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Sun: coronal mass ejections (CMEs)
27
Magnetic fields
20
Solar wind
19
Sun: magnetic fields
14
Magnetic flux
13
Sun: coronal mass ejection
13
Coronal mass ejection
12
Interplanetary spacecraft
12
Magnetic clouds
12
Astrophysics
11
Flux ropes
10
Interplanetary medium
10
Magnetohydrodynamics
10
Solar system
10
Sun
9
Rope
8
Magnetic flux ropes
7
Magnetic structure
7
Minimum variance
7
Spacecraft
7
Sun: heliosphere
7
Boundary layer flow
6
Expansion rate
6
In-situ observations
6
Magnetic helicity
6
Self-similar
6
Solar-terrestrial relations
6
Sun: corona
6
Velocity
6
interplanetary medium
6
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1“...Magnetic clouds (MCs) are highly magnetized plasma structures that have a low proton temperature...”
JOUR -
2“... of the local flux-rope parameters such as its radius and orientation. Since the flux-rope distributions have a...”
JOUR -
3“... with constant current. We have fitted the set of free parameters for the six cases and have found that the two...”
JOUR -
4“... monitors. Results. We find that slow MCs at 1 AU have on average more massive sheaths. We conclude...”
JOUR -
5“... using a minimum variance analysis (MVA), and have identified a small number of MCs within which multiple...”
JOUR -
6“... hours, with a radius typically less than 0.1 AU, larger FRs, or magnetic clouds (hereafter, MCs), have...”
JOUR -
7“... rope axis and shock surface have several potential applications. First, these shapes can be used...”
INPR -
8por Dasso, S., Asorey, H.“... monitors or muon detectors, have been recording the variability of the cosmic ray flux at ground level...”
JOUR -
9“...Theoretical models of magnetic reconnection have been traditionally developed within the framework...”
JOUR -
10“... considering four different theoretical configurations (two force free and two non-force free) that have been...”
JOUR -
11“... rope axis and shock surface have several potential applications. First, these shapes can be used...”
JOUR -
12“... considering four different theoretical configurations (two force free and two non-force free) that have been...”
Artículo publishedVersion -
13“... near their apex can only be rare cases. Next, the sheath thickness and the ICME velocity have no global...”
JOUR -
14“... considering four different theoretical configurations (two force free and two non-force free) that have been...”
Artículo publishedVersion -
15“... ejections (CMEs). Some of these ejections are detected in the solar wind as magnetic clouds (MCs) that have...”
JOUR -
16por Démoulin, P., Dasso, S.“..., such as the internal over-pressure, the radial distribution, and the amount of twist within the flux rope have a much...”
JOUR -
17“... the typical three-part structure. These events have been also observed by SOHO/UVCS, allowing us to infer...”
CONF -
18“... angle, and a non force-free model with constant current. We have fitted the set of free parameters...”
CONF -
19“..., such as the internal over-pressure, the radial distribution, and the amount of twist within the flux rope have a much...”
Artículo publishedVersion -
20“... ejections (CMEs). Some of these ejections are detected in the solar wind as magnetic clouds (MCs) that have...”
Artículo publishedVersion