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

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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Guardado en:
Detalles Bibliográficos
Autor principal: Vasquez, Alberto Marcos
Publicado: 2012
Materias:
magnetic fields
magnetohydrodynamics (MHD)
solar wind
Sun: corona
waves
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v756_n2_p_Evans
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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