EISCAT measurements of the solar wind
EISCAT observations of interplanetary scintillation have been used to measure the velocity of the solar wind at distances between 15 and 130 R<sub>⊙</sub> (solar radii) from the Sun. The results show that the solar wind consists of two distinct components, a fast stream wi...
| Main Authors: | , , , , , , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Copernicus Publications
1996-12-01
|
| Series: | Annales Geophysicae |
| Online Access: | https://www.ann-geophys.net/14/1235/1996/angeo-14-1235-1996.pdf |