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Comparison of Wide Band, Narrow Band, and SLW Models with HITRAN and HITEMP for Predicting Radiative Heat Transfer

机译:宽带,窄带和SLW模型与HITRAN和HITEMP的预测辐射热传递的比较

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Accurate modeling of radiative heat transfer is critical to atmospheric science applications, as well as propulsion systems, including combustion chambers and rocket plumes. The objectives of this study are to: (1) predict radiative heat transfer using the wide band, narrow band, and global property models, and (2) compare the results obtained with those from line-by-line (LBL) simulations performed using HITRAN and HITEMP databases. The five radiative property models considered in the current study are the Exponential Wide Band Model (EWBM), Spectrally-Resolved Exponential Wide Band Model (SR-EWBM), Elsasser Narrow Band Model (Elsasser NBM), Malkmus Narrow Band Model (Malkmus NBM), and the Spectral Line Weighted-Sum-of-Gray-Gases (SLW) model. The problem considered consists of a non-gray, one-dimensional (1-D) enclosure containing H_2O with uniform temperature and species mass fraction. The radiative transfer equation (RTE) was solved using the Discrete Ordinates Method (DOM). First, the spectral absorption coefficients computed from these models are compared with the LBL data obtained using the HITRAN and HITEMP databases. The effects of varying the medium temperature and pressure, as well as the wall temperature, on the model predictions of radiative heat flux and its divergence are studied through comparison with the corresponding data obtained using HITRAN and HITEMP. For all of the medium temperatures and pressures considered, the SLW model predictions showed excellent agreement and Malkmus NBM showed reasonable agreement with the HITEMP data. At lower temperatures (and at constant pressure), the two wide band models and the Elsasser NBM showed reasonable agreement with HITEMP. At high temperatures (and at constant pressure), the SR-EWBM and the Elsasser NBM showed poor agreement with HITEMP. At low pressures (and at constant temperature), the two wide band models and the Elsasser NBM showed reasonable agreement with HITEMP. However, at high pressures, the EWBM showed poor agreement with HITEMP. Finally, we investigate DOM for a variety of cases, including isothermal, homogeneous, non-isothermal, inhomogeneous, and mixture cases for HITRAN and HITEMP. Two-dimensional domains, as well as additional spatial inhomogeneities in temperature and species concentrations, will also be considered in the near future.
机译:辐射传热的精确模型对于大气科学应用以及包括燃烧室和火箭羽流在内的推进系统至关重要。这项研究的目的是:(1)使用宽带,窄带和全局属性模型预测辐射热传递,以及(2)将使用线对线(LBL)模拟获得的结果进行比较HITRAN和HITEMP数据库。当前研究中考虑的五个辐射特性模型是指数宽带模型(EWBM),光谱分辨指数宽带模型(SR-EWBM),Elsasser窄带模型(Elsasser NBM),Malkmus窄带模型(Malkmus NBM) ,以及光谱线加权总和灰色气体(SLW)模型。所考虑的问题包括一个非灰色的一维(1-D)外壳,该外壳包含温度和物种质量分数均一的H_2O。使用离散纵坐标方法(DOM)求解了辐射传递方程(RTE)。首先,将从这些模型计算出的光谱吸收系数与使用HITRAN和HITEMP数据库获得的LBL数据进行比较。通过与使用HITRAN和HITEMP获得的相应数据进行比较,研究了介质温度和压力以及壁温的变化对辐射热通量及其散度模型预测的影响。对于所考虑的所有中等温度和压力,SLW模型的预测显示出极好的一致性,而Malkmus NBM与HITEMP数据显示出合理的一致性。在较低的温度(和恒定压力)下,两个宽带模型和Elsasser NBM与HITEMP表现出合理的一致性。在高温(和恒定压力)下,SR-EWBM和Elsasser NBM与HITEMP的一致性较差。在低压(和恒温)下,两个宽带模型和Elsasser NBM与HITEMP表现出合理的一致性。但是,在高压下,EWBM与HITEMP的一致性差。最后,我们研究DOM的各种情况,包括HITRAN和HITEMP的等温,均相,非等温,不均匀和混合情况。在不久的将来,还将考虑二维域以及温度和物种浓度的其他空间不均匀性。

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