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BGK and MD Simulations of H_2O Supersonic Condensed Jets

机译:H_2O超音速冷凝喷嘴的BGK和MD模拟

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Homogeneous water condensation and ice formation in supersonic expansions to vacuum for stagnation pressures from 12 to 1,000 mbar are studied using the particle-based Ellipsoidal-Statistical Bhatnagar-Gross-Krook (ES-BGK) method. We find that when condensation starts to occur, at a stagnation pressure of 96 mbar, the increase in the degree of condensation causes an increase in the rotational temperature due to the latent heat of vaporization. The simulated rotational temperature profiles along the plume expansion agree well with measurements confirming the kinetic homogeneous condensation models and the method of simulation. Comparisons of the simulated gas and cluster number densities, cluster size for different stagnation pressures along the plume centerline were made and it is found that the cluster size increase linearly with respect to stagnation pressure, consistent with classical nucleation theory. The sensitivity of our results to cluster nucleation model and latent heat values based on bulk water, specific cluster size, or bulk ice are examined. In particular, the ES-BGK simulations are found to be too coarse-grained to provide information on the phase or structure of the clusters formed. For this reason, molecular dynamics simulations of water condensation in a one-dimensional free expansion to simulate the conditions in the core of a plume are performed. We find that the internal structure of the clusters formed depends on the stagnation temperature. A larger cluster of average size 21 was tracked down the expansion, and a calculation of its average internal temperature as well as a comparison of its radial distribution functions (RDFs) with values measured for solid amorphous ice clusters lead us to conclude that this cluster is in a solid-like rather than liquid form. In another molecular-dynamics simulation at a much lower stagnation temperature, a larger cluster of size 324 and internal temperature 200 K was extracted from an expansion plume and equilibrated to determine its RDF and self-diffusion coefficient. The value of the latter shows that this cluster is formed in a supercooled liquid state rather than in an amorphous solid state.
机译:使用基于粒子的椭球统计Bhatnagar-Gross-Krook(ES-BGK)方法研究了超声速膨胀至真空中在12至1,000 mbar的滞止压力下的均相水凝结和冰的形成。我们发现当凝结开始发生时,在96 mbar的停滞压力下,凝结度的增加会由于汽化潜热而导致旋转温度升高。沿羽流膨胀的模拟旋转温度曲线与测量结果吻合良好,从而确定了动力学均相冷凝模型和模拟方法。对沿羽流中心线的不同滞止压力下的模拟气体和簇数密度,簇大小进行了比较,发现簇大小相对于滞止压力呈线性增加,这与经典成核理论一致。检查了我们的结果对团簇形核模型和基于散装水,特定团簇尺寸或散装冰的潜热值的敏感性。特别是,发现ES-BGK模拟的粒度太粗,无法提供有关所形成簇的相或结构的信息。因此,进行了一维自由膨胀中水冷凝的分子动力学模拟,以模拟羽流核心中的条件。我们发现,形成的团簇的内部结构取决于停滞温度。追踪到了一个更大的平均尺寸为21的较大星团,对其平均内部温度的计算以及其径向分布函数(RDFs)与固态无定形冰星团的测量值的比较使我们得出结论,该星团是呈固态而不是液态。在另一个低得多的停滞温度下进行的分子动力学模拟中,从膨胀羽流中提取了尺寸较大的簇324和内部温度200 K,并进行了平衡以确定其RDF和自扩散系数。后者的值表明该团簇以过冷液态而不是非晶态固态形成。

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