Heat-flux Instabilities of Regularized Kappa Distributed Strahl Electrons Resolved with ALPS
The fluid behavior of the solar wind is affected by the heat flux carried by the suprathermal electron populations, especially the electron strahl (or beam) that propagates along the magnetic field. In turn, the electron strahl cannot be stable, and in the absence of collisions, its properties are r...
Αποθηκεύτηκε σε:
| Κύριοι συγγραφείς: | , , , |
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| Μορφή: | Artigo |
| Γλώσσα: | Inglês |
| Έκδοση: |
IOP Publishing
2025-01-01
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| Σειρά: | The Astrophysical Journal |
| Θέματα: | |
| Διαθέσιμο Online: | https://doi.org/10.3847/1538-4357/ade0c0 |
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