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Horizontal vorticity redistribution and vortex alignment in developing and mature tropical cyclones.

机译:发展中和成熟的热带气旋的水平涡度再分布和涡旋对准。

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摘要

The three-dimensional redistribution of vorticity within a vortex is examined here in the context of tropical cyclone (TC) structure and intensity change. Aspects of the horizontal vorticity mixing dynamics are first presented in a novel analysis of high temporal resolution wind fields derived from airborne dual-Doppler observations of Hurricane Olivia (1994). Seven consecutive composites of Olivia's wind field with 30-min time resolution depict a weakening storm undergoing substantial structural changes.; The problem of vortex alignment (and the attendant three-dimensional redistribution of vorticity) is then re-examined in an effort to further understand the underlying dynamics of TC-like vortices tilted by vertical shear. The study is motivated in part by the analysis of Hurricane Olivia. Olivia's asymmetric evolution in the presence of increasing environmental vertical shear is consistent with that predicted by existing “vortex in shear” theories. These theories, however, are based on a nonlinear interpretation of unforced vortex alignment originally developed to explain the emergence of vertically-coherent vortex structures in geostrophic turbulence. For small to moderate vortex tilts, a simpler and more insightful linear model for unforced vortex alignment is presented. This model provides the basis for a deeper understanding of the dynamics of rapidly-rotating, vertically-sheared vortices.; The linear model is formally valid as long as the tilted vortex can be meaningfully represented through a wave, mean-flow decomposition. This is typically true if the vortex cores at upper and lower levels overlap. The validity of the linear model is tested for a range of vortex tilts using a quasi-geostrophic model in both its complete and linear, equivalent-barotropic forms.; The vertical alignment dynamics in the aforementioned small to moderate tilt regime is accurately captured by linear vortex Rossby wave processes. For internal Rossby deformation radii larger than the horizontal scale of the tilted vortex, an azimuthal wavenumber one near-discrete vortex Rossby wave, or quasi-mode, exists. The quasi-mode is characterized by its steady cyclonic propagation, long lifetime, and resistance to differential rotation, behaving much like a discrete vortex Rossby wave. The quasi-mode traps disturbance energy causing the vortex to precess and thus prevents alignment. For internal deformation radii smaller than the horizontal vortex scale, the quasi-mode disappears into the continuous spectrum of vortex Rossby waves which promote complete alignment by irreversibly (but linearly) redistributing potential vorticity (PV).; The linear alignment theory is extended to stronger vortices in the Asymmetric Balance system with results similar to those for geostrophic vortices. In addition to providing new insight into the asymptotic dynamics of vortex merger in three dimensions, these results also are believed to have relevance to the problem of tropical cyclogenesis. Cyclogenesis initiated through the merger of low-level convectively-generated positive PV within a weak incipient vortex is captured by quasi-linear dynamics. A potential dynamical barrier to TC development in which the quasi-mode frustrates vertical alignment can be identified using the linear alignment theory in this case.
机译:本文在热带气旋(TC)结构和强度变化的背景下,研究了涡旋内涡度的三维重新分布。首先从对奥利维亚飓风(1994年)的机载双多普勒观测资料推导出的高时间分辨率风场的新型分析中,首先介绍了水平涡旋混合动力学的各个方面。奥利维亚风场的七个连续复合材料(时间分辨率为30分钟)表示正在减弱的风暴正在经历实质性的结构变化。然后重新检查涡旋对准的问题(以及随之而来的三维三维涡度再分配),以进一步了解垂直剪切倾斜的TC类涡旋的基本动力学。这项研究的部分动机是对奥利维亚飓风的分析。在环境垂直剪切增加的情况下,Olivia的不对称演变与现有“剪切涡”理论所预测的一致。然而,这些理论基于对非强迫涡旋对准的非线性解释,该解释最初是为解释地转湍流中垂直相干涡旋结构的出现而开发的。对于小到中等的涡旋倾斜度,提出了一种用于无力涡旋对准的更简单,更深入的线性模型。该模型为深入理解快速旋转的垂直剪切涡流的动力学提供了基础。线性模型在形式上是有效的,只要倾斜的涡流可以通过波浪均流分解来有意义地表示即可。如果上下两层的涡流核重叠,通常会发生这种情况。使用准地转营养模型以其完整和线性,等效正压形式测试了线性模型的有效性。通过线性涡旋Rossby波过程可以准确地捕获上述小到中等倾斜状态下的垂直对齐动力学。对于大于倾斜涡旋水平尺度的内部Rossby变形半径,存在一个接近一离散涡旋的Rossby波或准模式的方位角波。准模式的特征在于其稳定的气旋传播,较长的寿命以及对微分旋转的抵抗力,其行为非常类似于离散涡旋罗斯比波。准模式捕获扰动能量,使旋涡进动,从而阻止对准。对于小于水平涡旋尺度的内部变形半径,准模消失在涡旋罗斯比波的连续光谱中,通过不可逆地(但线性地)重新分配潜在涡度(PV),促进了完全对准。线性对准理论被扩展到非对称平衡系统中更强的涡旋,其结果与地转涡旋的结果相似。除了在三个维度上提供关于涡旋合并的渐近动力学的新见解外,还认为这些结果与热带气旋的产生有关。准线性动力学捕获了由弱对流中低水平对流生成的正PV合并而启动的循环生成。在这种情况下,可以使用线性对准理论来确定准模阻碍垂直对准的潜在的TC发展动力障碍。

著录项

  • 作者

    Reasor, Paul David.;

  • 作者单位

    Colorado State University.;

  • 授予单位 Colorado State University.;
  • 学科 Physics Atmospheric Science.
  • 学位 Ph.D.
  • 年度 2000
  • 页码 167 p.
  • 总页数 167
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 大气科学(气象学);
  • 关键词

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