1.Global Systems Laboratory, NOAA/OAR, Boulder, CO 80305, USA 2.General Atomics, Electromagnetic Systems Group, Longmont, CO 80501, USA 3.Earth Signals and Systems Group, Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA 4.Department of Civil and Environmental Engineering University of Connecticut, Storrs, CT 06269, USA Manuscript received: 2020-07-28 Manuscript revised: 2021-02-09 Manuscript accepted: 2021-02-18 Abstract: Weather manifests in spatiotemporally coherent structures. Weather forecasts hence are affected by both positional and structural or amplitude errors. This has been long recognized by practicing forecasters (cf., e.g., Tropical Cyclone track and intensity errors). Despite the emergence in recent decades of various objective methods for the diagnosis of positional forecast errors, most routine verification or statistical post-processing methods implicitly assume that forecasts have no positional error. The Forecast Error Decomposition (FED) method proposed in this study uses the Field Alignment technique which aligns a gridded forecast with its verifying analysis field. The total error is then partitioned into three orthogonal components: (a) large scale positional, (b) large scale structural, and (c) small scale error variance. The use of FED is demonstrated over a month-long MSLP data set. As expected, positional errors are often characterized by dipole patterns related to the displacement of features, while structural errors appear with single extrema, indicative of magnitude problems. The most important result of this study is that over the test period, more than 50% of the total mean sea level pressure forecast error variance is associated with large scale positional error. The importance of positional error in forecasts of other variables and over different time periods remain to be explored. Keywords: forecast error, orthogonal decomposition, positional, structural 摘要:天气系统显示出时空连续的结构。因此,天气预报受到位置误差和结构(或振幅)误差的影响。预报员很早就已经认识到这个问题了(例如对于热带气旋的路径和强度的预报误差)。尽管最近几十年,已经有一些客观的方法用于对位置相关的预报误差进行诊断,大多数常规的检验或者统计后处理方法仍然假定预报中不存在位置相关的误差。本文提出了一种预报误差分解的方法(Forecast Error Decomposition, FED),该方法利用场调整的技术,将一个格点的预报场向其对应的分析场进行调整。利用这种方法可以将总误差分解成三个正交分量:(a)大尺度位置误差,(b)大尺度结构误差,和(c)小尺度误差。将FED方法应用于一个月的平均海表气压数据。结果显示,位置误差呈现偶极型,和特征的位置偏移有关,而结构(振幅)误差呈现单极型,表征了特征的振幅偏差。该研究中最重要的结果就是在试验的时长内,海表气压预报的总误差方差有50%以上和大尺度的位置误差有关,说明了预报中的位置误差的重要性。其它变量和其它时间段的预报误差的分解和位置误差的比重还需要进一步的研究。 关键词:预报误差, 正交分解, 位置误差, 结构误差
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2.1. Field Alignment
As Hoffman et al. (1995) point out, there is no unique way of defining forecast displacement errors. In this study, we test the use of an alternative technique, the FA technique (Ravela et al., 2007) in FED. FA and its variants in the Field Alignment System and Testbed (FAST, Ravela, 2007; Ravela et al., 2007) align two gridded fields (in its FED application, a forecast with its verifying analysis field) by smoothly remapping the coordinate system underlying the state of a variable. For example, for two 2D fields of a state variable (e.g. surface temperature), where one field is the observed or analyzed field (which would be considered as the target state) and the other one is a forecast of that field valid at the same time, the FA method estimates a smooth 2D displacement vector field that aligns the forecast with the analysis field. If the displacement vectors are applied to each grid point of the original forecast field as a translation operation in 2D space, the result is an adjusted forecast field for which the difference in RMSE between this aligned field and the analysis field (i.e., cost function) is minimized. The displacement vector field and the aligned field are derived through a variational minimization of the cost function in FA (Ravela, 2007). The smoothness of the displacement vector field is controlled via a “smoothness wavenumber parameter” (SWP) in the FA truncation algorithm (Ravela, 2012). SWP defines the scales at which alignments of features between two fields are performed. Smaller scale features are moved along with the larger scale features that are aligned, without additional adjustments. SWP is the only free parameter in FA and it is analogous to the choice of truncation in Hoffman et al.’s (1995) approach. Unlike the method proposed by Hoffman et al. (1995), FA does not rely on forecast error covariance information. For additional details on how FA differs from the method of Hoffman et al. (1995), see Ravela et al., 2007; and Ravela, 2014. As for other FA applications, Ravela (Ravela, 2007; Ravela et al., 2007) and Williams (2008) align the first guess forecast field with the latest observations before the application of a standard data assimilation scheme. This pre-processing reduces the remaining, mostly amplitude errors for a further improvement in the fit to the observations. FA has also been used to analyze (with ensemble-based analysis approaches, Ravela et al., 2009; Ravela, 2012, 2014) and represent (e.g., Ravela et al., 2009) coherent structures in other fluid applications. Additionally, FA has been found to be an effective tool for nowcasting (Ravela, 2012, 2014), initialization, verification (Ravela et al., 2007; Ravela, 2014), and various other applications (Yang and Ravela, 2009a,b; Ravela, 2015a, b).
