Non-radial solar wind flows induced by the motion of interplanetary coronal mass ejections
A survey of the non-radial flows (NRFs) during nearly five years of interplanetary observations revealed the average non-radial speed of the solar wind flows to be ~30km/s, with approximately one-half of the large (>100km/s) NRFs associated with ICMEs. Conversely, the average non-radial fl...
Main Authors: | , |
---|---|
Format: | Article |
Language: | English |
Published: |
Copernicus Publications
2004-12-01
|
Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/22/4397/2004/angeo-22-4397-2004.pdf |