Expansion of magnetic clouds in the outer heliosphere
Context. A large amount of magnetized plasma is frequently ejected from the Sun as coronal mass ejections (CMEs). Some of these ejections are detected in the solar wind as magnetic clouds (MCs) that have flux rope signatures. Aims. Magnetic clouds are structures that typically expand in the inner he...
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| Autores principales: | , |
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2012
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v543_n_p_Gulisano http://hdl.handle.net/20.500.12110/paper_00046361_v543_n_p_Gulisano |
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