Coronal heating by surface Alfvén wave damping: Implementation in a global magnetohydrodynamics model of the solar wind

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The heating and acceleration of the solar wind is an active area of research. Alfvén waves, because of their ability to accelerate and heat the plasma, are a likely candidate in both processes. Many models have explored wave dissipation mechanisms which act either in closed or open magnetic field re...

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Detalles Bibliográficos
Autores principales: Evans, R.M., Opher, M., Oran, R., Van Der Holst, B., Sokolov, I.V., Frazin, R., Gombosi, T.I., Vásquez, A.
Formato: JOUR
Materias:
magnetic fields
magnetohydrodynamics (MHD)
solar wind
Sun: corona
waves
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_0004637X_v756_n2_p_Evans
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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