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Scales, Growth Rates, and Spectral Fluxes of Baroclinic Instability in the Ocean

机译:海洋中斜压不稳定的规模,增长率和谱通量

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摘要

An observational, modeling, and theoretical study of the scales, growth rates, and spectral fluxes of baroclinic instability in the ocean is presented, permitting a discussion of the relation between the local instability scale; the first baroclinic deformation scale R_(def); and the equilibrated, observed eddy scale. The geography of the large-scale, meridional quasigeostrophic potential vorticity (QGPV) gradient is mapped out using a cli-matological atlas, and attention is drawn to asymmetries between midlatitude eastward currents and subtropical return flows, the latter of which has westward and eastward zonal velocity shears. A linear stability analysis of the climatology, under the "local approximation," yields the growth rates and scales of the fastest-growing modes. Fastest-growing modes on eastward-flowing currents, such as the Kuroshio and the Antarctic Circumpolar Current, have a scale somewhat larger (by a factor of about 2) than R_(def). They are rapidly growing (e folding in 1-3 weeks) and deep reaching, and they can be characterized by an interaction between interior QGPV gradients, with a zero crossing in the QGPV gradient at depth. In contrast, fastest-growing modes in the subtropical return flows (as well as much of the gyre interiors) have a scale smaller than R_(def) (by a factor of between 0.5 and 1), grow more slowly (e-folding scale of several weeks), and owe their existence to the interaction of a positive surface QGPV gradient and a negative gradient beneath. These predictions of linear theory under the local approximation are then compared to observed eddy length scales and spectral fluxes using altimetric data. It is found that the scale of observed eddies is some 2-3 times larger than the instability scale, indicative of a modest growth in horizontal scale. No evidence of an inverse cascade over decades in scale is found. Outside of a tropical band, the eddy scale varies with latitude along with but somewhat less strongly than R_(def). Finally, exactly the same series of calculations is carried out on fields from an idealized global eddying model, enabling study in a more controlled setting. Broadly similar conclusions are reached, thus reinforcing inferences made from the data.
机译:对海洋中斜压不稳定的尺度,增长率和光谱通量进行了观测,建模和理论研究,从而可以讨论局部不稳定尺度之间的关系;第一斜压变形尺度R_(def);以及均衡的观察涡度。使用气候图集绘制大尺度子午准营养液涡度(QGPV)梯度的地理分布,并注意中纬度东向洋流与亚热带回流之间的不对称性,其中亚热带回流具有西向和东向纬向带速度剪。在“局部近似”下对气候学进行线性稳定性分析,可以得出增长速度最快的模式的规模和规模。黑潮和南极绕极洋等东向洋流中增长最快的模式的尺度比R_(def)稍大(约为2倍)。它们迅速生长(在1-3周内折叠)并到达深处,它们的特征在于内部QGPV梯度之间的相互作用,深度处QGPV梯度为零。相比之下,亚热带回流(以及许多回旋内部)中增长最快的模式的尺度小于R_(def)(介于0.5到1之间),增长速度较慢(电子折叠尺度)数周之内),并且它们的存在归因于正表面QGPV梯度和下方的负梯度的相互作用。然后使用高度计数据将这些在局部近似下的线性理论预测与观测到的涡流长度尺度和频谱通量进行比较。发现所观察到的涡旋的尺度比不稳定性尺度大大约2-3倍,这表明水平尺度的适度增长。没有发现数十年来规模逆级联的证据。在热带带以外,涡旋尺度随纬度变化,但略小于R_(def)。最后,从理想的全局涡流模型对场进行完全相同的一系列计算,从而可以在更可控的环境中进行研究。得出大致相似的结论,从而加强了从数据得出的推论。

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  • 来源
    《Journal of Physical Oceanography》 |2011年第6期|p.1057-1076|共20页
  • 作者单位

    Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139;

    Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts;

    Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts;

    Center for Atmosphere Ocean Science, New York University, New York, New York;

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