2 2.2. Forecast Error Decomposition -->
2.2. Forecast Error Decomposition
The purpose of this study is to demonstrate the use of the FA technique in FED for the quantification of what is subjectively perceived as major modes of error. In our study, we will use Error Variance (EV, or on some figures, its root, the Root Mean Square error—RMS) as traditional, scalar references measuring the difference between two 2D fields. The total forecast error variance (Et) is defined as a difference between forecast (F) and analysis (A) fields. A displacement operator (D) adjusts the forecast field to a new, aligned state (Fa) for which the difference in RMSE between the forecast field (F) and the analysis (A) is minimized. The displacement operator generates both the displacement vector field and the scalar field of the magnitude of displacement. As pointed out in section 2.1, only large scale features of F are aligned with similar features in A. Correspondingly, positional (Pls) and structural (Sls) errors in F will also be defined for the large scales. To calculate large scale positional and structural errors, we first smooth fields F, Fa, and A with the moving average method, using 5 points as the smoothing parameter. The level of smoothing (over 5 points) was chosen so the lines defined by Fs–$F_{{\rm{a}}}^{\rm{s}} $ and $F_{{\rm{a}}}^{\rm{s}} $ are approximately orthogonal. To ensure orthogonality between large scale positional and large-scale structural errors, Fs–$F_{{\rm{a}}}^{\rm{s}} $, we introduce $F_{{\rm{a}}}^{\rm{s'}} $ (adjusted smoothed aligned forecast) as the point closest to As (see the schematic in Fig. 1). Note that since $F_{{\rm{a}}}^{\rm{s'}} $ lies on a line defined by two smoothed fields (Fs–$F_{{\rm{a}}}^{\rm{s}} $), this field itself is composed of large scales only, without any additional filtering. Figure1. Schematic of a forecast, verifying analysis, and aligned forecast (open black circles) situated in the phase space of full atmospheric variability, shown in 3D here. Smoothed versions of these fields (solid red circles) reside in the subspace of large scale atmospheric variability, represented with a plane. The orthogonally adjusted smoothed aligned forecast (green solid circle) is defined as a point on the Forecast – Aligned Forecast line in the large scale subspace closest to the Analysis. Large scale positional, large scale structural, and small scale error variances are defined as the variance distance between Forecast and Aligned Forecast, and Aligned Forecast and Analysis in the large scale subspace, and the sum of the variance distances between the original and smoothed Analyses, and the original and smoothed Forecasts, respectively. For further discussion, see text.
Large scale positional and structural errors are then defined as Fs–$F_{{\rm{a}}}^{\rm{s'}} $, and $F_{{\rm{a}}}^{\rm{s'}} $–As, respectively. Total error is thus decomposed into three orthogonal components: large scale positional and structural errors and small scale error, the latter of which is orthogonal to the large scale error components as it resides in a different part of the spatial spectrum. Small scale error variance then can be determined either as the difference between total error variance and large scale error variance (i.e., the sum of large scale positional and large scale structural error variance), or as the sum of the differences A–As, and F–Fs.