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首页> 外文期刊>Journal of Quantitative Spectroscopy & Radiative Transfer >Generalization of the k-moment method using the maximum entropy principle. Application to the NBKM and full spectrum SLMB gas radiation models
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Generalization of the k-moment method using the maximum entropy principle. Application to the NBKM and full spectrum SLMB gas radiation models

机译:使用最大熵原理的k矩方法的推广。在NBKM和全光谱SLMB气体辐射模型中的应用

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摘要

The k-moment method is generalized by applying the maximum entropy principle to get several estimates of the k-distribution function on any kind of spectral interval as a function of the first two moments of the absorption coefficient. Corresponding formulations of the blackbody weighted band averaged transmission function of a gaseous uniform path are obtained. Different constraints involving the first and second order positive, first order negative and logarithmic moments are introduced together with a physical meaning whenever it is possible. Different sets of these constraints are considered to get maximum entropy estimates of the distributions functions: the Dirac, exponential, Gamma, inverse Gaussian and reciprocal inverse Gaussian k-distribution functions. Analytical formulas are provided for each of these distributions and for their associated transmission function, as a function of the mean and variance of the absorption coefficient. The methodology can be applied considering any spectral interval: narrow, wide, the full spectrum, continuous or not. Thus the resulting associated transmission and cumulative k-distribution functions can be utilized in the frame of a large variety of gas radiation models. Hence the k-moment method using the maximum entropy principle is assessed in the frame of the NBKM and full spectrum SLMB gas radiation models. A series of test cases implying comparisons with reference Line-by-Line results exhibits which maximum entropy k-distributions are likely to give the best estimations of narrow band or total emitted intensities, curves-of-growth of the total emission function and full spectrum cumulative k-distribution functions. In particular, the inverse Gaussian and Gamma k-distributions seem most of the time to perform very well.
机译:通过应用最大熵原理来概括k矩方法,以获得在任何种类的光谱区间上作为吸收系数的前两个矩的函数的k分布函数的多个估计。得到了气体均匀路径的黑体加权能带平均传输函数的相应公式。尽可能引入涉及一阶和二阶正,一阶负和对数矩的不同约束以及物理意义。考虑这些约束的不同集合以获取分布函数的最大熵估计:狄拉克(Dirac),指数,伽马,高斯逆函数和倒数高斯逆k分布函数。根据吸收系数的均值和方差,为每个分布及其关联的传递函数提供了分析公式。可以考虑任何光谱间隔来应用该方法:窄,宽,全光谱,连续或不连续。因此,可以在各种气体辐射模型的框架中利用所得的关联的透射和累积k分布函数。因此,在NBKM和全光谱SLMB气体辐射模型的框架中评估了使用最大熵原理的k矩方法。一系列测试案例暗示与参考的逐行结果进行比较,结果表明最大熵k分布可能对窄带或总发射强度,总发射函数的增长曲线和全光谱进行最佳估计累积k分布函数。特别地,逆高斯和伽玛k分布在大多数情况下似乎表现得非常好。

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