地球外核处于高温、高压、高密度的等离子体状态，可以支持多种磁流体波的激发和传播。
The outer core of the earth, being in the plasma state with high temperature, high pressure, high density, and immersed in a strong toroidal magnetic field, can support varieties of plasma waves.
本文利用MHD波与日冕大气耦合的磁流体动力学方程组，计算得到冕洞内的日冕大气的温度T、密度N和流速V的分布。
The distributions of. temperature T, density N and velocity V are given using the equations coupling the MHD waves with the coronal atmosphere.
本文研究了磁流体力学与高频等离子体波(包括纵横模式)之间的精巧的相互作用。
The subtle interactions between magnetohydrodynamics and high-frequency plasma waves involving transverse and longitudinal modes are investigated.
磁流体力学数值解析方法，磁流体力学数值模拟方法，非线性波传播及其应用。
Analytic Methods in Magnetohydrodynamics, Numerical Methods in Magnetohydrodynamics, Nonlinear Wave Propagation and Its Applications.
磁流体力学数值解析方法，磁流体力学数值模拟方法，非线性波传播及其应用。
Analytic Methods in Magnetohydrodynamics, Numerical Methods in Magnetohydrodynamics, Nonlinear Wave Propagation and Its Applications.
应用推荐