Magnetohydrodynamic(MHD) equations are important models for the fluid's dynamics theory in the plasma.MHD models for the initial stages of solar flares are considered in this paper.%MHD方程组是来解释耀斑的复杂特性的等离子体流体动力学理论的重要模型.为此,主要通过太阳耀斑初期阶段的MHD模型来讨论耀斑的一些特征.
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