Investigating the observational signatures of magnetic cloud substructure
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...
Guardado en:
| Publicado: |
2011
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_21699402_v116_n1_p_Steed http://hdl.handle.net/20.500.12110/paper_21699402_v116_n1_p_Steed |
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