Helicity analysis for expanding magnetic clouds: A case study

Magnetic Clouds (MCs) are the interplanetary counterpart of coronal mass ejections (CMEs). They transport to the interplanetary medium the magnetic flux and helicity released in CMEs by the Sun. At 1 AU from the Sun, MCs are generally modeled as static flux ropes, i.e., considering them as rigid bod...

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Detalles Bibliográficos
Autores principales: Nakwacki, M.S., Dasso, S., Mandrimi, C.H., Demoalin, P.
Formato: CONF
Materias:
Magnetic clouds
Magnetic helicity
Magnetic properties
Mathematical models
Solar radiation
Magnetic materials
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_03796566_v_n592_p629_Nakwacki
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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