Absence of the strahl during times of slow wind
It is not uncommon during periods when the solar wind speed is less than 425 km s<sup>−1</sup> to observe near 1 AU no evidence of a strahl population in either the electron solar wind or within the foreshock. Estimating the fluid flow within each energy step returned from the Plasma...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
Copernicus Publications
2017-01-01
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| Series: | Annales Geophysicae |
| Online Access: | https://www.ann-geophys.net/35/71/2017/angeo-35-71-2017.pdf |