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, Maria Soledad, Dasso, Sergio Ricardo
Publicado:	2005
Materias:	Magnetic clouds Magnetic helicity Magnetic properties Mathematical models Solar radiation Magnetic materials
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03796566_v_n592_p629_Nakwacki 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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