论文标题
在重力分层等温培养基中声波传播的两流体建模
Two-fluid Modeling of Acoustic Wave Propagation in Gravitationally Stratified Isothermal Media
论文作者
论文摘要
为了研究部分电离等离子体中的声波传播和相应的能量沉积,我们使用了两种流体的计算模型,将中性颗粒(电子和离子)视为两个独立的流体。这个两流体模型考虑了离子中性的碰撞,电离和重组,使我们能够研究等离子体中未偶联离子和中性的碰撞和反应性相互作用。在当前的数值模拟中,指定初始密度达到静水平衡,并且为了进行比较,还考虑了化学平衡,以提供与典型的静水压平衡曲线不同的密度曲线。然后施加外部速度驱动器以产生单色声波。众所周知,由于密度呈指数降低,向上传播的声波在重力分层的等离子体中陡峭,并且它们在非线性方案中加热了等离子体,在非线性状态下,在激波波和碰撞相互作用中动力学消散。特别是,由于当前初始化学平衡而产生的较低的电离分数显着提高了加热效率。此外,电离过程吸收了大量的能量,并且在考虑电离和重组时也增强了离子和中性之间的脱钩。因此,在不考虑电离和重组的情况下进行的模拟可能高估了整体加热效应,但也低估了能量耗散。结果还表明,更准确的电离和重组模型对于改善部分电离等离子体的建模至关重要。
To study acoustic wave propagation and the corresponding energy deposition in partially ionized plasmas, we use a two-fluid computational model that treats neutrals and charged particles (electrons and ions) as two separate fluids. This two-fluid model takes into account the ion-neutral collisions, ionization, and recombination, allowing us to investigate both the collisional and reactive interactions between uncoupled ions and neutrals in the plasmas. In the present numerical simulations, the initial density is specified to reach hydrostatic equilibrium, and as a comparison, chemical equilibrium is also taken into account to provide a density profile that differs from typical hydrostatic equilibrium profiles. External velocity drivers are then imposed to generate monochromatic acoustic waves. As is well known, the upward propagating acoustic waves steepen in gravitationally stratified plasmas due to the exponentially decreasing density, and they heat the plasmas in the nonlinear regimes where kinetic energy is dissipated by shock waves and collisional interactions. In particular, the lower ionization fraction resulting from the present initial chemical equilibrium significantly enhances the heating efficiency. Moreover, the ionization process absorbs a significant amount of energy, and the decoupling between ions and neutrals is also enhanced while considering ionization and recombination. Therefore, simulations without considering ionization and recombination may overestimate the overall heating effects but also underestimate the energy dissipation. The results also suggest that a more accurate ionization and recombination model could be essential for improving the modeling of partially ionized plasmas.