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On the meridional structure of extra-tropical Rossby waves

机译:关于温带罗斯比波的子午线结构

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摘要

The common derivation of Rossby waves is based on the quasi-geostrophic approximation. A simple non-harmonic approximation for extratropical Rossby waves on the sphere is proposed, in which the meridional coordinate is a parameter instead of a continuous variable. It is shown that, in contrast to the quasi-geostrophic solution, to first order the meridional structure of these non-harmonic Rossby waves becomes irrelevant for determining the dispersion relation in this theory. The proposed approximation accurately reproduces numerical results obtained from runs of an ocean general circulation model initiated from several initial meridional structures and captures the latitudinal dependence of the phase speed of these waves. The proposed theory yields explicit expressions for the dispersion relation and for the meridional structure of the waves.
机译:Rossby波的常见推导基于准地转近似。提出了球面上温带Rossby波的简单非谐波近似,其中子午坐标是一个参数,而不是连续变量。结果表明,与准地转解相反,这些非谐波罗斯比波的子午结构对确定该色散关系不重要。拟议的近似值准确地再现了从几个初始子午线结构启动的海洋总环流模型的运行中获得的数值结果,并捕获了这些波的相速度的纬度相关性。所提出的理论为波的色散关系和子午线结构给出了明确的表达式。

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  • 来源
    《Tellus》 |2011年第4期|p.817-827|共11页
  • 作者单位

    Solar Energy and Environmental Physics, BIDR, Ben-Gurion University of the Negev, Midreshet Ben-Gurion 84990, Israel;

    Institute of Earth Sciences, The Hebrew University of Jerusalem, Jerusalem 91904, Israel;

    Solar Energy and Environmental Physics, BIDR, Ben-Gurion University of the Negev, Midreshet Ben-Gurion 84990, Israel;

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