Institut de Mécanique des Fluides de Toulouse (IMFT), Université de Toulouse, CNRS-INPT-UPS, Toulouse, France.
CEA, DEN, Cadarache, SMTA/LPMA, F13108 St Paul lez Durance, France.
Phys Rev E. 2017 Sep;96(3-1):033103. doi: 10.1103/PhysRevE.96.033103. Epub 2017 Sep 11.
We study the effect of an impressing AC magnetic field at the bottom of a liquid metal layer of thickness h. In this situation the fluid is set in motion by the buoyancy forces caused by internal heat sources. The heat sources, caused by the Joule effect induced by the AC field, present an exponentially decaying profile, with characteristic length δ. As the magnetic field is horizontal, the Lorentz force has no influence on the dynamics of the system since it contributes only to the magnetic pressure. We propose an analysis of both the transient and fully developed regimes using linear stability analysis (LSA) and direct numerical simulations (DNSs). The transient period is governed by the temporal evolution of the temperature field as well as the development of the convective instability, which can be concomitant and therefore requires adopting a transient LSA algorithm to track these two effects. The DNSs have been performed for various distributions of the heat sources and various total heat input. This corresponds to independently varying δ/h in the range 0.04≤δ/h≤0.45 and a Rayleigh number 1.1×10^{4}≤Ra≤1.2×10^{5}. We observe the relaxation of the temperature up to the steady conductive profile before the transition to the nonlinear regime when Ra is small, whereas for larger Ra, nonlinear effects appear during the relaxation of the temperature profile. The unsteadiness of the temperature field significantly alters the development of the instability because of a much smaller growth rate. Surprisingly, we observe that δ/h has only a limited influence on averaged quantities as well as on the patterns for both the linear and nonlinear regimes. This comes with the fact that the profiles present an apparent reflectional symmetry, despite the asymmetry of the governing equations.
我们研究了在厚度为 h 的液态金属层底部施加交流磁场的影响。在这种情况下,由于内部热源引起的浮力,流体被带动。热源由交流场引起的焦耳效应产生,呈指数衰减分布,特征长度为 δ。由于磁场是水平的,洛伦兹力对系统的动力学没有影响,因为它只贡献磁压力。我们使用线性稳定性分析(LSA)和直接数值模拟(DNS)对瞬态和充分发展两种情况进行了分析。瞬态阶段由温度场的时间演化以及对流不稳定性的发展来控制,这两种效应可能同时出现,因此需要采用瞬态 LSA 算法来跟踪这两种效应。DNS 已经针对不同的热源分布和不同的总热量输入进行了模拟。这对应于独立地改变 δ/h 的范围为 0.04≤δ/h≤0.45 和瑞利数 1.1×10^{4}≤Ra≤1.2×10^{5}。我们观察到温度在过渡到非线性阶段之前,在 Ra 较小时会达到稳定的热传导分布,而在 Ra 较大时,非线性效应会在温度分布的弛豫过程中出现。温度场的非稳态会显著改变不稳定性的发展,因为增长率小得多。令人惊讶的是,我们发现 δ/h 对线性和非线性两种情况下的平均量和模式只有有限的影响。这是因为尽管控制方程存在不对称性,但分布呈现出明显的反射对称。