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The breakup of stratospheric polar vortices.

机译:平流层极涡旋破裂。

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摘要

The temperature in the Earth's stratosphere (between 12 to 50 km) increases with altitude due to ultraviolet heating of ozone. A strong circumpolar flow, called the stratospheric polar vortex, forms during polar winter when ultraviolet heating ceases in this region. These polar vortices last until spring and then break up as ultraviolet heating returns. The structure and evolution of the polar vortices have significant implications on ozone depletion and on global and regional climates.; In this thesis 40 years of meteorological analyses are used to examine the evolution of, and stirring around, the Arctic vortex, with focus on the breakup stage. Two extreme regimes of vortex breakup are found, late and early breakups, with very different decay characteristics. The occurrence of these different breakups is closely related to the interannual variability of the forcing due to the upward propagating planetary waves.; A shallow water model is used to examine the basic processes responsible for the different observed regimes. This model includes topographic forcing, to represent the upward propagating waves, and relaxation to an equilibrium state, to represent radiative processes. The roles of, and competition between, topographic wave forcing and radiative relaxation are examined by systematically varying the different parameters. Both steady and vacillation states are produced, which may be related to cold and warm polar stratospheres, respectively. Calculations with an annual cycle for the radiative equilibrium state and different timing and seasonality of the bottom forcing are also performed to produce the observed breakup regimes.; A new hybrid numerical method which includes diabatic forcing and can resolve steep gradients is also tested and used to further examine the competition between the external forcing and radiative relaxation. Calculations of idealized planar flows show that the relaxation damps out the oscillations in the elongation as well as orientation of a forced vortex, but steep vorticity gradients are preserved for at least 10 vortex overturning periods.
机译:由于臭氧的紫外线加热,地球平流层中的温度(12至50 km之间)随海拔升高而升高。当极地冬季在该区域停止紫外线加热时,会形成强烈的绕极流,称为平流层极涡。这些极地涡旋一直持续到春天,然后随着紫外线的加热而破裂。极地涡旋的结构和演变对臭氧消耗以及全球和区域气候具有重要影响。在这篇论文中,使用了40年的气象分析来研究北极涡旋的演变过程,并围绕其解旋阶段进行研究。发现了两种极端的涡旋破裂状态,即晚期破裂和早期破裂,其衰减特性非常不同。由于向上传播的行星波,这些不同的破裂的发生与强迫的年际变化密切相关。浅水模型用于检查负责不同观测方案的基本过程。此模型包括地形强迫(代表向上传播的波)和松弛到平衡状态(代表辐射过程)。通过系统地改变不同的参数,研究了地形波强迫和辐射弛豫的作用以及它们之间的竞争。稳态和波动状态都会产生,这可能分别与冷平流层和暖流平流层有关。还以辐射平衡状态的年度周期以及底部强迫的不同时机和季节进行了计算,以产生观察到的破裂状态。还测试了一种新的混合数值方法,该方法包括非绝热强迫并且可以解决陡峭的梯度,并用于进一步检查外部强迫与辐射松弛之间的竞争。理想化平面流动的计算表明,弛豫可减弱强迫涡旋的伸长率和取向中的振荡,但是在至少10个涡旋翻转周期中,陡峭的涡度梯度会保留下来。

著录项

  • 作者

    Rong, Ping-ping.;

  • 作者单位

    The Johns Hopkins University.;

  • 授予单位 The Johns Hopkins University.;
  • 学科 Physics Atmospheric Science.; Geophysics.
  • 学位 Ph.D.
  • 年度 2003
  • 页码 251 p.
  • 总页数 251
  • 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

  • 入库时间 2022-08-17 11:44:54

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