Does spacecraft trajectory strongly affect detection of magnetic clouds?

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Context. Magnetic clouds (MCs) are a subset of interplanetary coronal mass ejections (ICMEs). One property of MCs is the presence of a magnetic flux rope. Is the difference between ICMEs with and without MCs intrinsic or rather due to an observational bias? Aims. As the spacecraft has no relationshi...

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Detalles Bibliográficos
Autores principales: Démoulin, P., Dasso, S., Janvier, M.
Formato: Artículo publishedVersion
Publicado: 2013
Materias:
Magnetic fields
Solar-terrestrial relations
Sun: coronal mass ejections (CMEs)
Sun: heliosphere
Affect detection
Boundary shapes
Current distribution
Decreasing functions
Flux rope model
Flux ropes
Force free fields
Frequency distributions
Heliospheres
Impact-parameter
Interplanetary coronal mass ejections
Large parts
Low field
Magnetic clouds
Magnetic flux ropes
Natural consequences
Non-detection
Parameter spaces
Rotation angles
Spacecraft trajectories
Sun: coronal mass ejection
Uniform distribution
Aspect ratio
Computer simulation
Magnetic flux
Planetary surface analysis
Spacecraft
Trajectories
Parameter estimation
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v550_n_p_Demoulin
https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_00046361_v550_n_p_Demoulin_oai
Aporte de:
Repositorio Digital de la Universidad de Buenos Aires (UBA) de Universidad de Buenos Aires

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