Energy radiation produced by mass defect can be used to explain some astronomical astronomical phenomena such as the eruption of supernova.
由于其质量亏损而产生的能量辐射可用来解释超新星的爆发等一些天文现象。
In such a situation, mass fraction probability density function model is an appropriate method to approach the reaction phenomena.
在这样情况,许多分数可能性密度函数模型是接近反应现象的一个适当的方法。
The ideal Magnetohydrodynamic equations (MHD), the governing equations of the solar atmosphere dynamical process, are taken to numerically simulate Coronal Mass Ejection (CME) phenomena.
采用理想磁流体力学方程组(MHD)作为太阳大气动力学过程的控制方程组,定性数值模拟日冕物质抛射(CME)现象。
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