Nonlocal heat transport in the solar wind
It is shown that a nonlocal, suprathermal tail originated near the solar corona base dominates the conductive energy flux at distances r ≥: 2 R ⊙ . A nonlocal analytical expression for the electron heat flux in weakly collisional plasmas is derived by solving the Fokker-Planck equation...
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| Autores principales: | Canullo, M.V., Costa, A., Ferro-Fontán, C. |
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| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v462_n2PARTI_p1005_Canullo |
| Aporte de: |
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