Quantitative model for the generic 3D shape of ICMEs at 1 AU
Context. Interplanetary imagers provide 2D projected views of the densest plasma parts of interplanetary coronal mass ejections (ICMEs), while in situ measurements provide magnetic field and plasma parameter measurements along the spacecraft trajectory, that is, along a 1D cut. The data therefore on...
Guardado en:
Autores principales: | Démoulin, P., Janvier, M., Masías-Meza, J.J., Dasso, S. |
---|---|
Formato: | JOUR |
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00046361_v595_n_p_Demoulin |
Aporte de: |
Ejemplares similares
-
Quantitative model for the generic 3D shape of ICMEs at 1 AU
por: Dasso, Sergio Ricardo
Publicado: (2016) -
Global axis shape of magnetic clouds deduced from the distribution of their local axis orientation
por: Janvier, M., et al.
Publicado: (2013) -
Global axis shape of magnetic clouds deduced from the distribution of their local axis orientation
por: Janvier, M., et al. -
Global axis shape of magnetic clouds deduced from the distribution of their local axis orientation
por: Janvier, M., et al.
Publicado: (2013) -
Global axis shape of magnetic clouds deduced from the distribution of their local axis orientation
por: Dasso, Sergio Ricardo
Publicado: (2013)