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Astrophysics
Magnetic fields
12
Sun
12
Sun: magnetic fields
12
Magnetic flux
11
Boundary layer flow
9
Coronal mass ejection
9
Interplanetary spacecraft
9
Solar wind
9
Flux ropes
7
Magnetic clouds
7
Magnetic structure
7
Sun: coronal mass ejections (CMEs)
7
Expansion
6
In-situ observations
6
Interplanetary medium
6
Magnetic flux ropes
6
Magnetohydrodynamics
6
Semiconductor counters
6
Velocity
6
Coronal mass ejections (CME)
4
Magnetic field effects
4
Magnetic helicity
4
Sun: corona
4
Sun: coronal mass ejection
4
X rays
4
Arbitrary cross section
3
Aspect ratio
3
Boundary pressure
3
Boundary shapes
3
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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“... dynamical laws, which are mainly dominated by magnetic forces.Aims. With in-situ observations the magnetic...”
Artículo publishedVersion -
5“... dynamical laws, which are mainly dominated by magnetic forces.Aims. With in-situ observations the magnetic...”
Artículo publishedVersion -
6por Démoulin, P., Dasso, S.“... dynamical laws, which are mainly dominated by magnetic forces.Aims. With in-situ observations the magnetic...”
JOUR -
7por Mandrini, C.H., López Fuentes, M.C., Démoulin, P., Van Driel-Gesztelyi, L., Pevtsov, A.A., Sawaya-Lacoste H.“...We study the long term evolution of a set of bipolar active regions (ARs) in which the main...”
CONF -
8por van Driel-Gesztelyi, L., Goff, C.P., Démoulin, P., Culhane, J.L., Matthews, S.A., Harra, L.K., Mandrini, C.H., Klein, K.-L., Kurokawa, H.“... main conclusions. First, we link the first two impulsive flares to tether-cutting reconnections...”
JOUR -
9“...We study the long term evolution of a set of 22 bipolar active regions (ARs) in which the main...”
JOUR -
10por 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...”
JOUR -
11por 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 -
12“... that the decrease of the total SW pressure with distance is the main origin of the observed MC expansion rate. We...”
Artículo publishedVersion -
13por 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 -
14“... that the decrease of the total SW pressure with distance is the main origin of the observed MC expansion rate. We...”
Artículo publishedVersion -
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