Large-scale velocity fluctuations in polar solar wind
The 3-D structure of the solar wind varies dramatically along the Sun's activity cycle. In the present paper we focus on some properties of the polar solar wind. This is a fast, teneous, and steady flow (as compared to low-latitude conditions) that fills the high-latitude heliosphere at low...
| Main Authors: | , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Copernicus Publications
2005-03-01
|
| Series: | Annales Geophysicae |
| Online Access: | https://www.ann-geophys.net/23/1025/2005/angeo-23-1025-2005.pdf |