Evolution of magnetic clouds in the inner heliosphere
Magnetic clouds (MCs) are objects in expansion during their travel through the heliosphere. In situ observations indicate that their front travel faster than their back, showing a clear empirical signature of expansion. With the aim of quantifying the expansion rate of MCs in the inner heliosphere (...
Guardado en:
| Autores principales: | Gulisano, A.M., Démoulin, P., Dasso, S., Ruiz, M.E., Marsch, E. |
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| Formato: | Documento de conferencia publishedVersion |
| Publicado: |
2010
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| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0094243X_v1216_n_p391_Gulisano https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_0094243X_v1216_n_p391_Gulisano_oai |
| Aporte de: |
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