Anisotropy in fast and slow solar wind fluctuations
Using 5 years of spacecraft data from near Earth orbit, we investigate the correlation anisotropy of solar wind magnetohydrodynamic-scale fluctuations and show that the nature of the anisotropy differs in fast (>500 km s -1) and slow (<400 km s-1) streams. In particular, fast streams a...
Guardado en:
| Publicado: |
2005
|
|---|---|
| Materias: | |
| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v635_n2II_pL181_Dasso http://hdl.handle.net/20.500.12110/paper_0004637X_v635_n2II_pL181_Dasso |
| Aporte de: |
Ejemplares similares
-
Anisotropy in fast and slow solar wind fluctuations
por: Dasso, S., et al. -
A turbulence-driven model for heating and acceleration of the fast wind in coronal holes
por: Dmitruk, Pablo Ariel
Publicado: (2010) -
A turbulence-driven model for heating and acceleration of the fast wind in coronal holes
por: Verdini, A., et al.
Publicado: (2010) -
A turbulence-driven model for heating and acceleration of the fast wind in coronal holes
por: Verdini, A., et al. -
A turbulence-driven model for heating and acceleration of the fast wind in coronal holes
por: Verdini, A., et al.
Publicado: (2010)