Causes and consequences of magnetic cloud expansion
Context. A magnetic cloud (MC) is a magnetic flux rope in the solar wind (SW), which, at 1 AU, is observed ∼2-5 days after its expulsion from the Sun. The associated solar eruption is observed as a coronal mass ejection (CME).Aims. Both the in situ observations of plasma velocity distribution and th...
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2009
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Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v498_n2_p551_Demoulin http://hdl.handle.net/20.500.12110/paper_00046361_v498_n2_p551_Demoulin |
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