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Sun: coronal mass ejections (CMEs)
Magnetic fields
14
Magnetic clouds
11
Interplanetary spacecraft
10
Magnetic flux
10
Coronal mass ejection
9
Flux ropes
9
In-situ observations
9
Magnetic flux ropes
9
Solar wind
9
Sun
8
Sun: coronal mass ejection
8
Sun: heliosphere
8
Astrophysics
7
Solar system
7
Sun: magnetic fields
7
Aspect ratio
6
Boundary layer flow
6
Dynamical evolution
6
Expansion
6
Expansion rate
6
Global quantities
6
Helicities
6
Interplanetary medium
6
Magnetic configuration
6
Magnetic energies
6
Magnetic structure
6
Magnetohydrodynamics
6
Planetary surface analysis
6
Solar source
6
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1“... of this work is to find the main causes of this expansion and to derive a model to explain the plasma velocity...”
Artículo publishedVersion -
2“... of this work is to find the main causes of this expansion and to derive a model to explain the plasma velocity...”
Artículo publishedVersion -
3por Démoulin, P., Dasso, S.“... of this work is to find the main causes of this expansion and to derive a model to explain the plasma velocity...”
JOUR -
4“... interplanetary coronal mass ejection (ICME) is detected. Aims. The main aim of this study is to constrain...”
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5“... dynamical laws, which are mainly dominated by magnetic forces.Aims. With in-situ observations the magnetic...”
Artículo publishedVersion -
6“... dynamical laws, which are mainly dominated by magnetic forces.Aims. With in-situ observations the magnetic...”
Artículo publishedVersion -
7por Démoulin, P., Dasso, S.“... dynamical laws, which are mainly dominated by magnetic forces.Aims. With in-situ observations the magnetic...”
JOUR -
8por Harra, L.K., Démoulin, P., Mandrini, C.H., Matthews, S.A., Van Driel-Gesztelyi, L., Culhane, J.L., Fletcher, L.“... the main phase, the ongoing magnetic reconnection is demonstrated by upflows located at the edges...”
JOUR -
9por Démoulin, P., Mandrini, C.H., Van Driel-Gesztelyi, L., Thompson, B.J., Plunkett, S., Kovári, Zs., Aulanier, G., Young, A.“... as the studied AR and n number of turns in the interval [0.5, 2.0]. We suggest that the main source of helicity...”
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10“... and in situ data do not provide any direct estimation of the general flux rope properties. Aims. The main aim...”
Artículo publishedVersion -
11“... and in situ data do not provide any direct estimation of the general flux rope properties. Aims. The main aim...”
Artículo publishedVersion -
12“... and in situ data do not provide any direct estimation of the general flux rope properties. Aims. The main aim...”
JOUR -
13“... determination of the FR axis orientation. The main remaining bias is moderate (lower than 6°) and is present...”
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14“... and mainly determined by their own magnetic forces and the interaction with the surrounding solar wind. Aims...”
Artículo publishedVersion -
15“... and mainly determined by their own magnetic forces and the interaction with the surrounding solar wind. Aims...”
Artículo publishedVersion -
16“... and mainly determined by their own magnetic forces and the interaction with the surrounding solar wind. Aims...”
JOUR