摘要
白光耀斑是第22周太阳活动峰年的一个重要研究课题.本文扼要地探讨了白光耀斑的研究近况,针对目前尚未解决的白光耀斑连续发射起源问题,提出了色球凝聚可能对应产生白光连续辐射增强的新观点.
White-light flare is one of the most important research topics in the nearly coming 22nd peak years of solar activity. In this research note, after a brief review of current studies on white-light flares. we propose tentatively that the chromospheric condensation may be the best candidate responsible for the continuum emission of white-light flares. It is also predicted that in the eve of continuum emission, Hα line profile may be reversed with blue asymmetry.
出处
《天文学报》
CSCD
北大核心
1990年第1期94-96,共3页
Acta Astronomica Sinica
