Coronal mass ejections

被引：0

作者：

Gosling, JT ^{[1
]}

机构：

[1] Los Alamos Natl Lab, Los Alamos, NM 87545 USA

来源：

26TH INTERNATIONAL COSMIC RAY CONFERENCE | 2000年 / 516卷

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：

The most dramatic changes in the solar,corona occur during coronal mass ejections, or CMEs, during which solar material is propelled outward into the heliosphere from regions in the corona not previously participating in the solar wind expansion. These ejections often produce major solar wind disturbances, targe geomagnetic storms, enhancements of moderate energy (MeV) particle fluxes and decreases in the galactic cosmic ray particle flux. This paper provides an overview of the CME phenomenon with emphasis on the CMEs themselves and how they evolve as they propagate out through the heliosphere.

引用

页码：59 / 79

页数：5

共 58 条

[1] HOW MUCH ENERGY CAN BE STORED IN A 3-DIMENSIONAL FORCE-FREE MAGNETIC-FIELD [J].