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首页> 外文期刊>ournal of the Meteorological Society of Japan >Normal-Mode Energetics Analysis and the Intercomparison for the Recent ECMWF, NMC, and JMA Global Analyses
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Normal-Mode Energetics Analysis and the Intercomparison for the Recent ECMWF, NMC, and JMA Global Analyses

机译:正态模式能量学分析和最近ECMWF,NMC和JMA Global分析的比对

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In this study, normal-mode energetics diagnosis was carried out for the 9-year period of ECMWF (European Center for Medium-Range Weather Forecasts) analysis during winters (DJF) of 1986 to 1994. The diagnosis was performed also for operational global analyses by JMA (Japan Meteorological Agency) and NMC (National Meteorological Center) during the winter of 1988/89 for comparison. Special attention is focussed on the total energy spectra for Rossby and gravity modes over the 3-D scale index. The result was compared with our former studies for other datasets, including original and re-analyses of the First GARP Global Experiment (FGGE). The result for the 9-year average of ECMWF shows that the slopes of the Rossby-mode energy spectra in the eigenfrequency domain are estimated as 2.2, 2.1, 3.5, 5.0, 5.5 for vertical modes m=0 to 4, respectively, whereas the corresponding slopes are -1.8, -1.7, -1.6, -1.3, -1.0, respectively, for the gravity mode. We confirm that the energy spectra of Rossby and gravity modes are connected with each other in the high-frequency range, at least for the vertical modes m=1 to 4. However, the mechanism to create the spectral peaks within the Rossby modes is not known. The intercomparison of the normal-mode energetics for JMA, NMC, and ECMWF shows that the Rossby-mode energy levels are virtually the same, having a minor discrepancy less than 8%. We find that the total energy level pertaining to the gravity modes is about 45 (1O3 Jm-2) and shows a minor discrepancy of only about 8% between the analyses. According to our former studies for the FGGE reanalyses, the corresponding energy levels for the gravity modes are 90 and 41 (103 Jm-2) for GFDL and ECMWF, respectively. Hence, we can conclude that the total energy levels of the gravity modes in the recent operational analyses are converging to the value of ECMWF FGGE data. Since the amount of the total energy of the atmosphere is about 6800 (103 Jm-2), the energy level of the gravity mode is found to be only 0.7% of the total energy.
机译:在这项研究中,对1986年至1994年冬季(DJF)的ECMWF(欧洲中距离天气预报中心)分析进行了为期9年的正常模式能量诊断。由JMA(日本气象厅)和NMC(国家气象中心)在1988/89年冬季进行比较。特别注意的是在3-D比例指数上的Rossby模式和重力模式的总能谱。将该结果与我们先前对其他数据集的研究进行了比较,包括首次GARP全球实验(FGGE)的原始和重新分析。 ECMWF的9年平均值的结果表明,对于垂直模式m = 0到4,本征频域中的Rossby模式能谱的斜率分别估计为2.2、2.1、3.5、5.0、5.5。对于重力模式,相应的斜率分别为-1.8,-1.7,-1.6,-1.3,-1.0。我们确认,至少对于垂直模式m = 1到4,Rossby模式和重力模式的能谱在高频范围内相互连接。但是,在Rossby模式内创建谱峰的机制并不完全众所周知。 JMA,NMC和ECMWF的正常模式能量学之间的比较表明,Rossby模式的能量水平实际上是相同的,差异仅小于8%。我们发现,与重力模式有关的总能级约为45(1O3 Jm-2),分析之间的细微差异仅为8%。根据我们以前对FGGE重新分析的研究,GFDL和ECMWF的重力模式相应的能级分别为90和41(103 Jm-2)。因此,我们可以得出结论,在最近的运行分析中,重力模式的总能级正在收敛到ECMWF FGGE数据的值。由于大气的总能量约为6800(103 Jm-2),因此重力模式的能级仅为总能量的0.7%。

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