The solar wind at solar maximum: comparisons of EISCAT IPS and in situ observations
The solar maximum solar wind is highly structured in latitude, longitude and in time. Coronal measurements show a very high degree of variability, with large variations that are less apparent within in situ spacecraft measurements. Interplanetary scintillation (IPS) observations from EISCAT,...
| Main Authors: | , , , , , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Copernicus Publications
2002-09-01
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| Series: | Annales Geophysicae |
| Online Access: | https://www.ann-geophys.net/20/1291/2002/angeo-20-1291-2002.pdf |