Dynamical evolution of a magnetic cloud from the Sun to 5.4 AU

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Context. Significant quantities of magnetized plasma are transported from the Sun to the interstellar medium via interplanetary coronal mass ejections (ICMEs). Magnetic clouds (MCs) are a particular subset of ICMEs, forming large-scale magnetic flux ropes. Their evolution in the solar wind is comple...

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Detalles Bibliográficos
Autores principales: Nakwacki, M.S., Dasso, S., Démoulin, P., Mandrini, C.H., Gulisano, A.M.
Formato: Artículo publishedVersion
Lenguaje:Inglés
Publicado: 2011
Materias:
Magnetic fields
Magnetohydrodynamics (MHD)
Solar wind
Sun: coronal mass ejections (CMEs)
Sun: heliosphere
Sun: magnetic topology
Cross section
Dynamical evolution
Expansion rate
Flux ropes
Global quantities
Helicities
In-situ observations
Interplanetary coronal mass ejections
Interplanetary medium
Interstellar mediums
Link structure
Magnetic clouds
Magnetic configuration
Magnetic energies
Magnetic flux ropes
Magnetic force
Magnetic-field intensity
Magnetized plasmas
Mass densities
Radial direction
Solar source
Surrounding environment
Velocity profiles
Aspect ratio
Clouds
Expansion
Interplanetary spacecraft
Magnetic flux
Magnetoplasma
Planetary surface analysis
Solar system
Wind
Magnetohydrodynamics
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v535_n_p_Nakwacki
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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