Materias dentro de su búsqueda.
Materias dentro de su búsqueda.
Interplanetary spacecraft
Magnetic fields
16
Solar wind
12
Solar system
10
Sun: coronal mass ejections (CMEs)
10
Sun: heliosphere
10
Astrophysics
9
Coronal mass ejection
9
Interplanetary medium
9
Magnetic flux
9
High-energy particles
7
Interplanetary coronal mass ejections
7
Solar-terrestrial relations
7
Sun: coronal mass ejection
7
Aspect ratio
6
Boundary layer flow
6
Clouds
6
Dynamical evolution
6
Expansion
6
Flux ropes
6
Global quantities
6
Helicities
6
In-situ observations
6
Magnetic clouds
6
Magnetic configuration
6
Magnetic flux ropes
6
Magnetic structure
6
Magnetohydrodynamics
6
Magnetoplasma
6
Planetary surface analysis
6
-
1“... interplanetary coronal mass ejection (ICME) is detected. Aims. The main aim of this study is to constrain...”
JOUR -
2“... dynamical laws, which are mainly dominated by magnetic forces.Aims. With in-situ observations the magnetic...”
Artículo publishedVersion -
3“... dynamical laws, which are mainly dominated by magnetic forces.Aims. With in-situ observations the magnetic...”
Artículo publishedVersion -
4por Démoulin, P., Dasso, S.“... dynamical laws, which are mainly dominated by magnetic forces.Aims. With in-situ observations the magnetic...”
JOUR -
5por Mandrini, C.H., Pohjolainen, S., Dasso, S., Green, L.M., Démoulin, P., Van Driel-Gesztelyi, L., Copperwheat, C., Foley, C.“... structure, observed mainly in EUV, and we found a very high level of non-potentiality in the modelled...”
Publicado 2005
Artículo publishedVersion -
6“... that the decrease of the total SW pressure with distance is the main origin of the observed MC expansion rate. We...”
Artículo publishedVersion -
7“.... The timing of the first high-energy particle arrival on Earth is mainly determined by the type of IMF...”
Artículo publishedVersion -
8“... and in situ data do not provide any direct estimation of the general flux rope properties. Aims. The main aim...”
Artículo publishedVersion -
9por Mandrini, C.H., Pohjolainen, S., Dasso, S., Green, L.M., Démoulin, P., Van Driel-Gesztelyi, L., Copperwheat, C., Foley, C.“... structure, observed mainly in EUV, and we found a very high level of non-potentiality in the modelled...”
Publicado 2005
Artículo publishedVersion -
10“... that the decrease of the total SW pressure with distance is the main origin of the observed MC expansion rate. We...”
Artículo publishedVersion -
11“.... The timing of the first high-energy particle arrival on Earth is mainly determined by the type of IMF...”
Artículo publishedVersion -
12“... and in situ data do not provide any direct estimation of the general flux rope properties. Aims. The main aim...”
Artículo publishedVersion -
13“... and in situ data do not provide any direct estimation of the general flux rope properties. Aims. The main aim...”
JOUR -
14“.... The timing of the first high-energy particle arrival on Earth is mainly determined by the type of IMF...”
JOUR -
15“... that the decrease of the total SW pressure with distance is the main origin of the observed MC expansion rate. We...”
JOUR -
16por Mandrini, C.H., Pohjolainen, S., Dasso, S., Green, L.M., Démoulin, P., Van Driel-Gesztelyi, L., Copperwheat, C., Foley, C.“... structure, observed mainly in EUV, and we found a very high level of non-potentiality in the modelled...”
JOUR -
17“... and mainly determined by their own magnetic forces and the interaction with the surrounding solar wind. Aims...”
Artículo publishedVersion -
18“... and mainly determined by their own magnetic forces and the interaction with the surrounding solar wind. Aims...”
Artículo publishedVersion -
19“... and mainly determined by their own magnetic forces and the interaction with the surrounding solar wind. Aims...”
JOUR