论粘性范德瓦耳斯气体中磁流体力学冲击波的结构

IF 0.8 4区 综合性期刊 Q3 MULTIDISCIPLINARY SCIENCES
Sewa Singh, Raj Kumar Anand
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引用次数: 0

摘要

假设气态介质遵循范德华状态方程,建立了一个分析模型来探索存在轴向磁场的一维粘性冲击波的结构。考虑到冲击过渡区域的耗散过程,得到了压力、温度、流体速度和熵的精确解。对冲击前沿结构的详细分析显示了冲击前沿厚度对绝热指数、磁场强度、粘度系数、冲击强度和气体非理想参数的依赖性。研究结果以图形和表格形式显示,冲击前沿厚度随磁场强度和气体粘性系数的增加而增加,而随气体非理想参数值的增加而减小。最后,还比较了根据范德瓦耳斯状态方程得出的当前研究结果和根据阿尼索莫夫和斯宾纳状态方程得出的先前可用数据。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

On the Structure of Magnetohydrodynamics Shock Waves in Viscous van der Waals gases

On the Structure of Magnetohydrodynamics Shock Waves in Viscous van der Waals gases

An analytical model has been developed to explore the structure of one-dimensional viscous shock waves in the presence of an axial magnetic field assuming the gaseous medium to follow the van der Waals equation of state. The exact solutions for pressure, temperature, fluid velocity and entropy are obtained taking into account the dissipative processes in the shock transition region. The detailed analysis of the structure of shock-front has been presented showing the dependence of the thickness of shock-front on the adiabatic index, the strength of magnetic field, coefficient of viscosity, shock strength and the non-idealness parameter of the gases. The findings are presented in graphical as well as in tabular forms which reveal that the shock-front thickness increases with increasing the strength of magnetic field and the viscous coefficient of gases, whereas it decreases with the increasing value of non-idealness parameter of the gases. Finally, a comparison has been done between the current findings following the van der Waals equation of state and the previously available data following the Anisomov and Spiner equation of state.

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来源期刊
CiteScore
2.60
自引率
0.00%
发文量
37
审稿时长
>12 weeks
期刊介绍: To promote research in all the branches of Science & Technology; and disseminate the knowledge and advancements in Science & Technology
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