Expected in situ velocities from a hierarchical model for expanding interplanetary coronal mass ejections
In situ data provide only a one-dimensional sample of the plasma velocity along the spacecraft trajectory crossing an interplanetary coronal mass ejection (ICME). Then, to understand the dynamics of ICMEs it is necessary to consider some models to describe it. We derive a series of equations in a hi...
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Autores principales: | Démoulin, P., Nakwacki, M.S., Dasso, S., Mandrini, C.H. |
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Formato: | JOUR |
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00380938_v250_n2_p347_Demoulin |
Aporte de: |
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