I. INTRODUCTION It has been recognized since the 1940s that flare emission lines are usually asymmetric. Svestka summarized in his book the spectral observations before the 1970s. His main resuits are as follows: (ⅰ)...I. INTRODUCTION It has been recognized since the 1940s that flare emission lines are usually asymmetric. Svestka summarized in his book the spectral observations before the 1970s. His main resuits are as follows: (ⅰ) for most flares, a short-lived blue asymmetry appears at the flare on-展开更多
基金Project supported by the National Natural Science Foundation of China
文摘I. INTRODUCTION It has been recognized since the 1940s that flare emission lines are usually asymmetric. Svestka summarized in his book the spectral observations before the 1970s. His main resuits are as follows: (ⅰ) for most flares, a short-lived blue asymmetry appears at the flare on-