Magnetic cloud models with bent and oblate cross-section boundaries

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Context. Magnetic clouds (MCs) are formed by magnetic flux ropes that are ejected from the Sun as coronal mass ejections. These structures generally have low plasma beta and travel through the interplanetary medium interacting with the surrounding solar wind. Thus, the dynamical evolution of the int...

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Guardado en:
Detalles Bibliográficos
Autores principales: Démoulin, P., Dasso, S.
Formato: Artículo publishedVersion
Lenguaje:Inglés
Publicado: 2009
Materias:
Interplanetary medium
Sun: coronal mass ejections (CMEs)
Sun: magnetic fields
Arbitrary cross section
Boundary shapes
Coronal mass ejection
Cylindrical models
Cylindrical symmetry
Dynamical evolution
Field strengths
Flux ropes
Global quantities
Helicities
In-situ data
In-situ observations
Internal structure
Large anisotropy
Magnetic clouds
Magnetic configuration
Magnetic field orientations
Magnetic field profile
Magnetic field strengths
Magnetic flux ropes
Magnetic models
Minimum variance
Solar source
Sun: coronal mass ejection
Sun: magnetic field
Theoretical models
Time evolutions
Total pressure
Aspect ratio
Astrophysics
Boundary layer flow
Interplanetary spacecraft
Magnetic fields
Magnetic flux
Magnetic structure
Planetary surface analysis
Solar wind
Sun
Semiconductor counters
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v507_n2_p969_Demoulin
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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