带磁场旋转介质中弱不连续性的评估、特征冲击和弱不连续性相互作用

Gorakh Nath, Prakash Upadhyay
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引用次数: 0

摘要

在这篇文章中,我们研究了在轴向磁场下一维(1-D)绝热运动情况下,由偏微分方程(PDEs)系统支配的完美气体旋转介质中的特征冲击波和弱不连续波。我们得到了该偏微分方程系统的几类解析解,它们证明了时空相关性。随着旋转参数、绝热指数和初始磁压与动压之比值的变化,我们详细分析了加速波振幅和跨特征冲击流变量跃迁的影响。我们得到了弱不连续面相互作用后入射波在特征冲击波上引起的冲击加速度跃变、透射波和反射波振幅的表达式。研究发现,跃迁函数跨越了特征冲击衰减效应,在时间 t → ∞ 时归于 0,而弱不连续波可能最终变成冲击波,这取决于初始振幅值。研究还发现,由于考虑到磁场或旋转介质,冲击形成时间会缩短。
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Evaluation of weak discontinuity in rotating medium with magnetic field, characteristic shock and weak discontinuity interaction
In this article we investigated the characteristic shock and weak discontinuity wave in a rotating medium of perfect gas in the case of one-dimensional (1-D) adiabatic motion under an axial magnetic field governed by the system of PDEs (partial differential equations). We have obtained some classes of analytical solutions of the system of PDEs that demonstrates the time-space dependency. With change in the values of rotational parameter, adiabatic index and the ratio of initial magnetic pressure to dynamic pressure, effect on the acceleration wave’s amplitude and jump in the flow variables across the characteristic shock is analyzed in detail. We have obtained an expression for the jump in shock acceleration, the amplitudes of transmitted and reflected waves caused by the incident wave on the characteristic shock after the interaction of a weak discontinuity. It is investigated that the jump function across the characteristic shock decay effect, and goes to 0 as time t → ∞, whereas a weak discontinuity wave may culminate into a shock wave, depending on the initial amplitude value. It is also found that the shock formation time reduces due to the consideration of magnetic field or rotating medium.
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