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arXiv physics/0307142physics.ao-ph
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深海对上层海洋斜压不穩定饱和度的影响

Deep ocean influence on upper ocean baroclinic instability saturation

M. J. Olascoaga, F. J. Beron-Vera, J. Sheinbaum

摘要:

在本文中,我们推广了以前的结果,关于海洋的下层(以下的温跃层)的斜压不穩定的上层(以上的温跃层)的影响。我们面对的准地转斜压不穩定性质的2.5层模式与3层模式的一个非常厚的深层,这已被证明是预测谱不稳定的基本状态参数的2.5层模式预测的非线性稳定。我们计算并比较了最大正模扰动增长率,以及不稳定基本状态扰动非线性增长的严格上界,特别注意2.5层和3层模型的稳定性特性差异很大的基本状态参数区域。我们发现,正常模式的扰动增长率在3层模型往往在这一地区最大化。我们还发现,涡振幅增长的状态空间的大小趋于最小化,在同一区域。此外,我们发现,对于一个大的传播参数值在这个区域中,后者的大小减少到只有一小部分的系统的总拟能,从而使我们能够作出评估的意义的不稳定性。

英文摘要:

In this paper we extend earlier results regarding the effects of the lower layer of the ocean (below the thermocline) on the baroclinic instability within the upper layer (above the thermocline). We confront quasigeostrophic baroclinic instability properties of a 2.5-layer model with those of a 3-layer model with a very thick deep layer, which has been shown to predict spectral instability for basic state parameters for which the 2.5-layer model predicts nonlinear stability. We compute and compare maximum normal-mode perturbation growth rates, as well as rigorous upper bounds on the nonlinear growth of perturbations to unstable basic states, paying particular attention to the region of basic state parameters where the stability properties of the 2.5- and 3-layer model differ substantially. We found that normal-mode perturbation growth rates in the 3-layer model tend to maximize in this region. We also found that the size of state space available for eddy-amplitude growth tends to minimize in this same region. Moreover, we found that for a large spread of parameter values in this region the latter size reduces to only a small fraction of the total enstrophy of the system, thereby allowing us to make assessments of the significance of the instabilities.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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