论文标题
属于Beltrami流量的三维衰减磁场
Three-dimensional decaying magnetic field belonging to Beltrami flow
论文作者
论文摘要
这项研究分析了在应用磁场下的三维泰勒衰减涡流作为基准测试问题,以验证电磁流体流量的计算方法,并研究了衰减磁场模型的有效性。首先,我们观察到没有施加磁场的三维泰勒腐烂涡流的流量结构。当网格点的数量和雷诺数变化时,我们研究了计算结果与精确解决方案之间误差的变化,并显示了基准测试的有效性。接下来,我们在应用磁场下分析了三维泰勒腐烂的涡旋,并阐明了衰减磁场的特征。当应用磁场时,低磁压区域以网格模式连接,并且具有扭曲的立方结构的磁压分布围绕着高磁性压力区域。在停滞区域中,磁能变低,磁通线与速度场的流线相似。高电流密度以网格模式出现,磁通量线在高电流密度区域周围旋转。高电流密度区域中的磁压力和磁能很高。当雷诺数和磁性雷诺数变化时,各种能量的衰减趋势与精确的解决方案非常吻合。向湍流的过渡发生在较高的雷诺数,动力学和总能量迅速减少。动能的耗散速率最大化后,涡流结构衰减,流场接近没有磁场的固定状态。属于Beltrami流的三维泰勒衰减磁场是验证电磁流体流量计算方法的有价值模型。
This study analysed a three-dimensional Taylor decaying vortex under an applied magnetic field as a benchmark test problem to verify the calculation method of an electromagnetic fluid flow and investigated the validity of the decaying magnetic field model. First, we observed the flow structure of a three-dimensional Taylor decaying vortex without an applied magnetic field. We investigated the changes in the error between the calculation result and the exact solution when the number of grid points and the Reynolds number varied and showed the effectiveness of the benchmark test. Next, we analysed a three-dimensional Taylor decaying vortex under an applied magnetic field and clarified the characteristics of the decaying magnetic field. When a magnetic field is applied, low magnetic pressure regions are connected in a mesh pattern, and the magnetic pressure distribution with a distorted cubic structure occurs to surround a high magnetic pressure region. In a stagnation region, the magnetic energy becomes low, and the magnetic flux line is similar to the streamline of the velocity field. High current densities occur in a grid pattern, and the magnetic flux lines swirl around the high current density region. The magnetic pressure and magnetic energy are high in the high current density region. When the Reynolds number and the magnetic Reynolds number vary, the decay trends of various energies agree well with the exact solution. The transition to turbulent flow occurs at a high Reynolds number, and the kinetic and total energies decrease rapidly. After the dissipation rate of kinetic energy becomes maximum, the vortex structure decays, and the flow field approaches a stationary state without magnetic fields. The three-dimensional Taylor decaying magnetic field belonging to the Beltrami flow is a valuable model for verifying the calculation method of electromagnetic fluid flows.