Comparing generic models for interplanetary shocks and magnetic clouds axis configurations at 1 AU
Interplanetary coronal mass ejections (ICMEs) are the manifestation of solar transient eruptions, which can significantly modify the plasma and magnetic conditions in the heliosphere. They are often preceded by a shock, and a magnetic flux rope is detected in situ in a third to half of them. The mai...
Guardado en:
Autores principales: | Janvier, M., Dasso, S., Démoulin, P., Masías-Meza, J.J., Lugaz, N. |
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Formato: | INPR |
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_21699380_v_n_p_Janvier |
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