Expansion of magnetic clouds in the outer heliosphere

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Context. A large amount of magnetized plasma is frequently ejected from the Sun as coronal mass ejections (CMEs). Some of these ejections are detected in the solar wind as magnetic clouds (MCs) that have flux rope signatures. Aims. Magnetic clouds are structures that typically expand in the inner he...

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Detalles Bibliográficos
Autores principales: Gulisano, A.M., Démoulin, P., Dasso, S., Rodriguez, L.
Formato: Artículo publishedVersion
Lenguaje:Inglés
Publicado: 2012
Materias:
Interplanetary medium
Magnetic fields
Magnetohydrodynamics (MHD)
Solar wind
Sun: coronal mass ejections (CMEs)
Astronomical units
Coronal mass ejection
Expansion properties
Expansion rate
Flux ropes
Heliospheres
In-situ
Linear functions
Linear velocity
Magnetic clouds
Magnetized plasmas
Mean magnetic field
Minimum variance
Outer heliosphere
Plasma measurement
Plasma parameter
Power-law
Self-similar
Strong field
Sun: coronal mass ejection
Temporal evolution
Ulysses spacecraft
Velocity profiles
Magnetohydrodynamics
Magnetoplasma
Rope
Solar system
Velocity
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v543_n_p_Gulisano
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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