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. |
|---|---|
| Formato: | CONF |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0094243X_v1216_n_p391_Gulisano |
| Aporte de: |
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