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。
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。
Simulation results show that heat pipe receiver lightens system mass, improves heat efficiency of system and avoids phenomena of heat spot and heat relaxing.
模拟结果表明,热管吸热器减轻了系统的质量,提高了系统的热效率,并能避免热斑和热松脱现象。
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