Phenomenology of coronal mass ejections

被引：0

作者：

Mogilevsky, EI ^{[1
]}

Obridko, VN ^{[1
]}

Shilova, NS ^{[1
]}

机构：

[1] Russian Acad Sci, Inst Terr Magnetism Ionosphere & Radiowave Propag, Troitsk 142092, Moscow Oblast, Russia

来源：

ASTRONOMY REPORTS | 1999年 / 43卷 / 04期

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

An attempt to describe the phenomenology of solar coronal mass ejections (CMEs) at all wavelength bands is undertaken. The development of several typical CMEs in 1996 and 1997 is considered in detail. Among the properties revealed, we especially emphasize (1) the presence of initial eruption prominences that are relatively distant from each other, (2) the development of CMEs from two eruption sites, and (3) the connection of CMEs with structural evolution, i.e., large-scale solar-activity complexes. In addition to determining the basic properties of CMEs, we compare scenarios for CMEs and hares and search for common features in the natures of these phenomena, which have very different temporal and spatial scales. A qualitative model for the above phenomena is put forward.

引用

页码：255 / 266

页数：12