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Geostrophic dynamics at surfaces in the atmosphere and ocean.

机译:大气和海洋表面的地转动力学。

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摘要

Observed dynamics near bounding upper surfaces in the atmosphere and ocean are interpreted in terms of quasi-geostrophic theory. The quasi-geostrophic equations consist of advection of linearized potential vorticity coupled with advection of temperature at the upper and lower bounding surfaces. We show that the standard vertical finite difference formulation of 3D quasi-geostrophic flow accurately represents the flow only down to a critical horizontal scale that decreases with vertical grid spacing. To overcome this constraint, we derive a surface-modal formulation which accurately and efficiently captures both the surface dynamics due to temperature anomalies on the upper and lower boundaries, and the interior dynamics due to potential vorticity anomalies, without the need for high vertical resolution.In the atmosphere, the horizontal wavenumber spectra of wind and temperature near the tropopause have a steep -3 slope at synoptic scales and a shallow -5/3 slope at mesoscales, with a smooth transition between the two regimes from 800km to 200km. We demonstrate that when the surface temperature anomalies are resolved, quasi-geostrophic flow driven by baroclinic instability exhibits such a transition near the tropopause. The horizontal scale of transition between -3 and -5/3 slopes depends on the relative magnitudes of the mean surface temperature gradient and the mean potential vorticity gradient.In the ocean, sea surface height anomalies measured by satellite altimetry exhibit shallower spectral slopes than quasi-geostrophic theory predicts, and faster than expected westward phase propagation of sea surface height in the midlatitudes. We argue that, in some regions, the shallow spectral slopes are due to surface quasi-geostrophic dynamics, and that the westward phase propagation in the midlatitudes is indicative of a transition from a linear Rossby wave regime in the tropics to a nonlinear turbulent regime in the midlatitudes.
机译:大气和海洋边界上表面附近的观测动力学是用准地转理论来解释的。准地转方程由线性势能涡度的对流与上下边界表面的温度对流组成。我们显示了3D准地转流的标准垂直有限差分公式准确地表示了仅向下到临界水平尺度的流量,该水平尺度随垂直网格间距而减小。为克服此限制,我们推导了一种表面模态公式,该公式可准确有效地捕获由于上下边界温度异常引起的表面动力学以及由于潜在涡度异常引起的内部动力学,而无需很高的垂直分辨率。在大气层中,对流层顶附近的风和温度的水平波数谱在天气尺度上具有陡峭的-3斜率,在中尺度上具有较浅的-5/3斜率,这两种模式在800km至200km之间平滑过渡。我们证明,当表面温度异常得到解决时,斜压不稳定性驱动的准地转流在对流层顶附近表现出这种过渡。 -3和-5/3斜率之间的水平过渡尺度取决于平均表面温度梯度和平均潜在涡度梯度的相对大小。在海洋中,通过卫星测高仪测得的海面高度异常显示出比准海面浅的光谱斜率地转理论预测中纬度海面高度向西传播的速度要快于预期。我们认为,在某些地区,较浅的光谱斜率是由于地表准地转动力学引起的,中纬度的西向传播是热带地区从线性罗斯比波态向非线性湍流态的转变。中纬度地区。

著录项

  • 作者

    Tulloch, Ross.;

  • 作者单位

    New York University.;

  • 授予单位 New York University.;
  • 学科 Physical Oceanography.Atmospheric Sciences.
  • 学位 Ph.D.
  • 年度 2008
  • 页码 184 p.
  • 总页数 184
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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