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Influences of planetary waves upon the dynamics of the mesosphere and lower thermosphere.

机译:行星波对中层和低层热层动力学的影响。

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摘要

Planetary Waves (PW) are global scale atmospheric oscillations usually with periods of 2–25 days and westward propagation with zonal wave numbers typically of 1–3. This project is to study the influences of PWs upon the mesosphere and lower thermosphere (MLT, 60–110 km), including the wave propagation, energy transfer and their climatology and variations.; Methodology has involved the analysis of data obtained from the Saskatoon MF (medium frequency) radar along with several other MF radars located from the arctic to equator; each of them can detect the local horizontal winds in the MLT region. The satellite measurements (UARS-HRDI) were also used in an attempt to obtain a global view of the waves.; Considering 16-day waves for example, they usually dominate the winter PW spectrum. Because of this, and since the 2-day waves have been extensively studied, the focus of this program of research has been upon the 16-day wave. The winter dominance of this wave is in good agreement with theoretical predictions that for westward travelling waves the vertical propagation is permitted only in a relatively eastward background wind. The wave longitudinal/latitudinal phase differences also indicate small horizontal wavenumbers (i.e. global scale features). The wave has been shown to be highly episodic in space and time in the MLT region. The wave vertical characteristics show significant energy deposition; also in some situations they show standing wave structures. A special experiment was carried out with the Global Scale Wave Model (GSWM) and the results were compared with the observations with special focus upon latitudinal variations. The comparisons show similarities in many aspects, but there are also dramatic differences in some situations that indicate the extreme sensitivity of the 16-day wave to the global background winds, and the complexity of the real atmosphere.; Energy sources directly associated with solar activity have also been considered for the explanation of some extra-long period (20–40 day) oscillations, which are comparable with the solar-rotation period. Finally, the modulation of gravity waves by 2 and 16-day waves, as well as non-linear interaction with tidal waves were investigated.
机译:行星波(PW)是全球范围的大气振荡,周期通常为2-25天,向西传播的纬向波数通常为1-3。该项目旨在研究PW对中层和低层热圈(MLT,60-110 km)的影响,包括波的传播,能量传递及其气候和变化。方法论涉及从萨斯卡通MF(中频)雷达以及从北极到赤道的其他几个MF雷达获得的数据的分析。他们每个人都可以检测MLT区域的局部水平风。卫星测量(UARS-HRDI)也被用于试图获得海浪的整体视线。例如,考虑16天的海浪,它们通常在冬季PW频谱中占主导地位。因此,由于对2天的浪潮进行了广泛的研究,因此本研究计划的重点一直放在16天的浪潮上。该波的冬季优势与理论预测非常一致,即对于向西传播的波,仅在相对向东的背景风中才允许垂直传播。波的纵向/纬度相位差也表示水平波数较小(即整体尺度特征)。在MLT区域,该波在时空上表现出高度的偶发性。波的垂直特性显示出明显的能量沉积;在某些情况下,它们也表现出驻波结构。使用全球尺度波模型(GSWM)进行了一项特殊的实验,并将结果与​​观察结果进行了比较,并特别关注纬度变化。比较显示了许多方面的相似性,但是在某些情况下也存在巨大差异,这表明16天的波浪对全球背景风的极端敏感性以及真实大气的复杂性。还考虑了与太阳活动直接相关的能源来解释某些超长周期(20-40天)的振荡,这与太阳旋转周期相当。最后,研究了2天和16天波对重力波的调制以及与潮汐波的非线性相互作用。

著录项

  • 作者

    Luo, Yi.;

  • 作者单位

    The University of Saskatchewan (Canada).;

  • 授予单位 The University of Saskatchewan (Canada).;
  • 学科 Physics Atmospheric Science.; Geophysics.
  • 学位 Ph.D.
  • 年度 2002
  • 页码 217 p.
  • 总页数 217
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 大气科学(气象学);地球物理学;
  • 关键词

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