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...

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Bibliographic Details
Main Authors: M. Owens, P. Cargill
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