Flux rope axis geometry of magnetic clouds deduced from in situ data

Magnetic clouds (MCs) consist of flux ropes that are ejected from the low solar corona during eruptive flares. Following their ejection, they propagate in the interplanetary medium where they can be detected by in situ instruments and heliospheric imagers onboard spacecraft. Although in situ measure...

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Detalles Bibliográficos
Autores principales: Janvier, M., Démoulin, P., Dasso, S.
Formato: SER
Materias:
Interplanetary medium
Sun: coronal mass ejections (CMEs)
Sun: magnetic fields
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_17439213_v8_nS300_p265_Janvier
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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