Evolution of shock waves in dusty nonideal gas flow with magnetic field

Shweta, Pradeep, S. Srivastava, L. P. Singh
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Abstract

This paper deals with the study of propagation of shock waves in 2-D steady supersonic magnetogasdynamics flow of nonideal dusty gas using wavefront analysis method. We derived the transport equation, which determines the condition for the shock formation. Our aim is to analyze the effect of interaction of dust particles with magnetic field in nonideal gas on the evolution of shock formation and to examine how the flow patterns of the disturbance vary with respect to the variations in the physical parameters of the medium. It is found that the presence of magnetic field plays an essential role in the wave propagation phenomena. The nature of the solution with respect to the Mach number is analyzed, and it is examined how the shock formation distance changes with an increase or decrease in the value of Mach number. Also, the combined effect of nonidealness, magnetic field, and dust particles on the shock formation distance is elucidated and examined how the formation of shocks is affected by the increase in the value of corresponding physical parameters.
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尘埃状非理想气体流中的冲击波随磁场的演变
本文利用波前分析方法研究了冲击波在非理想含尘气体的二维稳定超音速磁气动力流中的传播。我们导出了决定冲击形成条件的传输方程。我们的目的是分析非理想气体中尘埃粒子与磁场的相互作用对冲击形成演化的影响,并研究扰动的流动模式如何随介质物理参数的变化而变化。研究发现,磁场的存在对波的传播现象起着至关重要的作用。分析了与马赫数有关的解的性质,并研究了冲击形成距离如何随马赫数值的增减而变化。此外,还阐明了非理想性、磁场和尘埃粒子对冲击形成距离的综合影响,并研究了冲击的形成如何受到相应物理参数值增加的影响。
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