磁声波是一种磁流体力学波，在磁声波中，磁压力和等离子体的热压力同时起作用。
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而在赤道附近，传播扰动是快模磁声波，在源区附近还存在一非传播的扰动。
Whereas in the vicinity of solar equator, propagating disturbance is regarded as fast mode wave, and a standing disturbance is found to be located near the source region.
结果表明，在极区，压力脉冲导致的扰动传播可以区分成两类不同模式的波动；快磁声波与慢磁声波。
Numerical results indicate that, in polar region, propagating disturbances can be distinguished into two modes, i. e. fast and slow magneto-acoustic waves.
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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