一种数据同化算法:湍流三维Leray-α模型的范式

A. Farhat, E. Lunasin, E. Titi
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引用次数: 22

摘要

. 本文综述了一种新的基于空间粗网格测量的数据同化(降尺度)算法的各种实现。作为范例,我们演示了该算法在三维Leray- α亚网格尺度湍流模型中的应用。最重要的是,我们使用这种范式来表明,为了恢复相应的精确参考解,并不总是需要收集所有状态变量的粗网格测量,这些状态变量涉及潜在的进化系统。具体来说,我们证明了在三维Leray- α湍流模型的情况下,该算法的解仅使用三维速度场的任意两个分量的粗网格观测,而不包含任何第三个分量的信息,以指数速度收敛到三维Leray- α模型的相应精确参考解。本研究作为我们最近对二维Navier-Stokes方程的简化连续数据同化工作的补充。值得注意的是,最近在三维粘性行星地转环流模型中也建立了类似的结果,其中我们表明,通过我们的数据同化算法,仅粗网格温度测量就足以恢复完整的解;即速度矢量场和温度的三个分量。从而证明了三维行星地转模型的Charney猜想;也就是说,大空间尺度温度的历史足以确定模型的所有其他量(状态变量)。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A Data Assimilation Algorithm: the Paradigm of the 3D Leray-α Model of Turbulence
. In this paper we survey the various implementations of a new data assimilation (downscaling) algorithm based on spatial coarse mesh measurements. As a paradigm, we demonstrate the application of this algorithm to the 3D Leray- α subgrid scale turbulence model. Most importantly, we use this paradigm to show that it is not always necessary that one has to collect coarse mesh measurements of all the state variables, that are involved in the underlying evolutionary system, in order to recover the corresponding exact reference solution. Specifically, we show that in the case of the 3D Leray- α model of turbulence the solutions of the algorithm, constructed using only coarse mesh observations of any two components of the three-dimensional velocity field , and without any information of the third component, converge, at an exponential rate in time, to the corresponding exact reference solution of the 3D Leray- α model. This study serves as an addendum to our recent work on abridged continuous data assimilation for the 2D Navier-Stokes equations. Notably, similar results have also been recently established for the 3D viscous Planetary Geostrophic circulation model in which we show that coarse mesh measurements of the temperature alone are sufficient for recovering, through our data assimilation algorithm, the full solution; viz. the three components of velocity vector field and the temperature. Consequently, this proves the Charney conjecture for the 3D Planetary Geostrophic model; namely, that the history of the large spatial scales of temperature is sufficient for determining all the other quantities (state variables) of the model.
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