色球耀斑Hα谱线轮廓不对称性研究进展
H α Line Profile Asymmetry in Chromospheric Flare
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 .