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41por 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 -
42por 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 -
43“... that the decrease of the total SW pressure with distance is the main origin of the observed MC expansion rate. We...”
Artículo publishedVersion -
44“.... The timing of the first high-energy particle arrival on Earth is mainly determined by the type of IMF...”
Artículo publishedVersion -
45“... and in situ data do not provide any direct estimation of the general flux rope properties. Aims. The main aim...”
Artículo publishedVersion -
46por 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 -
47“... that the decrease of the total SW pressure with distance is the main origin of the observed MC expansion rate. We...”
Artículo publishedVersion -
48“.... The timing of the first high-energy particle arrival on Earth is mainly determined by the type of IMF...”
Artículo publishedVersion -
49“... and in situ data do not provide any direct estimation of the general flux rope properties. Aims. The main aim...”
Artículo publishedVersion -
50“... durations of about half a day. The main aim of this study is to compare the properties of both populations...”
JOUR -
51“... and in situ data do not provide any direct estimation of the general flux rope properties. Aims. The main aim...”
JOUR -
52“.... The timing of the first high-energy particle arrival on Earth is mainly determined by the type of IMF...”
JOUR -
53“... that the decrease of the total SW pressure with distance is the main origin of the observed MC expansion rate. We...”
JOUR -
54por Mandrini, C.H., Démoulin, P., Bagala, L.G., Van Driel-Gesztelyi, L., Hénoux, J.C., Schmieder, B., Rovira, M.G.“...A conventional view of magnetic reconnection is mainly based on the 2-D picture of an X-type...”
JOUR -
55por López Fuentes, M., Mandrini, C.H., Poisson, M., Démoulin, P., Cristiani, G., López, F.M., Luoni, M.L.“... linking the main AR polarities. By analyzing the magnetic topology using a force-free model of the coronal...”
JOUR -
56por 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 -
57“...) decreases. Aims. The main aims of this paper are to find common plasma and magnetic properties of different...”
JOUR -
58“... determination of the FR axis orientation. The main remaining bias is moderate (lower than 6°) and is present...”
JOUR -
59“... and mainly determined by their own magnetic forces and the interaction with the surrounding solar wind. Aims...”
Artículo publishedVersion -
60“... and mainly determined by their own magnetic forces and the interaction with the surrounding solar wind. Aims...”
Artículo publishedVersion