Dawn-dusk asymmetry in particles of solar wind origin within the magnetosphere
Solar wind/magnetosheath plasma in the magnetosphere can be identified using a component that has a higher charge state, lower density and, at least soon after their entry into the magnetosphere, lower energy than plasma from a terrestrial source. We survey here observations taken over 3 years o...
| Main Authors: | , , , , , , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Copernicus Publications
2001-01-01
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| Series: | Annales Geophysicae |
| Online Access: | https://www.ann-geophys.net/19/1/2001/angeo-19-1-2001.pdf |