本文讨论磁流体中间激波的相互作用规律。
This paper discusses the interaction between MHD intermediate shocks.
本文采用特征线方法和激波装配法，对磁流体中间激波在行星际空间的演化过程进行数值模拟。
Using the method of characteristics and shock fitting techniques, this paper simulates numerically the evolution of MHD (Magnetohydrodynamic) intermediate shocks in interplanetary space.
太阳附近形成的慢激波-快磁声波系统，将在向外传播的过程中演变为以中间激波作为必要组成部分的混合激波。
A slow shock-fast magnetosonic wave system formed near the sun evolves into a hybrid shock with an intermediate shock as its necessary component while propagating outward.
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