A slow shock-fast magnetosonic wave system formed near the sun evolves into a hybrid shock with an intermediateshock as its necessary component while propagating outward.
Using the method of characteristics and shock fitting techniques, this paper simulates numerically the evolution of MHD (Magnetohydrodynamic) intermediate shocks in interplanetary space.
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。
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