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...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Dasso, S., Milano, L.J., Matthaeus, W.H., Smith, C.W., Velli M., Bruno R., Malara F.
Formato: CONF
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: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

Ejemplares similares

Ejemplares similares