A new model-independent method to compute magnetic helicity in magnetic clouds

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Context. Magnetic clouds are transient magnetic structures expulsed from the Sun that travel toward the external heliosphere carrying a significant amount of magnetic flux and helicity. Aims. To improve our understanding of magnetic clouds in relation to their solar source regions, we need a reliabl...

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Detalles Bibliográficos
Autores principales:	Dasso, S., Mandrini, C.H., Démoulin, P., Luoni, M.L.
Formato:	JOUR
Materias:	Interplanetary medium Sun: coronal mass ejections (CMEs) Sun: magnetic fields Magnetic fields Magnetic flux Spacecraft Sun Magnetic cloud boundaries Sun: coronal mass ejections (CME) Astronomy
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00046361_v455_n1_p349_Dasso
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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