日冕物质抛射和太阳表面磁活动的关系  

Correlation Between Coronal Mass Ejections and Solar Surface Magnetic Activities

作　　者：周桂萍[1] 曹卓良[1] 汪景琇[2] 

机构地区：[1]安徽大学物理系,合肥230039 [2]中国科学院国家天文台,北京100012

出　　处：《天文学进展》2003年第1期41-54,共14页Progress In Astronomy

摘　　要：综述了近年来日冕物质抛射与耀斑、日珥、冕流和日冕暗化相关关系的研究进展,指出了这些相关关系上的一些不确定因素。同时,介绍了我们所做的部分工作,探讨了不同尺度磁活动之间的物理联系,并提出今后需要进一步解决的问题。This paper mainly overviews the recent progress on the relationship between Coronal mass ejections (CMEs) and flares, prominences, coronal streamers or coronal dimming. It points out some uncertain factors in such correlation studies. A part of the authors' work is introduced and some physical links among different scale magnetic activities are discussed. Finally, some important questions, which need to be resolved further, are presented.

关 键 词：日冕物质抛射 太阳表面磁活动 耀斑 日珥 冕流 

分 类 号：P182.6[天文地球—天文学] P182.7