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A consistent thermodynamics of the MHD wave-heated two-fluid solar wind
We start our considerations from two more recent findings in heliospheric physics: One is the fact that the primary solar wind protons do not cool off adiabatically with distance, but appear to be heated. The other one is that secondary protons, embedded in the solar wind as pick-up ions, be...
Wedi'i Gadw mewn:
| Prif Awduron: | , , |
|---|---|
| Fformat: | Artigo |
| Iaith: | Inglês |
| Cyhoeddwyd: |
Copernicus Publications
2003-07-01
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| Cyfres: | Annales Geophysicae |
| Mynediad Ar-lein: | https://www.ann-geophys.net/21/1405/2003/angeo-21-1405-2003.pdf |
| Tagiau: |
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