Typical Profiles and Distributions of Plasma and Magnetic Field Parameters in Magnetic Clouds at 1 AU
Magnetic clouds (MCs) are a subset of interplanetary coronal mass ejections (ICMEs). They are important because of their simple internal magnetic field configuration, which resembles a magnetic flux rope, and because they represent one of the most geoeffective types of solar transients. In this stud...
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| Autores principales: | Dasso, Sergio Ricardo, Gulisano, Adriana María |
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| Publicado: |
2016
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| Materias: | |
| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00380938_v291_n7_p2145_Rodriguez http://hdl.handle.net/20.500.12110/paper_00380938_v291_n7_p2145_Rodriguez |
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