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Development and evaluation of a shortwave full-spectrum correlated k-distribution radiative transfer algorithm for numerical weather prediction.

机译:开发和评估用于数值天气预报的短波全谱相关k分布辐射传输算法。

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The Full Spectrum Correlated k-distribution (FSCK) method, originally developed for applications in combustion systems, is adapted for use in shortwave atmospheric radiative transfer. By weighting k-distributions by the solar source function, the FSCK method eliminates the requirement that the Planck function be constant over a spectral interval. Consequently, integration may be carried out across the full spectrum as long as the assumption of correlation from one atmospheric level to the next remains valid. Errors resulting from the lack of correlation across the full spectrum are removed by partitioning the spectrum at a wavelength of 0.68 mum into two bands. The resulting two-band approach in the FSCK formalism requires only 15 quadrature points per atmospheric layer. This represents a 40--90% reduction in computation time relative to existing correlated k-distribution models.; The two-band FSCK approach is developed for general atmospheric conditions through the use of tabulated gas k-values, with nongray cloud absorption coefficients added on-the-fly. A two-part evaluation of the FSCK calculations is presented. First, the two-band FSCK results are compared with line-by-line (LBL) benchmarks alongside results from an earlier radiative transfer model intercomparison study. The median of 24 1-D models included in the intercomparison has a clear-sky mean bias error of -0.27 K/day relative to LBL benchmark heating rates, while the operational FSCK model has a mean bias error of +0.04 K/day. In a second set of calculations, two-band FSCK results are compared with those from six popular state-of-the-art operational and research radiative transfer models. The clear-sky RMS heating rate errors for three empirically-based models range from 0.78 to 6.28 K/day, while RMS errors for three correlated k-distribution models range from 0.85 to 2.83 K/day. For the same clear-sky case the FSCK RMS error is 0.57 K/day. Cloudy-sky cases show that the correlated k-distribution models overestimate in-cloud heating, while the FSCK approach with nongray cloud absorption is closer to the benchmark.
机译:全谱相关k分布(FSCK)方法最初是为燃烧系统开发的,适用于短波大气辐射传输。通过利用太阳能功能对k分布进行加权,FSCK方法消除了普朗克功能在整个光谱区间内保持恒定的要求。因此,只要从一个大气水平到下一个大气水平的相关性假设仍然有效,就可以在整个光谱范围内进行积分。通过将波长为0.68μm的光谱分成两个波段,可以消除由于整个光谱之间缺乏相关性而导致的误差。在FSCK形式主义中产生的两波段方法每个大气层仅需要15个正交点。与现有的相关k分布模型相比,这意味着计算时间减少了40--90%。通过使用表格化的气体k值开发了适用于一般大气条件的两波段FSCK方法,并动态添加了非灰色云的吸收系数。给出了FSCK计算的两部分评估。首先,将两个频段的FSCK结果与逐行(LBL)基准进行比较,并与较早的辐射传输模型比对研究进行比较。相互比较中包含的24个1-D模型的中位数相对于LBL基准加热速率的晴空平均偏差为-0.27 K /天,而运行FSCK模型的平均偏差为+0.04 K /天。在第二组计算中,将两个频段的FSCK结果与六个流行的最新操作和研究辐射传输模型的结果进行了比较。三个基于经验的模型的晴空RMS加热速率误差范围为0.78至6.28 K /天,而三个相关的k分布模型的RMS误差范围为0.85至2.83 K /天。对于相同的晴朗情况,FSCK RMS误差为0.57 K /天。多云的情况表明,相关的k分布模型高估了云中的加热,而具有非灰色云吸收的FSCK方法更接近基准。

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