磁场重联作为一种重要的耀斑触发机制，和耀斑过程中的这些电磁辐射现象有着密切关系。
Magnetic reconnection as an important mechanism to trigger the solar flares is closely related to these electromagnetic radiation phenomena in the course of flares.
上述无力场的触发释能过程可能是太阳耀斑的一种重要的释能机制。
This triggered energy release process is probably an important mechanism for energy release associated with solar flares.
色球压缩区是耀斑大气动力学过程的一个基本特征，是产生色球谱线红不对称性的基础。
The chromospheric condensation is a basic property of the flare dynamical process and the cause of the red asymmetry of chromospheric lines.
应用推荐