Materias dentro de su búsqueda.
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Magnetic fields
Solar wind
17
Interplanetary spacecraft
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Sun
15
Sun: coronal mass ejections (CMEs)
14
Coronal mass ejection
13
Astrophysics
12
Magnetic flux
12
Sun: heliosphere
12
Solar system
11
Flux ropes
10
Magnetic clouds
10
Magnetic structure
10
Magnetohydrodynamics
10
Sun: coronal mass ejection
10
Sun: magnetic fields
10
Boundary layer flow
9
Expansion
9
In-situ observations
9
Interplanetary medium
9
Magnetic flux ropes
9
Interplanetary coronal mass ejections
8
Solar-terrestrial relations
8
High-energy particles
7
Magnetoplasma
7
Planetary surface analysis
7
Solar energy
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Aspect ratio
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Clouds
6
Dynamical evolution
6
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1“... concentrations of magnetic flux, by "peculiar" we mean regions in which the main polarities rotate one around...”
CONF -
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 -
3“... of this work is to find the main causes of this expansion and to derive a model to explain the plasma velocity...”
Artículo publishedVersion -
4por 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 -
5“... interplanetary coronal mass ejection (ICME) is detected. Aims. The main aim of this study is to constrain...”
JOUR -
6“... dynamical laws, which are mainly dominated by magnetic forces.Aims. With in-situ observations the magnetic...”
Artículo publishedVersion -
7“... dynamical laws, which are mainly dominated by magnetic forces.Aims. With in-situ observations the magnetic...”
Artículo publishedVersion -
8por Démoulin, P., Dasso, S.“... dynamical laws, which are mainly dominated by magnetic forces.Aims. With in-situ observations the magnetic...”
JOUR -
9“... the observed CME activity in specific cases. The main candidates being differential rotation, shear motions...”
JOUR -
10por 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 -
11“..., such bright patches are not observed before the main flare, they are only observed after it.3.On October 28...”
JOUR -
12“... emerged in between the two main polarities and arch filament systems (AFS) were observed to be linked...”
JOUR -
13por 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 -
14“... and shearing photospheric motions towards the main magnetic inversion line. The large scale quadrupolar...”
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15“...We study the long term evolution of a set of 22 bipolar active regions (ARs) in which the main...”
JOUR -
16por Mandrini, C.H., Nuevo, F.A., Vásquez, A.M., Démoulin, P., van Driel-Gesztelyi, L., Baker, D., Culhane, J.L., Cristiani, G.D., Pick, M.“... and be released into the SW via magnetic reconnection, which occurs in at least two main steps. We analyse data...”
JOUR -
17“... that the decrease of the total SW pressure with distance is the main origin of the observed MC expansion rate. We...”
Artículo publishedVersion -
18“.... The timing of the first high-energy particle arrival on Earth is mainly determined by the type of IMF...”
Artículo publishedVersion -
19“... and in situ data do not provide any direct estimation of the general flux rope properties. Aims. The main aim...”
Artículo publishedVersion -
20“... that the decrease of the total SW pressure with distance is the main origin of the observed MC expansion rate. We...”
Artículo publishedVersion