Cross Helicity Correlations in the Solar Wind

Over the last decade, several magnetohydrodynamic models of the solar wind proposed a two component structure for the fluctuations: a "slab" (Alfvénic) component with wavenumbers parallel to the ambient dc magnetic field and a quasi two-dimensional (turbulent) component with wavenumbers mo...

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Detalles Bibliográficos
Publicado:	2003
Materias:	Magnetohydrodynamics Cross correlations Cross-correlation function DC magnetic field Initial support Magnetohydrodynamic model Three-dimensional correlation Turbulent properties Two-component structures Solar wind
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0094243X_v679_n_p546_Dasso http://hdl.handle.net/20.500.12110/paper_0094243X_v679_n_p546_Dasso
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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