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首页> 外文期刊>Journal of Geophysical Research. Biogeosciences >A STATISTICAL METHOD FOR TESTING A GENERAL CIRCULATION MODEL WITH SPECTRALLY RESOLVED SATELLITE DATA
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A STATISTICAL METHOD FOR TESTING A GENERAL CIRCULATION MODEL WITH SPECTRALLY RESOLVED SATELLITE DATA

机译:用光谱分解的卫星数据检验一般环流模型的统计方法。

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The motivation for this paper is to understand better the means available for testing climate models. Statistics of observed, outgoing, thermal spectra are compared with those predicted from a climate model, on the basis of data collected over a period of approximately 1 year. This is a powerful approach to testing a model with respect to processes internal to the atmosphere. These processes, which have characteristic timescales of less than a year, define the atmosphere's response to external forcing. Second-moment statistics are particularly important fur testing model variability, which is key to predicting the results of forcing the atmosphere, for example, by ocean surface temperature changes, increase of greenhouse gases, etc. Comparisons are presented between statistical data from the infrared interferometer spectrometer (IRIS), an orbiting fourier transform spectrometer, and spectra calculated using the medium-resolution spectral code, MODTRAN, applied to the temperature and humidity profiles from a well-known climate model. Ten months of IRIS data are available, and we have compared means, standard deviations, skew, and kurtosis of its spectrally resolved brightness temperature in three tropical regions for individual months and for a range of timescales. Also presented are comparisons of covariances using Empirical Orthogonal Functions (EOFs) calculated in frequency space. All data that are presented are based on radiance differences from two like spectra, which eliminates many of the errors generated by the use of MODTRAN and most of the errors due to calibration uncertainties in IRIS. Important differences (i.e., residuals) between the IRIS and the GCM statistics are found in comparisons, demonstrating that the spectral data can provide a severe test of many aspects of the variability of a general circulation model. Vile discuss some of the residuals and how they may be used to improve model performance in the context of an adjoint formalism. In the long run the only way to have confidence in the performance of a model is to subject it to as many discriminating comparisons with data as are practicable, and we present a good candidate. [References: 30]
机译:本文的动机是更好地了解可用于测试气候模型的方法。在大约一年的时间内收集的数据的基础上,将观测到的,向外的,热光谱的统计数据与根据气候模型预测的光谱进行比较。这是一种针对大气内部过程测试模型的有效方法。这些过程的时间尺度不到一年,定义了大气层对外部强迫的响应。第二时刻的统计数据是特别重要的毛皮测试模型可变性,这对于预测强迫大气的结果非常关键,例如,通过海洋表面温度变化,温室气体增加等来进行预测。红外干涉仪的统计数据之间进行比较光谱仪(IRIS),一种轨道傅里叶变换光谱仪,并使用中等分辨率的光谱代码MODTRAN计算出的光谱应用于众所周知的气候模型的温度和湿度剖面。可以使用10个月的IRIS数据,并且我们比较了三个热带地区在各个月份和一段时间范围内其光谱解析的亮度温度的均值,标准差,偏度和峰度。还介绍了使用在频率空间中计算的经验正交函数(EOF)进行协方差的比较。呈现的所有数据均基于两个相似光谱的辐射差异,从而消除了使用MODTRAN产生的许多误差以及由于IRIS中的校准不确定性而导致的大多数误差。在比较中发现了IRIS和GCM统计数据之间的重要差异(即残差),这表明光谱数据可以对通用循环模型可变性的许多方面进行严格的检验。 Vile讨论了一些残差以及如何在伴随形式主义的背景下使用它们来改善模型性能。从长远来看,对模型的性能充满信心的唯一方法是,在可行的情况下,对模型进行尽可能多的区分性比较,我们提出了一个不错的选择。 [参考:30]

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