利用corner transport upwind和constrained transport算法求解非理想磁流体动力学方程组,对匀强平行磁场作用下,黏性各向异性等离子体自由剪切层中的Kelvin-Helmholtz不稳定性进行了数值模拟.从流动结构、涡结构演化、磁场分布、横向...利用corner transport upwind和constrained transport算法求解非理想磁流体动力学方程组,对匀强平行磁场作用下,黏性各向异性等离子体自由剪切层中的Kelvin-Helmholtz不稳定性进行了数值模拟.从流动结构、涡结构演化、磁场分布、横向磁压力、抗弯磁张力等角度对各向同性和各向异性黏性算例结果进行了讨论,分析了黏性各向异性对Kelvin-Helmholtz不稳定性的影响.结果表明,黏性各向异性比黏性各向同性更利于流动的稳定.其稳定性作用是由于磁感线方向上剪切速率降低导致界面卷起程度和圈数的降低,并使卷起结构中小涡产生增殖、合并,破坏了涡的常规增长,从而导致流动的稳定.黏性各向异性对横向磁压力的影响比对抗弯磁张力更大.展开更多
为了探究高背压水介质条件下,固体火箭发动机垂直气体射流在浮力影响下的流场结构和发动机推力特点,建立了轴对称几何模型,在考虑有/无浮力的条件下,采用VOF(Volume of fluid)多相流模型进行气体-水两相耦合仿真计算,获取尾流气体射流...为了探究高背压水介质条件下,固体火箭发动机垂直气体射流在浮力影响下的流场结构和发动机推力特点,建立了轴对称几何模型,在考虑有/无浮力的条件下,采用VOF(Volume of fluid)多相流模型进行气体-水两相耦合仿真计算,获取尾流气体射流流场结构,以及发动机尾部壁面受力和推力振荡曲线进行分析。研究结果表明,考虑浮力的仿真结果更加符合试验结果;射流动量段气体的马赫数分布会导致喷管出口附近的气-水界面产生周期性胀鼓-颈缩,从而引起尾部空间背压振荡,在设计工况下,尾部压力变化范围为环境水深压强的0.327到2.43倍;背压振荡将引起尾壁面受力振荡和推力振荡,振荡频率为736.89Hz;气体射流喷出过程中,气-水界面由速度梯度主导的开尔文-亥姆赫兹(K-H)不稳定性逐渐转变为由重力和浮力主导的瑞利-泰勒(R-T)不稳定性。展开更多
Alfve′n waves(AWs) can play an important role in the macroscopic dynamics as well as in the microscopic wave–particle interaction in various magnetoplasma environments. A very wide observed range of the relative amp...Alfve′n waves(AWs) can play an important role in the macroscopic dynamics as well as in the microscopic wave–particle interaction in various magnetoplasma environments. A very wide observed range of the relative amplitude of magnetic fluctuations of AWs from lower than 10-3in the terrestrial magnetosphere up to *1in the solar wind implies the complexity of saturation mechanisms of AWs. Taking account of the ion-neutral collision damping in a partially ionized plasma, the saturation level of AWs driven by the Kelvin–Helmholtz(K–H) instability is investigated in this paper. The intensified magnetic field due to the excited AWs may result in the saturation of the excited AWs when the growth rate is balanced by the damping rate. An equation determining the saturation level of the AWs is obtained. The results show that, for a fixed-frequency wave, the saturation level of the AWs considerably increases as the ionization degree increases as well as the sheared-flow velocity. On the other hand, for a fixed ionization degree the saturation level of the AWs slightly increases as the plasma b increases but decreases as the wave frequency increases. These results have potential importance for us to estimate the saturation level of AWs in space and astrophysical plasmas.展开更多
文摘利用corner transport upwind和constrained transport算法求解非理想磁流体动力学方程组,对匀强平行磁场作用下,黏性各向异性等离子体自由剪切层中的Kelvin-Helmholtz不稳定性进行了数值模拟.从流动结构、涡结构演化、磁场分布、横向磁压力、抗弯磁张力等角度对各向同性和各向异性黏性算例结果进行了讨论,分析了黏性各向异性对Kelvin-Helmholtz不稳定性的影响.结果表明,黏性各向异性比黏性各向同性更利于流动的稳定.其稳定性作用是由于磁感线方向上剪切速率降低导致界面卷起程度和圈数的降低,并使卷起结构中小涡产生增殖、合并,破坏了涡的常规增长,从而导致流动的稳定.黏性各向异性对横向磁压力的影响比对抗弯磁张力更大.
文摘为了探究高背压水介质条件下,固体火箭发动机垂直气体射流在浮力影响下的流场结构和发动机推力特点,建立了轴对称几何模型,在考虑有/无浮力的条件下,采用VOF(Volume of fluid)多相流模型进行气体-水两相耦合仿真计算,获取尾流气体射流流场结构,以及发动机尾部壁面受力和推力振荡曲线进行分析。研究结果表明,考虑浮力的仿真结果更加符合试验结果;射流动量段气体的马赫数分布会导致喷管出口附近的气-水界面产生周期性胀鼓-颈缩,从而引起尾部空间背压振荡,在设计工况下,尾部压力变化范围为环境水深压强的0.327到2.43倍;背压振荡将引起尾壁面受力振荡和推力振荡,振荡频率为736.89Hz;气体射流喷出过程中,气-水界面由速度梯度主导的开尔文-亥姆赫兹(K-H)不稳定性逐渐转变为由重力和浮力主导的瑞利-泰勒(R-T)不稳定性。
基金supported by the National Natural Science Foundation of China(41304136 and 11373070)Natural Science Foundation of Jiangsu Province(BK20131039)+1 种基金KeyLaboratory of Solar Activity at National Astronomical Observatories,Chinese Academy of Sciences(KLSA201305)the Ministry ofScience and Technology of China(2011CB811402)
文摘Alfve′n waves(AWs) can play an important role in the macroscopic dynamics as well as in the microscopic wave–particle interaction in various magnetoplasma environments. A very wide observed range of the relative amplitude of magnetic fluctuations of AWs from lower than 10-3in the terrestrial magnetosphere up to *1in the solar wind implies the complexity of saturation mechanisms of AWs. Taking account of the ion-neutral collision damping in a partially ionized plasma, the saturation level of AWs driven by the Kelvin–Helmholtz(K–H) instability is investigated in this paper. The intensified magnetic field due to the excited AWs may result in the saturation of the excited AWs when the growth rate is balanced by the damping rate. An equation determining the saturation level of the AWs is obtained. The results show that, for a fixed-frequency wave, the saturation level of the AWs considerably increases as the ionization degree increases as well as the sheared-flow velocity. On the other hand, for a fixed ionization degree the saturation level of the AWs slightly increases as the plasma b increases but decreases as the wave frequency increases. These results have potential importance for us to estimate the saturation level of AWs in space and astrophysical plasmas.
