A turbulence-driven model for heating and acceleration of the fast wind in coronal holes
A model is presented for generation of fast solar wind in coronal holes, relying on heating that is dominated by turbulent dissipation of MHD fluctuations transported upward in the solar atmosphere. Scale-separated transport equations include large-scale fields, transverse Alfvénic fluctuations, and...
Guardado en:
| Autores principales: | Verdini, A., Velli, M., Matthaeus, W.H., Oughton, S., Dmitruk, P. |
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| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_20418205_v708_n2PART2_pL116_Verdini |
| Aporte de: |
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