. The Doppler shift produced by the presence of a horizontal background wind is also examined since it leads to a redistribution of power in the observed frequency spectrum. The model is also generalized in order to determine the conditions for which the extended radar beam-width can affect the observed spectrum. An interpretation is further made of a two-dimensional observed spectrum by comparison to the two-dimensional model spectrum. The theoretical results are used to propose additional tests for the consistency of the acoustic-gravity wave model for atmospheric wind fluctuations.
机译:当前的研究表明,声重力波可以极大地影响中层大气的大规模动力学。引起重力现象的大气过程的形态和结构可以通过研究重力波谱来更好地理解。为了使用由MST雷达测得的中尺度风波动数据来研究此类频谱,有必要应用观测到的风波动谱与波谱之间的关系。本研究基于声波理论和雷达观测原理定量推导了正确的关系。理论光谱是针对垂直和方位对称波模型以及更一般的非对称模型计算的。举例说明了如何将理论结果用于解释一维观测数据以及推导出模型波谱的参数。由于存在水平背景风而产生的多普勒频移也被检查了,因为它会导致功率在观察到的频谱中重新分配。还对该模型进行了通用化,以确定扩展的雷达波束宽度可以影响所观察频谱的条件。通过与二维模型光谱比较,进一步解释了二维观察光谱。理论结果被用来为大气风波动的声重力波模型的一致性提出额外的测试。

著录项

  • 作者

    SCHEFFLER, ALBERT O.;

  • 作者单位

    University of Illinois at Urbana-Champaign.;

  • 授予单位 University of Illinois at Urbana-Champaign.;
  • 学科 Engineering Electronics and Electrical.
  • 学位 Ph.D.
  • 年度 1986
  • 页码 268 p.
  • 总页数 268
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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