Magnetic Flux and Helicity of Magnetic Clouds

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Magnetic clouds (MCs) are formed by flux ropes (FRs) launched from the Sun as part of coronal mass ejections (CMEs). They carry away a large amount of magnetic flux and helicity. The main aim of this study is to quantify these amounts from in situ measurements of MCs at 1 AU. The fit of these data b...

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Detalles Bibliográficos
Autores principales:	Démoulin, P., Janvier, M., Dasso, S.
Formato:	JOUR
Materias:	Coronal mass ejections Helicity, magnetic Magnetic fields, interplanetary
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00380938_v291_n2_p531_Demoulin
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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