Global axis shape of magnetic clouds deduced from the distribution of their local axis orientation
Context. Coronal mass ejections (CMEs) are routinely tracked with imagers in the interplanetary space, while magnetic clouds (MCs) properties are measured locally by spacecraft. However, both imager and in situ data do not provide any direct estimation of the general flux rope properties. Aims. The...
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| Autores principales: | Janvier, M., Démoulin, P., Dasso, S. |
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| Formato: | Artículo publishedVersion |
| Publicado: |
2013
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| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00046361_v556_n_p_Janvier https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_00046361_v556_n_p_Janvier_oai |
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