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Empirical orthogonal functions and related techniques in atmospheric science: A review

机译:大气科学中的经验正交函数及相关技术:综述

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Climate and weather constitute a typical example where high dimensional and complex phenomena meet. The atmospheric system is the result of highly complex interactions between many degrees of freedom or modes. In order to gain insight in understanding the dynamical/physical behaviour involved it is useful to attempt to understand their interactions in terms of a much smaller number of prominent modes of variability. This has led to the development by atmospheric researchers of methods that give a space display and a time display of large space-time atmospheric data. Empirical orthogonal functions (EOFs) were first used in meteorology in the late 1940s. The method, which decomposes a space-time field into spatial patterns and associated time indices, contributed much in advancing our knowledge of the atmosphere. However, since the atmosphere contains all sorts of features, e.g. stationary and propagating, EOFs are unable to provide a full picture. For example, EOFs tend, in general, to be difficult to interpret because of their geometric properties, such as their global feature, and their orthogonality in space and time. To obtain more localised features, modifications, e.g. rotated EOFs (REOFs), have been introduced. At the same time, because these methods cannot deal with propagating features, since they only use spatial correlation of the field, it was necessary to use both spatial and time information in order to identify such features. Extended and complex EOFs were introduced to serve that purpose. Because of the importance of EOFs and closely related methods in atmospheric science, and because the existing reviews of the subject are slightly out of date, there seems to be a need to update our knowledge by including new developments that could not be presented in previous reviews. This review proposes to achieve precisely this goal. The basic theory of the main types of EOFs is reviewed, and a wide range of applications using various data sets are also provided. Copyright (C) 2007 Royal Meteorological Society
机译:气候和天气是高维和复杂现象相遇的典型例子。大气系统是许多自由度或模式之间高度复杂的相互作用的结果。为了获得对所涉及的动力学/物理行为的理解的洞察力,尝试以数量少得多的突出可变性模式来理解它们的相互作用是有用的。这导致了大气研究人员开发出可以显示大时空大气数据的空间并对其进行时间显示的方法。经验正交函数(EOF)在1940年代后期首次用于气象学。该方法将时空场分解为空间模式和相关的时间指标,对增进我们对大气的了解做出了很大贡献。但是,由于大气层具有各种特征,例如静止的和传播中的EOF无法提供完整的图像。例如,由于它们的几何特性(例如它们的全局特征)以及它们在空间和时间上的正交性,通常,EOF往往难以解释。为了获得更多的局部特征,可以进行修改,例如引入了旋转EOF(REOF)。同时,由于这些方法不能处理传播的特征,因为它们仅使用场的空间相关性,因此有必要使用空间和时间信息来识别这些特征。为此目的引入了扩展的和复杂的EOF。由于EOF和紧密相关的方法在大气科学中的重要性,并且由于该主题的现有评论略有过时,因此似乎有必要通过纳入以前的评论中无法提供的新进展来更新我们的知识。 。这篇综述提出了精确实现这一目标的提议。回顾了EOF主要类型的基本理论,并提供了使用各种数据集的广泛应用。皇家气象学会(C)2007

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