Magnetic cloud models with bent and oblate cross-section boundaries
Context. Magnetic clouds (MCs) are formed by magnetic flux ropes that are ejected from the Sun as coronal mass ejections. These structures generally have low plasma beta and travel through the interplanetary medium interacting with the surrounding solar wind. Thus, the dynamical evolution of the int...
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2009
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v507_n2_p969_Demoulin http://hdl.handle.net/20.500.12110/paper_00046361_v507_n2_p969_Demoulin |
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