Global axis shape of magnetic clouds deduced from the distribution of their local axis orientation

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Context. Coronal mass ejections (CMEs) are routinely tracked with imagers in the interplanetary space, while magnetic clouds (MCs) properties are measured locally by spacecraft. However, both imager and in situ data do not provide any direct estimation of the general flux rope properties. Aims. The...

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Detalles Bibliográficos
Autores principales: Janvier, M., Démoulin, P., Dasso, S.
Formato: JOUR
Materias:
Magnetic fields
Solar-terrestrial relations
Sun: coronal mass ejections (CMEs)
Sun: heliosphere
Coronal mass ejection
High-energy particles
Orientation distributions
Space weather forecast
Statistical distribution
Sun: coronal mass ejection
Rope
Solar system
Weather forecasting
Interplanetary spacecraft
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v556_n_p_Janvier
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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