Investigating the observational signatures of magnetic cloud substructure

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Magnetic clouds (MCs) represent a subset of interplanetary coronal mass ejections (ICMEs) that exhibit a magnetic flux rope structure. They are primarily identified by smooth, large-scale rotations of the magnetic field. However, both small- and large-scale fluctuations of the magnetic field are obs...

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Autores principales: Steed, K., Owen, C.J., Démoulin, P., Dasso, S.
Formato: JOUR
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_21699402_v116_n1_p_Steed
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Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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